Author: "S. Perasso" - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"S. Perasso"' showing total 64 results

Start Over Author "S. Perasso"

64 results on '"S. Perasso"'

1. The Double Chooz antineutrino detectors

Author: H. de Kerret, Y. Abe, C. Aberle, T. Abrahão, J. M. Ahijado, T. Akiri, J. M. Alarcón, J. Alba, H. Almazan, J. C. dos Anjos, S. Appel, F. Ardellier, I. Barabanov, J. C. Barriere, E. Baussan, A. Baxter, I. Bekman, M. Bergevin, A. Bernstein, W. Bertoli, T. J. C. Bezerra, L. Bezrukov, C. Blanco, N. Bleurvacq, E. Blucher, H. Bonet, M. Bongrand, N. S Bowden, T. Brugière, C. Buck, M. Buizza Avanzini, J. Busenitz, A. Cabrera, E. Caden, E. Calvo, L. Camilleri, R. Carr, S. Cazaux, J. M. Cela, M. Cerrada, P. J. Chang, P. Charon, E. Chauveau, P. Chimenti, T. Classen, A. P. Collin, E. Conover, J. M Conrad, S. Cormon, O. Corpace, B. Courty, J. I. Crespo-Anadón, M. Cribier, K. Crum, S. Cuadrado, A. Cucoanes, M. D’Agostino, E. Damon, J. V. Dawson, S. Dazeley, M. Dierckxsens, D. Dietrich, Z. Djurcic, F. Dorigo, M. Dracos, V. Durand, Y. Efremeko, M. Elnimr, A. Etenko, E. Falk, M. Fallot, M. Fechner, J. Felde, S. M. Fernandes, C. Fernández-Bedoya, D. Francia, D. Franco, V. Fischer, A. J. Franke, M. Franke, H. Furuta, F. Garcia, J. Garcia, I. Gil-Botella, L. Giot, A. Givaudan, M. Göger-Neff, H. Gomez, L. F. G. Gonzalez, L. Goodenough, M. C. Goodman, J. Goon, B. Gramlich, D. Greiner, A. Guertin, B. Guillon, S. M. Habib, Y. Haddad, T. Hara, F. X. Hartmann, J. Hartnell, J. Haser, A. Hatzikoutelis, D. Hellwig, S. Hervé, R. Hofacker, G. Horton-Smith, A. Hourlier, M. Ishitsuka, K. Jänner, S. Jiménez, J. Jochum, C. Jollet, F. Kaether, K. Kale, L. Kalousis, Y. Kamyshkov, M. Kaneda, D. M. Kaplan, M. Karakac, T. Kawasaki, E. Kemp, Y. Kibe, T. Kirchner, T. Konno, D. Kryn, T. Kutter, M. Kuze, T. Lachenmaier, C. E. Lane, C. Langbrandtner, T. Lasserre, C. Lastoria, L. Latron, C. Leonardo, A. Letourneau, D. Lhuillier, H. P. Lima, M. Lindner, J. M. López-Castaño, J. M. LoSecco, B. Lubsandorzhiev, S. Lucht, J. Maeda, C. N. Maesano, C. Mariani, J. Maricic, F. Marie, J. J. Martinez, J. Martino, T. Matsubara, D. McKee, F. Meigner, G. Mention, A. Meregaglia, J. P. Meyer, T. Miletic, R. Milincic, J. F. Millot, A. Minotti, V. Mirones, H. Miyata, Th. A. Mueller, Y. Nagasaka, K. Nakajima, D. Navas-Nicolás, Y. Nikitenko, P. Novella, L. Oberauer, M. Obolensky, A. Onillon, A. Oralbaev, I. Ostrovskiy, C. Palomares, S. J. M. Peeters, I. M. Pepe, S. Perasso, P. Perrin, P. Pfahler, A. Porta, G. Pronost, J. C. Puras, R. Quéval, J. L. Ramirez, J. Reichenbacher, B. Reinhold, M. Reissfelder, A. Remoto, D. Reyna, I. Rodriguez, M. Röhling, R. Roncin, N. Rudolf, B. Rybolt, Y. Sakamoto, R. Santorelli, F. Sato, U. Schwan, S. Schönert, S. Schoppmann, L. Scola, M. Settimo, M. A. Shaevitz, R. Sharankova, V. Sibille, J.-L. Sida, V. Sinev, D. Shrestha, M. Skorokhvatov, P. Soldin, J. Spitz, A. Stahl, I. Stancu, P. Starzynski, M. R. Stock, L. F. F. Stokes, M. Strait, A. Stüken, F. Suekane, S. Sukhotin, T. Sumiyoshi, Y. Sun, Z. Sun, R. Svoboda, H. Tabata, N. Tamura, K. Terao, A. Tonazzo, F. Toral, M. Toups, H. Trinh Thi, F. Valdivia, G. Valdiviesso, N. Vassilopoulos, A. Verdugo, C. Veyssiere, B. Viaud, D. Vignaud, M. Vivier, S. Wagner, C. Wiebusch, B. White, L. Winslow, M. Worcester, M. Wurm, J. Wurtz, G. Yang, J. Yáñez, F. Yermia, and K. Zbiri
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract This article describes the setup and performance of the near and far detectors in the Double Chooz experiment. The electron antineutrinos of the Chooz nuclear power plant were measured in two identically designed detectors with different average baselines of about 400 m and 1050 m from the two reactor cores. Over many years of data taking the neutrino signals were extracted from interactions in the detectors with the goal of measuring a fundamental parameter in the context of neutrino oscillation, the mixing angle $$\theta _{13}$$ θ 13 . The central part of the Double Chooz detectors was a main detector comprising four cylindrical volumes filled with organic liquids. From the inside towards the outside there were volumes containing gadolinium-loaded scintillator, gadolinium-free scintillator, a buffer oil and, optically separated, another liquid scintillator acting as veto system. Above this main detector an additional outer veto system using plastic scintillator strips was installed. The technologies developed in Double Chooz were inspiration for several other antineutrino detectors in the field. The detector design allowed implementation of efficient background rejection techniques including use of pulse shape information provided by the data acquisition system. The Double Chooz detectors featured remarkable stability, in particular for the detected photons, as well as high radiopurity of the detector components.
Published: 2022
Full Text: View/download PDF

2. First results from the DarkSide-50 dark matter experiment at Laboratori Nazionali del Gran Sasso

Author: P. Agnes, T. Alexander, A. Alton, K. Arisaka, H.O. Back, B. Baldin, K. Biery, G. Bonfini, M. Bossa, A. Brigatti, J. Brodsky, F. Budano, L. Cadonati, F. Calaprice, N. Canci, A. Candela, H. Cao, M. Cariello, P. Cavalcante, A. Chavarria, A. Chepurnov, A.G. Cocco, L. Crippa, D. D'Angelo, M. D'Incecco, S. Davini, M. De Deo, A. Derbin, A. Devoto, F. Di Eusanio, G. Di Pietro, E. Edkins, A. Empl, A. Fan, G. Fiorillo, K. Fomenko, G. Forster, D. Franco, F. Gabriele, C. Galbiati, A. Goretti, L. Grandi, M. Gromov, M.Y. Guan, Y. Guardincerri, B. Hackett, K. Herner, E.V. Hungerford, Al. Ianni, An. Ianni, C. Jollet, K. Keeter, C. Kendziora, S. Kidner, V. Kobychev, G. Koh, D. Korablev, G. Korga, A. Kurlej, P.X. Li, B. Loer, P. Lombardi, C. Love, L. Ludhova, S. Luitz, Y.Q. Ma, I. Machulin, A. Mandarano, S. Mari, J. Maricic, L. Marini, C.J. Martoff, A. Meregaglia, E. Meroni, P.D. Meyers, R. Milincic, D. Montanari, A. Monte, M. Montuschi, M.E. Monzani, P. Mosteiro, B. Mount, V. Muratova, P. Musico, A. Nelson, S. Odrowski, M. Okounkova, M. Orsini, F. Ortica, L. Pagani, M. Pallavicini, E. Pantic, L. Papp, S. Parmeggiano, R. Parsells, K. Pelczar, N. Pelliccia, S. Perasso, A. Pocar, S. Pordes, D. Pugachev, H. Qian, K. Randle, G. Ranucci, A. Razeto, B. Reinhold, A. Renshaw, A. Romani, B. Rossi, N. Rossi, S.D. Rountree, D. Sablone, P. Saggese, R. Saldanha, W. Sands, S. Sangiorgio, E. Segreto, D. Semenov, E. Shields, M. Skorokhvatov, O. Smirnov, A. Sotnikov, C. Stanford, Y. Suvorov, R. Tartaglia, J. Tatarowicz, G. Testera, A. Tonazzo, E. Unzhakov, R.B. Vogelaar, M. Wada, S. Walker, H. Wang, Y. Wang, A. Watson, S. Westerdale, M. Wojcik, A. Wright, X. Xiang, J. Xu, C.G. Yang, J. Yoo, S. Zavatarelli, A. Zec, C. Zhu, and G. Zuzel
Subjects: Physics, QC1-999
Abstract: We report the first results of DarkSide-50, a direct search for dark matter operating in the underground Laboratori Nazionali del Gran Sasso (LNGS) and searching for the rare nuclear recoils possibly induced by weakly interacting massive particles (WIMPs). The dark matter detector is a Liquid Argon Time Projection Chamber with a (46.4±0.7) kg active mass, operated inside a 30 t organic liquid scintillator neutron veto, which is in turn installed at the center of a 1 kt water Cherenkov veto for the residual flux of cosmic rays. We report here the null results of a dark matter search for a (1422±67) kgd exposure with an atmospheric argon fill. This is the most sensitive dark matter search performed with an argon target, corresponding to a 90% CL upper limit on the WIMP-nucleon spin-independent cross section of 6.1×10−44 cm2 for a WIMP mass of 100 Gev/c2. Keywords: Dark matter, WIMP, Noble liquid detectors, Low-background detectors, Liquid scintillators
Published: 2015
Full Text: View/download PDF

3. The DarkSide Multiton Detector for the Direct Dark Matter Search

Author: C. E. Aalseth, P. Agnes, A. Alton, K. Arisaka, D. M. Asner, H. O. Back, B. Baldin, K. Biery, G. Bonfini, M. Bossa, A. Brigatti, J. Brodsky, F. Budano, L. Cadonati, M. Cadoni, F. Calaprice, N. Canci, A. Candela, H. Cao, M. Cariello, P. Cavalcante, A. Chepurnov, A. G. Cocco, C. Condon, L. Crippa, D. D’Angelo, M. D’Incecco, S. Davini, M. De Deo, A. Derbin, A. Devoto, F. Di Eusanio, E. Edkins, A. Empl, A. Fan, G. Fiorillo, K. Fomenko, G. Forster, M. Foxe, D. Franco, F. Gabriele, C. Galbiati, A. Goretti, L. Grandi, M. Gromov, M. Y. Guan, Y. Guardincerri, B. Hackett, K. Herner, A. Hime, P. Humble, E. Hungerford, Al. Ianni, An. Ianni, D. E. Jaffe, C. Jollet, K. Keeter, C. Kendziora, S. Kidner, V. Kobychev, G. Koh, D. Korablev, G. Korga, A. Kurlej, P. X. Li, M. Lissia, P. Lombardi, L. Ludhova, S. Luitz, G. Lukyachenko, Y. Q. Ma, I. Machulin, A. Mandarano, S. M. Mari, J. Maricic, L. Marini, D. Markov, J. Martoff, A. Meregaglia, E. Meroni, P. D. Meyers, T. Miletic, R. Milincic, M. Montuschi, M. E. Monzani, P. Mosteiro, B. Mount, V. Muratova, P. Musico, D. Montanari, A. Nelson, S. Odrowski, A. Odrzywolek, J. L. Orrell, M. Orsini, F. Ortica, L. Pagani, M. Pallavicini, E. Pantic, S. Parmeggiano, B. Parsells, K. Pelczar, N. Pelliccia, S. Perasso, L. Perasso, A. Pocar, S. Pordes, D. Pugachev, H. Qian, K. Randle, G. Ranucci, A. Razeto, K. Recine, B. Reinhold, A. Renshaw, A. Romani, N. Rossi, B. Rossi, S. D. Rountree, D. Sablone, P. Saggese, R. Saldanha, W. Sands, S. Sangiorgio, E. Segreto, D. Semenov, E. Shields, M. Skorokhvatov, M. Smallcomb, O. Smirnov, A. Sotnikov, Y. Suvurov, R. Tartaglia, J. Tatarowicz, G. Testera, A. Tonazzo, E. Unzhakov, R. B. Vogelaar, M. Wada, S. E. Walker, H. Wang, Y. Wang, A. W. Watson, S. Westerdale, R. Williams, M. Wojcik, J. Xu, C. G. Yang, J. Yoo, B. Yu, S. Zavatarelli, W. L. Zhong, and G. Zuzel
Subjects: Physics, QC1-999
Abstract: Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (
Published: 2015
Full Text: View/download PDF

4. First results from the DarkSide-50 dark matter experiment at Laboratori Nazionali del Gran Sasso

Author: S. Kidner, R. Tartaglia, A. L. Renshaw, E. V. Hungerford, Yanchu Wang, P. Cavalcante, A. Candela, C. Zhu, M. Cariello, S. Westerdale, A. Sotnikov, Samuele Sangiorgio, E. Shields, N. Rossi, F. Gabriele, E. Pantic, L. Crippa, D. Sablone, An. Ianni, V. N. Muratova, G. Testera, M. D. Skorokhvatov, L. Grandi, G. Forster, A. Devoto, A. E. Chavarria, K. Pelczar, K. Fomenko, Cristiano Galbiati, M. Wada, C. Love, G. Di Pietro, Min-Xin Guan, R. B. Vogelaar, Laura Cadonati, L. Papp, Y. Guardincerri, Gioacchino Ranucci, E. Edkins, P. Musico, K. Herner, M. E. Monzani, S. D. Rountree, P. J. Mosteiro, B. Baldin, Hui Wang, R. Parsells, G. Bonfini, A. Pocar, Thomas Alexander, Y. Q. Ma, Fausto Ortica, B. Rossi, K. Randle, P. Saggese, L. Marini, M. Bossa, N. Canci, Paolo Lombardi, B. R. Hackett, A. Empl, R. Saldanha, K. Arisaka, Henning O. Back, Stuart Derek Walker, M. Montuschi, M. Orsini, E. Meroni, Jilei Xu, A. Zec, O. Smirnov, D. Franco, G. Fiorillo, A. Monte, M. Okounkova, G. Zuzel, Alan Watson, J. Yoo, C. L. Kendziora, F. Di Eusanio, A. Razeto, L. Pagani, M. D'Incecco, J. Tatarowicz, D. Korablev, M. De Deo, A. V. Derbin, Nicomede Pelliccia, I. N. Machulin, B. Reinhold, Anselmo Meregaglia, H. Qian, S. Davini, E. Segreto, A. Wright, C. J. Martoff, A. Mandarano, Marcin Wójcik, S. Luitz, Marco Pallavicini, D. D'Angelo, K. J. Keeter, Frank Calaprice, F. Budano, X. Xiang, Sandra Zavatarelli, P. X. Li, V. V. Kobychev, W. Sands, Aldo Romani, B. Loer, M. Gromov, A. Tonazzo, S. Pordes, P. Agnes, Al. Ianni, G. Koh, J. Maricic, A. Nelson, G. Korga, Stefano Maria Mari, R. Milincic, Cécile Jollet, D. A. Semenov, A. Kurlej, S. Parmeggiano, K. Biery, A. Fan, D. A. Pugachev, S. Perasso, A. G. Cocco, A. K. Alton, B. J. Mount, Chung-Yao Yang, Augusto Brigatti, D. Montanari, E. V. Unzhakov, J. Brodsky, H. Cao, S. Odrowski, Peter Daniel Meyers, Y. Suvorov, Livia Ludhova, A. M. Goretti, A. S. Chepurnov, C. Stanford, Agnes, P, Alexander, T., Alton, A., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Cadonati, L., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Cavalcante, P., Chavarria, A., Chepurnov, A., Cocco, A. G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., De Deo, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Gromov, M., Guan, M. Y., Guardincerri, Y., Hackett, B., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., Jollet, C., Keeter, K., Kendziora, C., Kidner, S., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P. X., Loer, B., Lombardi, P., Love, C., Ludhova, L., Luitz, S., Ma, Y. Q., Machulin, I., Mandarano, A., Mari, S., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meroni, E., Meyers, P. D., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B., Muratova, V., Musico, P., Nelson, A., Odrowski, S., Okounkova, M., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Papp, L., Parmeggiano, S., Parsells, R., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Segreto, E., Semenov, D., Shields, E., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Walker, Susan Elizabeth, Wang, H., Wang, Y., Watson, A., Westerdale, S., Wojcik, M., Wright, A., Xiang, X., Xu, J., Yang, C. G., Yoo, J., Zavatarelli, S., Zec, A., Zhu, C., Zuzel, G., P. Agnes, Mari, Stefano Maria, and The Darkside, Collaboration
Subjects: Nuclear and High Energy Physics, Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Liquid scintillator, Physics - Instrumentation and Detectors, WIMP, Physics::Instrumentation and Detectors, low-background detectors, Dark matter, Noble liquid detectors, FOS: Physical sciences, liquid scintillators, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, WIMP Argon Programme, 01 natural sciences, dark matter, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Low-background detectors, 0103 physical sciences, Nuclear Experiment, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, ICARUS, Time projection chamber, 010308 nuclear & particles physics, Liquid scintillators, Dark matter WIMP Noble liquid detectors Low-background detectors Liquid scintillators, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), Low-background detector, noble liquid detectors, lcsh:QC1-999, DAMA/NaI, Weakly interacting massive particles, High Energy Physics::Experiment, Noble liquid detector, Astrophysics - Instrumentation and Methods for Astrophysics, lcsh:Physics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We report the first results of DarkSide-50, a direct search for dark matter operating in the underground Laboratori Nazionali del Gran Sasso (LNGS) and searching for the rare nuclear recoils possibly induced by weakly interacting massive particles (WIMPs). The dark matter detector is a Liquid Argon Time Projection Chamber with a (46.4+-0.7) kg active mass, operated inside a 30 t organic liquid scintillator neutron veto, which is in turn installed at the center of a 1 kt water Cherenkov veto for the residual flux of cosmic rays. We report here the null results of a dark matter search for a (1422+-67) kg d exposure with an atmospheric argon fill. This is the most sensitive dark matter search performed with an argon target, corresponding to a 90% CL upper limit on the WIMP-nucleon spin-independent cross section of 6.1x10^-44 cm^2 for a WIMP mass of 100 GeV/c^2., 26 pages, 7 figures; updated figures and references, notably Fig. 7 has updated CDMSII curve; fixed typos; clarified some language and figures; updated references
Published: 2015

5. Geo-neutrinos from 1353 Days with the Borexino Detector

Author: A.V. Etenko, D. Bravo, Caren Hagner, A. Pocar, Marcin Wójcik, O. Smirnov, K. Otis, P. Cavalcante, Y. Suvorov, Livia Ludhova, Aldo Romani, S. Gazzana, G. Lukyanchenko, G. Zuzel, A. V. Derbin, M. Misiaszek, A. M. Goretti, A. S. Chepurnov, P. J. Mosteiro, Lothar Oberauer, S. Manecki, Matthias Laubenstein, R. Saldanha, Denis Korablev, E. Litvinovich, N. Rossi, Marco Giammarchi, A. E. Chavarria, L. Perasso, F. von Feilitzsch, Fabio Mantovani, I. N. Machulin, Andrea Ianni, Alessandra Re, E. Meroni, D. Bick, Sandra Zavatarelli, Marco Pallavicini, M. D. Skorokhvatov, Michael Wurm, L. Grandi, D. D'Angelo, R. B. Vogelaar, Q. Meindl, Jingke Xu, Gioacchino Ranucci, C. Ghiano, Paolo Lombardi, Barbara Ricci, Cristiano Galbiati, G. Korga, A. Empl, S. Perasso, D. Kryn, Aldo Ianni, Lino Miramonti, T. Lewke, B. Caccianiga, V. N. Muratova, E. V. Hungerford, R. Tartaglia, M. Goeger-Neff, S. Schönert, Laura Cadonati, L. Papp, A. Sotnikov, C. Salvo, W. Maneschg, Fausto Ortica, G. Bellini, D. Vignaud, Giovanni Fiorentini, D. Franco, S. V. Sukhotin, M. Obolensky, G. Bonfini, M. Buizza Avanzini, A. Wright, O. Zaimidoroga, Frank Calaprice, Hardy Simgen, S. Davini, G. Testera, K. Fomenko, G. Manuzio, V. V. Kobychev, B. Loer, Yusuke Koshio, Jay Burton Benziger, F. Lombardi, A. Razeto, J. Winter, and A. A. Sabelnikov
Subjects: Physics, Nuclear physics, Physics and Astronomy (all), Detector, Ambientale, Physics and Astronomy(all), Mass ratio, Neutrino, Borexino
Abstract: We present a 1353 days measurement of the geo–neutrino flux in Borexino: the signal was found to be 14.3 ± 4.4 events. This result translates into S geo = (38.8 ± 12.0) TNU when a Th/U fixed chondritic mass ratio of 3.9 is assumed. Furthermore Borexino data are compatible with a mantle geo–neutrino signal of (15.4 ± 12.3) TNU.
Published: 2015

6. THE DARKSIDE-50 EXPERIMENT: A LIQUID ARGON TARGET FOR DARK MATTER PARTICLES

Author: R. Tartaglia, A. Razeto, B. R. Hackett, A. Zec, N. Canci, Thomas Alexander, S. Pordes, H. O. Back, M. Gromov, A. L. Renshaw, C. Giganti, A. Empl, S. De Cecco, Ivone F. M. Albuquerque, J. Tatarowicz, A. M. Goretti, J. Maricic, M. Cariello, Samuele Sangiorgio, D. Franco, M. Lissia, L. Crippa, G. Zuzel, A. Devoto, P. D. Meyers, W. Zhong, E. V. Hungerford, G. Di Pietro, J. P. Brodsky, B. Vogelaar, S. Westerdale, R. Milincic, Mariano Cadoni, N. Rossi, E. Pantic, J. Wilhelmi, M. Wada, L. Agostino, Nicomede Pelliccia, P. N. Singh, A. Sotnikov, M. E. Monzani, K. Arisaka, M. D. Skorokhvatov, B. Baldin, L. Grandi, A. Meregaglia, E. Edkins, L. Marini, M. Bossa, E. Shields, C. Stanford, G. Fiorillo, D. Rountree, G. Forster, M. Carlini, Gioacchino Ranucci, L. Pagani, P. Cavalcante, G. Koh, K. Randle, A. Vishneva, X. Li, Paolo Lombardi, B. Rossi, B. Reinhold, S. Bussino, A. Pocar, P. Trinchese, P. J. Mosteiro, Michele Montuschi, M. D'Incecco, M. De Vincenzi, E. Segreto, Alan Watson, An. Ianni, H. Qian, C. Jollet, C. J. Martoff, G. Bonfini, A. Mandarano, V. N. Muratova, M. Orsini, B. Bottino, K. Herner, B. J. Mount, K. J. Keeter, K. Biery, Yanchu Wang, G. Korga, K. Fomenko, Frank Calaprice, X. Xiang, F. Budano, V. V. Kobychev, P. Saggese, C. Savarese, Laura Cadonati, D. Sablone, F. Granato, A. Candela, J. Yoo, Jingke Xu, A. S. Kubankin, S. Davini, M. Cadeddu, T. Miletic, K. Pelczar, Fausto Ortica, Sandra Zavatarelli, W. Sands, Y. Guardincerri, Giovanni Covone, A. Monte, S. Luitz, Min-Xin Guan, Paolo Musico, D. Montanari, O. Smirnov, A. Fan, D. A. Pugachev, E. V. Unzhakov, Han Wang, R. Saldanha, Ann E. Nelson, I. N. Machulin, Al. Ianni, Caoxiang Zhu, Y. Suvorov, Stuart Derek Walker, S. Perasso, D. D'Angelo, Yanhui Ma, C. L. Kendziora, Irina James, M. De Deo, S. Catalanotti, A. G. Cocco, Marco Pallavicini, F. Gabriele, F. Di Eusanio, M. M. Wojcik, Jim Napolitano, Aldo Romani, A. Tonazzo, P. Agnes, S. Parmeggiano, D. A. Semenov, Chung-Yao Yang, A. V. Derbin, Augusto Brigatti, Denis Korablev, A. K. Alton, C. Galbiati, S. M. Mari, A. S. Chepurnov, H. Cao, S. Odrowski, G. Testera, Alexander I. Studenikin, Agnes, P., Agostino, L., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, Federico, Bussino, Severino Angelo Maria, Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., Crippa, L., D’Angelo, D., D’Incecco, M., Davini, S., De Cecco, S., De Deo, M., DE VINCENZI, Mario, Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., James, Irina, Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, Stefano Maria, Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Nelson, A., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Romani, A., Rossi, B., Rossi, N., Rountree, D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Budano, F., Bussino, S., D'Angelo, D., D'Incecco, M., de Cecco, S., de Deo, M., de Vincenzi, M., di Eusanio, F., di Pietro, G., Ianni, A., James, I., and Mari, S. M.
Subjects: Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Dark matter, scintillation counter: liquid, chemistry.chemical_element, WIMP Argon Programme, Scintillator, dark matter: direct detection, liquid argon: target, 7. Clean energy, Nuclear physics, Nuclear Experiment, Physics, Argon, Time projection chamber, shielding, background, Astronomy and Astrophysics, Gran Sasso, time projection chamber, dark matter: scattering, chemistry, Electromagnetic shielding, atmosphere, dark matter, argon, time projection chamber, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Directional Recoil Identification from Tracks, ArDM
Abstract: International audience; The DarkSide-50 experiment, located at the “Laboratori Nazionali del Gran Sasso (INFN)”, is based on low-radioactivity argon double phase time projection chamber, surrounded by an active liquid scintillator veto, designed for the zero background achievement. The liquid argon features sufficient self shielding and easy scalability to multi-tons scale. The impressive reduction of the 39Ar isotope (compared to the atmospheric argon), along with the excellent pulse shape discrimination, make this technology a possible candidate for the forthcoming generation of multi-ton Dark Matter experiments.
Published: 2017

7. Background-independent measurement of θ13 in Double Chooz

Author: Z. Djurcic, A. Stahl, M. Kuze, Christian Buck, B. Rybolt, J. Spitz, J. Maricic, Amanda Porta, H. de Kerret, D. Dietrich, R. Santorelli, J. M. López-Castaño, I. M. Pepe, P. Chimenti, Muriel Fallot, P. Novella, C. Grant, Yuri Kamyshkov, T. Matsubara, Y. Sakamoto, L. B. Bezrukov, M. Franke, J. Haser, A.C. Schilithz, V. Zimmer, A. Cucoanes, Florian Kaether, P.-J. Chang, I. Bekman, J. Felde, D. Franco, R. Carr, R. Sharankova, E. Kemp, N. Vassilopoulos, C. Mariani, J. C. dos Anjos, A.V. Etenko, J.V. Dawson, A. Minotti, Yoshio Abe, Josef Jochum, V. Sibille, J. M. LoSecco, M. D. Skorokhvatov, Michael Wurm, H. Watanabe, A. Stüken, F. Sato, F. von Feilitzsch, C. Palomares, I. Gil-Botella, A. Hourlier, Lydie Giot, Audrey Letourneau, E. Damon, M. Röhling, M. Vivier, D. Kryn, Sebastian Wagner, Anselmo Meregaglia, Y. Nikitenko, Daniel M. Kaplan, G. Yang, Marcos Cerrada, M. Elnimr, Manfred Lindner, H. P. Lima, Antoine Collin, J. Reichenbacher, Robert Svoboda, Eric Baussan, S. M. Fernandes, V. V. Sinev, Bayarto Lubsandorzhiev, Marcos Dracos, S. Schönert, T. Sumiyoshi, J. Busenitz, Kazuhiro Terao, Stefan Schoppmann, David Lhuillier, Lothar Oberauer, Thierry Lasserre, G. Mention, J. C. Barriere, L. Camilleri, M. Göger-Neff, M. Obolensky, S. Shimojima, Anatael Cabrera, F. Yermia, Christopher Wiebusch, G. A. Valdiviesso, I. Stancu, Michael Hofmann, Cécile Jollet, B. Reinhold, G. A. Horton-Smith, L. N. Kalousis, T.J.C. Bezerra, Matthew L Strait, H. H. Trinh Thi, M. C. Goodman, S. Roth, Yasushi Nagasaka, H. Furuta, M. H. Shaevitz, E. Conover, G. Pronost, A. Onillon, T. Kawasaki, S. Perasso, S. V. Sukhotin, A. Osborn, E. Smith, J. Maeda, J. Martino, N. Haag, Luis González, L. Goodenough, A. Tonazzo, E. Blucher, T. Miletic, Janet Conrad, R. Milincic, T. Konno, F. Suekane, L.F.F. Stokes, Tobias Lachenmaier, K. Nakajima, R. Roncin, Ying Sun, T. Hara, M. Bergevin, K. Crum, J. I. Crespo-Anadón, V. Fischer, S. Lucht, E. Chauveau, E. Caden, Masaki Ishitsuka, Lindley Winslow, P. Pfahler, C. E. Lane, and C. Veyssiere
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, 010308 nuclear & particles physics, Oscillation, CHOOZ, 7. Clean energy, 01 natural sciences, Nuclear physics, 13. Climate action, 0103 physical sciences, Modulation (music), Neutron, Neutrino, 010306 general physics, Neutrino oscillation, Charged current, Mixing (physics)
Abstract: The oscillation results published by the Double Chooz Collaboration in 2011 and 2012 rely on background models substantiated by reactor-on data. In this analysis, we present a background-model-independent measurement of the mixing angle θ13 by including 7.53 days of reactor-off data. A global fit of the observed antineutrino rates for different reactor power conditions is performed, yielding a measurement of both θ13 and the total background rate. The results on the mixing angle are improved significantly by including the reactor-off data in the fit, as it provides a direct measurement of the total background rate. This reactor rate modulation analysis considers antineutrino candidates with neutron captures on both Gd and H, whose combination yields sin2(2θ13)=0.102±0.028(stat.)±0.033(syst.). The results presented in this study are fully consistent with the ones already published by Double Chooz, achieving a competitive precision. They provide, for the first time, a determination of θ13 that does not depend on a background model.
Published: 2014

8. First measurement of θ13 from delayed neutron capture on hydrogen in the Double Chooz experiment

Author: J. Maricic, A. Onillon, S. Roth, S. M. Fernandes, J. M. LoSecco, Anselmo Meregaglia, A. Hatzikoutelis, Masahiro Kuze, Th. A. Mueller, R. Santorelli, H. H. Trinh Thi, L. Camilleri, T. Hayakawa, J. Tm. Goon, V. V. Sinev, W. Potzel, M. Franke, I. M. Pepe, P. Chimenti, Matthew L Strait, T. Konno, I. Gil-Botella, Z. Djurcic, T. Matsubara, M. Fechner, Robert Svoboda, R. Roncin, Ying Sun, F. Suekane, L.F.F. Stokes, J. M. López-Castaño, Michael Hofmann, M. Toups, G. Keefer, Muriel Fallot, T. Classen, Steven Dazeley, H. P. Lima, A.V. Etenko, D. Kryn, J.V. Dawson, Amanda Porta, M. Röhling, T. Hara, M. Elnimr, J. Busenitz, R. Carr, Florian Kaether, M. Worcester, J. Felde, D. Franco, I. Stancu, D. Greiner, H. Furuta, B. White, H. de Kerret, Stefan Schoppmann, A. Remoto, C. Aberle, A. Cucoanes, M. Göger-Neff, G. Mention, E. Damon, S. Perasso, J. Ebert, Sebastian Wagner, Manfred Lindner, F. Hartmann, C. Mariani, Antoine Collin, E. Blucher, Josef Jochum, Yasushi Nagasaka, V. Durand, Daniel M. Kaplan, I. Ostrovskiy, P. Novella, L. Bezrukhov, F. von Feilitzsch, G. Pronost, K. Nakajima, Cécile Jollet, B. Reinhold, C. Langbrandtner, Tobias Lachenmaier, Adam Bernstein, P. Perrin, J. Maeda, L. Goodenough, Lothar Oberauer, A. Letourneau, A. Tonazzo, P. Pfahler, C. E. Lane, V. Zimmer, T. Kawasaki, S. Lucht, V. Fischer, R. Milincic, T. Sumiyoshi, E. Caden, A. J. Franke, J. Martino, M. Bergevin, Masaki Ishitsuka, Lindley Winslow, K. Crum, A. Osborn, A. Stahl, J. L. Sida, J. I. Crespo-Anadón, J. Reichenbacher, J. C. dos Anjos, A. Stüken, F. Sato, Yoshio Abe, C. Veyssiere, D. Shrestha, Yuri Kamyshkov, D. McKee, J. Spitz, P.-J. Chang, Marcos Cerrada, Yu. Efremenko, Caren Hagner, M. D. Skorokhvatov, Michael Wurm, H. Watanabe, M. Obolensky, L. N. Kalousis, T.J.C. Bezerra, R. Gama, Bayarto Lubsandorzhiev, Thierry Lasserre, J. C. Barriere, Manuel Meyer, Marcos Dracos, S. V. Sukhotin, E. Smith, N. Haag, Anna Erickson, J. Haser, T. Miletic, S. Habib, D. Lhuillier, Y. Sakamoto, F. Yermia, Anatael Cabrera, E. Conover, C. L. Jones, M. H. Shaevitz, A. Hourlier, Lydie Giot, E. Kemp, S. Schönert, S. Shimojima, G. A. Horton-Smith, Luis González, Nathaniel Bowden, Thomas Schwetz, Janet Conrad, C. Palomares, Kazuhiro Terao, Christopher Wiebusch, G. A. Valdiviesso, M. C. Goodman, H. Miyata, Christian Buck, B. Rybolt, C. N. Maesano, and D. Dietrich
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, 010308 nuclear & particles physics, Flux, Photon energy, CHOOZ, 01 natural sciences, Nuclear physics, Neutron capture, Inverse beta decay, 0103 physical sciences, 010306 general physics, Neutrino oscillation, Delayed neutron, Charged current
Abstract: The Double Chooz experiment has determined the value of the neutrino oscillation parameter $\theta_{13}$ from an analysis of inverse beta decay interactions with neutron capture on hydrogen. This analysis uses a three times larger fiducial volume than the standard Double Chooz assessment, which is restricted to a region doped with gadolinium (Gd), yielding an exposure of 113.1 GW-ton-years. The data sample used in this analysis is distinct from that of the Gd analysis, and the systematic uncertainties are also largely independent, with some exceptions, such as the reactor neutrino flux prediction. A combined rate- and energy-dependent fit finds $\sin^2 2\theta_{13}=0.097\pm 0.034(stat.) \pm 0.034 (syst.)$, excluding the no-oscillation hypothesis at 2.0 \sigma. This result is consistent with previous measurements of $\sin^2 2\theta_{13}$.
Published: 2013

9. DarkSide-50, a background free experiment for dark matter searches

Author: P. Agnes, 1 T. Alexander, 2 A. Alton, 3 K. Arisaka, 4 H. O. Back, 5 B. Baldin, 6 K. Biery, 6 G. Bonfini, 7 M. Bossa, 8 A. Brigatti, 9 J. Brodsky, 5 F. Budano, 10 L. Cadonati, 2 F. Calaprice, 5 N. Canci, 4 A. Candela, 7 H. Cao, 5 M. Cariello, 11 P. Cavalcante, 7 A. Chavarria, 12 A. Chepurnov, 13 A. G. Cocco, 14 L. Crippa, 9 D. D’Angelo, 9 M. D’Incecco, 7 S. Davini, 15 M. De Deo, 7 A. Derbin, 16 A. Devoto, 17 F. Di Eusanio, 5 G. Di Pietro, 9 E. Edkins, 18 A. Empl, 15 A. Fan, 4 G. Fiorillo, 14 K. Fomenko, 19 G. Forster, 2 D. Franco, 1 F. Gabriele, 7 C. Galbiati, 5 A. Goretti, 5 L. Grandi, 12 M. Gromov, 13 M. Y. Guan, 20 Y. Guardincerri, 6 B. Hackett, 18 K. Herner, 6 E. V. Hungerford, 15 A.l. Ianni, 7 A.n. Ianni, 5 C. Jollet, 21 K. Keeter, 22 C. Kendziora, 6 S. Kidner, a. V. Kobychev, 24 G. Koh, 5 D. Korablev, 19 G. Korga, 15 A. Kurlej, 2 P. X. Li, 20 B. Loer, 5 P. Lombardi, 9 C. Love, 25 L. Ludhova, 9 S. Luitz, 26 Y. Q. Ma, 20 I. Machulin, 28 A. Mandarano, 10 J. Maricic, 18 L. Marini, 10 C. J. Martoff, 25 A. Meregaglia, 21 E. Meroni, 9 P. D. Meyers, 5 R. Milincic, 18 D. Montanari, 6 M. Montuschi, 7 M. E. Monzani, 26 P. Mosteiro, 5 B. Mount, 22 V. Muratova, 16 P. Musico, 11 A. Nelson, 5 S. Odrowski, 7 M. Okounkova, 5 M. Orsini, 7 F. Ortica, 29 L. Pagani, 11 M. Pallavicini, 11 E. Pantic, 4, 30 L. Papp, 23 S. Parmeggiano, 9 R. Parsells, 5 K. Pelczar, 31 N. Pelliccia, 29 S. Perasso, 1 A. Pocar, 2 S. Pordes, 6 D. Pugachev, 27 H. Qian, 5 K. Randle, 2 G. Ranucci, 9 A. Razeto, 7 B. Reinhold, 18 A. Renshaw, 4 A. Romani, 29 B. Rossi, 5, 14 N. Rossi, 7 S. D. Rountree, 23 D. Sablone, 15 P. Saggese, 7 R. Saldanha, 12 W. Sands, 5 S. Sangiorgio, 32 E. Segreto, 7 D. Semenov, 16 E. Shields, 5 M. Skorokhvatov, 28 O. Smirnov, 19 A. Sotnikov, 19 C. Stanford, 5 Y. Suvorov, 4 R. Tartaglia, 7 J. Tatarowicz, 25 G. Testera, 11 A. Tonazzo, 1 E. Unzhakov, 16 R. B. Vogelaar, 23 M. Wada, 5 S. Walker, 14 H. Wang, 4 Y. Wang, 20 A. Watson, 25 S. Westerdale, 5 M. Wojcik, 31 A. Wright, 5 X. Xiang, 5 J. Xu, 5 C. G. Yang, 20 J. Yoo, 6 S. Zavatarelli, 11 A. Zec, 2 C. Zhu, G. Zuzel31, MARI, Stefano Maria, P., Agne, 1 T., Alexander, 2 A., Alton, 3 K., Arisaka, 4 H. O., Back, 5 B., Baldin, 6 K., Biery, 6 G., Bonfini, 7 M., Bossa, 8 A., Brigatti, 9 J., Brodsky, 5 F., Budano, 10 L., Cadonati, 2 F., Calaprice, 5 N., Canci, 4 A., Candela, 7 H., Cao, 5 M., Cariello, 11 P., Cavalcante, 7 A., Chavarria, 12 A., Chepurnov, 13 A. G., Cocco, 14 L., Crippa, 9 D., D’Angelo, 9 M., D’Incecco, 7 S., Davini, 15 M., De Deo, 7 A., Derbin, 16 A., Devoto, 17 F., Di Eusanio, 5 G., Di Pietro, 9 E., Edkin, 18 A., Empl, 15 A., Fan, 4 G., Fiorillo, 14 K., Fomenko, 19 G., Forster, 2 D., Franco, 1 F., Gabriele, 7 C., Galbiati, 5 A., Goretti, 5 L., Grandi, 12 M., Gromov, 13 M. Y., Guan, 20 Y., Guardincerri, 6 B., Hackett, 18 K., Herner, 6 E. V., Hungerford, Ianni, 15 A. l., Ianni, 7 A. n., 5 C., Jollet, 21 K., Keeter, 22 C., Kendziora, 6 S., Kidner, a. V., Kobychev, 24 G., Koh, 5 D., Korablev, 19 G., Korga, 15 A., Kurlej, 2 P. X., Li, 20 B., Loer, 5 P., Lombardi, 9 C., Love, 25 L., Ludhova, 9 S., Luitz, 26 Y. Q., Ma, 20 I., Machulin, 28 A., Mandarano, Mari, Stefano Maria, 10 J., Maricic, 18 L., Marini, 10 C. J., Martoff, 25 A., Meregaglia, 21 E., Meroni, 9 P. D., Meyer, 5 R., Milincic, 18 D., Montanari, 6 M., Montuschi, 7 M. E., Monzani, 26 P., Mosteiro, 5 B., Mount, 22 V., Muratova, 16 P., Musico, 11 A., Nelson, 5 S., Odrowski, 7 M., Okounkova, 5 M., Orsini, 7 F., Ortica, 29 L., Pagani, 11 M., Pallavicini, 11 E., Pantic, 30 L., Papp, 23 S., Parmeggiano, 9 R., Parsell, 5 K., Pelczar, 31 N., Pelliccia, 29 S., Perasso, 1 A., Pocar, 2 S., Porde, 6 D., Pugachev, 27 H., Qian, 5 K., Randle, 2 G., Ranucci, 9 A., Razeto, 7 B., Reinhold, 18 A., Renshaw, 4 A., Romani, 29 B., Rossi, 14 N., Rossi, 7 S. D., Rountree, 23 D., Sablone, 15 P., Saggese, 7 R., Saldanha, 12 W., Sand, 5 S., Sangiorgio, 32 E., Segreto, 7 D., Semenov, 16 E., Shield, 5 M., Skorokhvatov, 28 O., Smirnov, 19 A., Sotnikov, 19 C., Stanford, 5 Y., Suvorov, 4 R., Tartaglia, 7 J., Tatarowicz, 25 G., Testera, 11 A., Tonazzo, 1 E., Unzhakov, 16 R. B., Vogelaar, 23 M., Wada, 5 S., Walker, 14 H., Wang, 4 Y., Wang, 20 A., Watson, 25 S., Westerdale, 5 M., Wojcik, 31 A., Wright, 5 X., Xiang, 5 J., Xu, 5 C. G., Yang, 20 J., Yoo, 6 S., Zavatarelli, 11 A., Zec, 2 C., Zhu, and G., Zuzel31
Subjects: Physics, Large Underground Xenon experiment, Physics::Instrumentation and Detectors, Hot dark matter, Dark matter, Scalar field dark matter, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Dark matter halo, Weakly interacting massive particles, Warm dark matter, Instrumentation, Light dark matter, Mathematical Physics
Abstract: The existence of dark matter is inferred from gravitational effects, but its nature remains a deep mystery. One possibility, motivated by considerations in elementary particle physics, is that dark matter consists of elementary particles, such as the hypothesized Weakly Interacting Massive Particles (WIMPs), with mass ~ 100 GeV and cross-section ~ 10−47 cm2, that can be gravitationally trapped inside our galaxy and revealed by their scattering on nuclei. It should be possible to detect WIMPs directly, as the orbital motion of the WIMPs composing the dark matter halo pervading the galaxy should result in WIMP-nucleus collisions of sufficient energy to be observable in the laboratory. The DarkSide-50 experiment is a direct WIMP search using a Liquid Argon Time Projection Chamber (LAr-TPC) with an active mass of 50 kg with a high sensitivity and an ultra-low background detector.
Published: 2014

10. First Results from the DarkSide-50 Dark Matter Experiment at Laboratori Nazionali del Gran Sasso

Author: P. Agnes, 1 T. Alexander, 2 A. Alton, 3 K. Arisaka, 4 H. O. Back, 5 B. Baldin, 6 K. Biery, 6 G. Bonfini, 7 M. Bossa, 8 A. Brigatti, 9 J. Brodsky, 5 F. Budano, 10 L. Cadonati, 2 F. Calaprice, 5 N. Canci, 4 A. Candela, 7 H. Cao, 5 M. Cariello, 11 P. Cavalcante, 7 A. Chavarria, 12 A. Chepurnov, 13 A. G. Cocco, 14 L. Crippa, 9 D. D’Angelo, 9 M. D’Incecco, 7 S. Davini, 15 M. De Deo, 7 A. Derbin, 16 A. Devoto, 17 F. Di Eusanio, 5 G. Di Pietro, 9 E. Edkins, 18 A. Empl, 15 A. Fan, 4 G. Fiorillo, 14 K. Fomenko, 19 G. Forster, 2 D. Franco, 1 F. Gabriele, 7 C. Galbiati, 5 A. Goretti, 5 L. Grandi, 12 M. Gromov, 13 M. Y. Guan, 20 Y. Guardincerri, 6 B. Hackett, 18 K. Herner, 6 E. V. Hungerford, 15 A.l. Ianni, 7 A.n. Ianni, 5 C. Jollet, 21 K. Keeter, 22 C. Kendziora, 6 S. Kidner, a. V. Kobychev, 24 G. Koh, 5 D. Korablev, 19 G. Korga, 15 A. Kurlej, 2 P. X. Li, 20 B. Loer, 5 P. Lombardi, 9 C. Love, 25 L. Ludhova, 9 S. Luitz, 26 Y. Q. Ma, 20 I. Machulin, 28 A. Mandarano, 10 J. Maricic, 18 L. Marini, 10 C. J. Martoff, 25 A. Meregaglia, 21 E. Meroni, 9 P. D. Meyers, 5 R. Milincic, 18 D. Montanari, 6 M. Montuschi, 7 M. E. Monzani, 26 P. Mosteiro, 5 B. Mount, 22 V. Muratova, 16 P. Musico, 11 A. Nelson, 5 S. Odrowski, 7 M. Okounkova, 5 M. Orsini, 7 F. Ortica, 29 L. Pagani, 11 M. Pallavicini, 11 E. Pantic, 4, 30 L. Papp, 23 S. Parmeggiano, 9 R. Parsells, 5 K. Pelczar, 31 N. Pelliccia, 29 S. Perasso, 1 A. Pocar, 2 S. Pordes, 6 D. Pugachev, 27 H. Qian, 5 K. Randle, 2 G. Ranucci, 9 A. Razeto, 7 B. Reinhold, 18 A. Renshaw, 4 A. Romani, 29 B. Rossi, 5, 14 N. Rossi, 7 S. D. Rountree, 23 D. Sablone, 15 P. Saggese, 7 R. Saldanha, 12 W. Sands, 5 S. Sangiorgio, 32 E. Segreto, 7 D. Semenov, 16 E. Shields, 5 M. Skorokhvatov, 28 O. Smirnov, 19 A. Sotnikov, 19 C. Stanford, 5 Y. Suvorov, 4 R. Tartaglia, 7 J. Tatarowicz, 25 G. Testera, 11 A. Tonazzo, 1 E. Unzhakov, 16 R. B. Vogelaar, 23 M. Wada, 5 S. Walker, 14 H. Wang, 4 Y. Wang, 20 A. Watson, 25 S. Westerdale, 5 M. Wojcik, 31 A. Wright, 5 X. Xiang, 5 J. Xu, 5 C. G. Yang, 20 J. Yoo, 6 S. Zavatarelli, 11 A. Zec, 2 C. Zhu, G. Zuzel 3, MARI, Stefano Maria, P. Agnes, P., Agne, 1 T., Alexander, 2 A., Alton, 3 K., Arisaka, 4 H. O., Back, 5 B., Baldin, 6 K., Biery, 6 G., Bonfini, 7 M., Bossa, 8 A., Brigatti, 9 J., Brodsky, 5 F., Budano, 10 L., Cadonati, 2 F., Calaprice, 5 N., Canci, 4 A., Candela, 7 H., Cao, 5 M., Cariello, 11 P., Cavalcante, 7 A., Chavarria, 12 A., Chepurnov, 13 A. G., Cocco, 14 L., Crippa, 9 D., D’Angelo, 9 M., D’Incecco, 7 S., Davini, 15 M., De Deo, 7 A., Derbin, 16 A., Devoto, 17 F., Di Eusanio, 5 G., Di Pietro, 9 E., Edkin, 18 A., Empl, 15 A., Fan, 4 G., Fiorillo, 14 K., Fomenko, 19 G., Forster, 2 D., Franco, 1 F., Gabriele, 7 C., Galbiati, 5 A., Goretti, 5 L., Grandi, 12 M., Gromov, 13 M. Y., Guan, 20 Y., Guardincerri, 6 B., Hackett, 18 K., Herner, 6 E. V., Hungerford, Ianni, 15 A. l., Ianni, 7 A. n., 5 C., Jollet, 21 K., Keeter, 22 C., Kendziora, 6 S., Kidner, a. V., Kobychev, 24 G., Koh, 5 D., Korablev, 19 G., Korga, 15 A., Kurlej, 2 P. X., Li, 20 B., Loer, 5 P., Lombardi, 9 C., Love, 25 L., Ludhova, 9 S., Luitz, 26 Y. Q., Ma, 20 I., Machulin, 28 A., Mandarano, Mari, Stefano Maria, 10 J., Maricic, 18 L., Marini, 10 C. J., Martoff, 25 A., Meregaglia, 21 E., Meroni, 9 P. D., Meyer, 5 R., Milincic, 18 D., Montanari, 6 M., Montuschi, 7 M. E., Monzani, 26 P., Mosteiro, 5 B., Mount, 22 V., Muratova, 16 P., Musico, 11 A., Nelson, 5 S., Odrowski, 7 M., Okounkova, 5 M., Orsini, 7 F., Ortica, 29 L., Pagani, 11 M., Pallavicini, 11 E., Pantic, 30 L., Papp, 23 S., Parmeggiano, 9 R., Parsell, 5 K., Pelczar, 31 N., Pelliccia, 29 S., Perasso, 1 A., Pocar, 2 S., Porde, 6 D., Pugachev, 27 H., Qian, 5 K., Randle, 2 G., Ranucci, 9 A., Razeto, 7 B., Reinhold, 18 A., Renshaw, 4 A., Romani, 29 B., Rossi, 14 N., Rossi, 7 S. D., Rountree, 23 D., Sablone, 15 P., Saggese, 7 R., Saldanha, 12 W., Sand, 5 S., Sangiorgio, 32 E., Segreto, 7 D., Semenov, 16 E., Shield, 5 M., Skorokhvatov, 28 O., Smirnov, 19 A., Sotnikov, 19 C., Stanford, 5 Y., Suvorov, 4 R., Tartaglia, 7 J., Tatarowicz, 25 G., Testera, 11 A., Tonazzo, 1 E., Unzhakov, 16 R. B., Vogelaar, 23 M., Wada, 5 S., Walker, 14 H., Wang, 4 Y., Wang, 20 A., Watson, 25 S., Westerdale, 5 M., Wojcik, 31 A., Wright, 5 X., Xiang, 5 J., Xu, 5 C. G., Yang, 20 J., Yoo, 6 S., Zavatarelli, 11 A., Zec, 2 C., Zhu, and G., Zuzel 3
Subjects: Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment, Astrophysics::Cosmology and Extragalactic Astrophysics, Nuclear Experiment
Abstract: We report the first results of DarkSide-50, a direct search for dark matter operating in the un- derground Laboratori Nazionali del Gran Sasso (LNGS) and searching for the rare nuclear recoils possibly induced by weakly interacting massive particles (WIMPs). The dark matter detector is a Liquid Argon Time Projection Chamber with a ( 46.4 0.7 ) kg active mass, operated inside a 30 t or- ganic liquid scintillator neutron veto, which is in turn installed at the center of a 1 kt water Cherenkov veto for the residual flux of cosmic rays. We report here the null results of a dark matter search for a ( 1422 67 ) kg d exposure with an atmospheric argon fill. This is the most sensitive dark matter search performed with an argon target, corresponding to a 90% CL upper limit on the WIMP-nucleon spin-independent cross section of 6.1 10
Published: 2014

11. The Electronics and Data Acquisition System of the DarkSide Dark Matter Search

Author: The DarkSide Collaboration, P. Agnes 1, T. Alexander 2, A. Alton 3, K. Arisaka 4, H. O. Back 5, B. Baldin 6, K. Biery 6, G. Bonfini 7, M. Bossa 8, A. Brigatti 9, J. Brodsky 5, F. Budano 10, L. Cadonati 2, F. Calaprice 5, N. Canci 4, A. Candela 7, H. Cao 5, M. Cariello 11, P. Cavalcante 7, A. Chavarria 12, A. Chepurnov 13, A. G. Cocco 14, L. Crippa 9, D. D’Angelo 9, M. D’Incecco 7, S. Davini 15, M. De Deo 7, A. Derbin 16, A. Devoto 17, F. Di Eusanio 5, G. Di Pieto 9, E. Edkins 18, A. Empl 15, A. Fan 4, G. Fiorillo 14, K. Fomenko 19, G. Forster 2, D. Franco 1, F. Gabriele 7, C. Galbiati 5, A. Goretti 5, L. Grandi 12, M. Gromov 13, M. Y. Guan 20, Y. Guardincerri 6, B. Hackett 18, K. Herner 6, E. Hungerford 15, A.l. Ianni 7, A.n. Ianni 5, C. Jollet 21, K. Keeter 22, C. Kendziora 6, S. Kidner 23, V. Kobychev 24, G. Koh 5, D. Korablev 19, G. Korga 15, A. Kurlej 2, P. X. Li 20, B. Loer 5, P. Lombardi 9, C. Love 25, L. Ludhova 9, S. Luitz 26, Y. Q. Ma 20, I. Machulin 27, A. Mandarano 10, J. Maricic 18, L. Marini 10, J. Martoff 25, A. Meregaglia 21, E. Meroni 9, P. D. Meyers 5, R. Milincic 18, D. Montanari 6, M. Montuschi 7, M. E. Monzani 26, P. Mosteiro 5, B. Mount 22, V. Muratova 16, P. Musico 11, A. Nelson 5, S. Odrowski 7, M. Okounkoa 5, M. Orsini 7, F. Ortica 19, L. Pagani 11, M. Pallavicini 11, E. Pantic 4, L. Papp 23, S. Parmeggiano 9, Bob Parsells 5, K. Pelczar 31, N. Pelliccia 29, S. Perasso 1, A. Pocar 2, S. Pordes 6, D. Pugachev 27, H. Qian 5, K. Randle 2, G. Ranucci 9, A. Razeto 7, B. Reinhold 18, A. Renshaw 4, A. Romani 29, B. Rossi 5, N. Rossi 7, S. D. Rountree 23, D. Sablone 15, P. Saggese 7, R. Saldanha 12, W. Sands 5, S. Sangiorgio 30, E. Segreto 7, D. Semenov 16, E. Shields 5, M. Skorokhvatov 27, O. Smirnov 19, A. Sotnikov 19, C. Stanford 5, Suvorov 4, R. Tartaglia 17, J. Tatarowicz 25, G. Testera 11, A. Tonazzo 1, E. Unzhakov 16, R. B. Vogelaar 23, M. Wada 5, S. E. Walker 14, H. Wang 4, Y. Wang 28, A. Watson 25, S. Westerdale 5, M. Wojcik 31, A. Wright 5, X. Xiang 5, J. Xu 5, C. G. Yang 20, J. Yoo 6, S. Zavatarelli 11, A. Zec 2, C. Zhu 5, G. Zuzel 31, MARI, Stefano Maria, P. Agnes, P.Agnes, The DarkSide, Collaboration, P., Agnes 1, T., Alexander 2, A., Alton 3, K., Arisaka 4, H. O., Back 5, B., Baldin 6, K., Biery 6, G., Bonfini 7, M., Bossa 8, A., Brigatti 9, J., Brodsky 5, F., Budano 10, L., Cadonati 2, F., Calaprice 5, N., Canci 4, A., Candela 7, H., Cao 5, M., Cariello 11, P., Cavalcante 7, A., Chavarria 12, A., Chepurnov 13, A. G., Cocco 14, L., Crippa 9, D., D’Angelo 9, M., D’Incecco 7, S., Davini 15, M., De Deo 7, A., Derbin 16, A., Devoto 17, F., Di Eusanio 5, G., Di Pieto 9, E., Edkins 18, A., Empl 15, A., Fan 4, G., Fiorillo 14, K., Fomenko 19, G., Forster 2, D., Franco 1, F., Gabriele 7, C., Galbiati 5, A., Goretti 5, L., Grandi 12, M., Gromov 13, M. Y., Guan 20, Y., Guardincerri 6, B., Hackett 18, K., Herner 6, E., Hungerford 15, Ianni 7, A. l., Ianni 5, A. n., C., Jollet 21, K., Keeter 22, C., Kendziora 6, S., Kidner 23, V., Kobychev 24, G., Koh 5, D., Korablev 19, G., Korga 15, A., Kurlej 2, P. X., Li 20, B., Loer 5, P., Lombardi 9, C., Love 25, L., Ludhova 9, S., Luitz 26, Y. Q., Ma 20, I., Machulin 27, A., Mandarano 10, Mari, Stefano Maria, J., Maricic 18, L., Marini 10, J., Martoff 25, A., Meregaglia 21, E., Meroni 9, P. D., Meyers 5, R., Milincic 18, D., Montanari 6, M., Montuschi 7, M. E., Monzani 26, P., Mosteiro 5, B., Mount 22, V., Muratova 16, P., Musico 11, A., Nelson 5, S., Odrowski 7, M., Okounkoa 5, M., Orsini 7, F., Ortica 19, L., Pagani 11, M., Pallavicini 11, E., Pantic 4, L., Papp 23, S., Parmeggiano 9, Bob Parsells, 5, K., Pelczar 31, N., Pelliccia 29, S., Perasso 1, A., Pocar 2, S., Pordes 6, D., Pugachev 27, H., Qian 5, K., Randle 2, G., Ranucci 9, A., Razeto 7, B., Reinhold 18, A., Renshaw 4, A., Romani 29, B., Rossi 5, N., Rossi 7, S. D., Rountree 23, D., Sablone 15, P., Saggese 7, R., Saldanha 12, W., Sands 5, S., Sangiorgio 30, E., Segreto 7, D., Semenov 16, E., Shields 5, M., Skorokhvatov 27, O., Smirnov 19, A., Sotnikov 19, C., Stanford 5, Suvorov, 4, R., Tartaglia 17, J., Tatarowicz 25, G., Testera 11, A., Tonazzo 1, E., Unzhakov 16, R. B., Vogelaar 23, M., Wada 5, S. E., Walker 14, H., Wang 4, Y., Wang 28, A., Watson 25, S., Westerdale 5, M., Wojcik 31, A., Wright 5, X., Xiang 5, J., Xu 5, C. G., Yang 20, J., Yoo 6, S., Zavatarelli 11, A., Zec 2, C., Zhu 5, and G., Zuzel 31
Abstract: It is generally inferred from astronomical measurements th at Dark Matter (DM) comprises approximately 27% of the energy-dens ity of the universe. If DM is a subatomic particle, a possible candidate is a Weakl y Interacting Mas- sive Particle (WIMP), and the DarkSide-50 (DS) experiment i s a direct search for evidence of WIMP-nuclear collisions. DS is located undergr ound at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, and consists of thr ee active, embedded components; an outer water veto (CTF), a liquid scintillato r veto (LSV), and a liquid argon (LAr) time projection chamber (TPC). This pap er describes the data acquisition and electronic systems of the DS detectors , designed to detect the residual ionization from s
Published: 2014

12. Muon capture on light isotopes measured with the Double Chooz detector

Author: A. Hourlier, L. B. Bezrukov, Eric Baussan, T. Brugière, S. M. Fernandes, J. Reichenbacher, A.V. Etenko, D. Hellwig, I. Stancu, L. Camilleri, T. Hara, C. Veyssiere, R. Carr, H. Furuta, G. Mention, Anatael Cabrera, J. C. dos Anjos, D. Shrestha, A. Onillon, M. H. Shaevitz, M. Vivier, J. M. LoSecco, C. Alt, Yoshio Abe, Anselmo Meregaglia, J. Spitz, H. Gomez, E. Conover, V. Zimmer, Amanda Porta, Marcos Cerrada, G. A. Horton-Smith, C. Mariani, H. P. Lima, H. de Kerret, G. Yang, J. Maeda, Josef Jochum, BayarJon Paul Lubsandorzhiev, A.C. Schilithz, I. Bekman, V. Sibille, S. Appel, I. Gil-Botella, N. Vassilopoulos, R. Roncin, J.V. Dawson, S. Perasso, L. Goodenough, Luis González, F. von Feilitzsch, J. Busenitz, R. Santorelli, J. M. López-Castaño, M. Kaneda, Muriel Fallot, B. Reinhold, A. Tonazzo, F. Yermia, Audrey Letourneau, Janet Conrad, E. Damon, E. Blucher, Y. Sakamoto, T. Miletic, Zelimir Djurcic, Matthew L Strait, T. Abrahão, Y. Kamyshkov, M. Franke, R. Svoboda, Masahiro Kuze, Florian Kaether, J. Felde, J. Dhooghe, G. Pronost, F. Suekane, M. Obolensky, L.F.F. Stokes, P. Novella, T. Sumiyoshi, D. Franco, J. Martino, David Lhuillier, V. V. Sinev, N. Walsh, E. Kemp, M. Röhling, Takeo Kawasaki, A. Minotti, I. M. Pepe, P. Chimenti, Lydie Giot, A. Stahl, Lothar Oberauer, T. Matsubara, M. Göger-Neff, R. Milincic, E. Chauveau, Cécile Jollet, S. Schönert, A. Osborn, Yasushi Nagasaka, Daniel M. Kaplan, Stefan Schoppmann, H. Almazan, C. E. Lane, Masaki Ishitsuka, J. Maricic, Tobias Lachenmaier, V. Fischer, Y. Sun, Stephen Robert Wagner, Marcos Dracos, M. Bergevin, S. V. Sukhotin, E. Smith, N. Haag, K. Crum, J. I. Crespo-Anadón, S. Lucht, R. Sharankova, Diana Navas-Nicolas, C. Palomares, Michael Hofmann, Christian Buck, L. N. Kalousis, T.J.C. Bezerra, D. Dietrich, Kazuhiro Terao, A. S. Cucoanes, Christopher Wiebusch, G. A. Valdiviesso, M. C. Goodman, J. Haser, M. D. Skorokhvatov, Michael Wurm, H. Watanabe, Thierry Lasserre, J. C. Barriere, D. Kryn, M. Soiron, H. H. Trinh Thi, Manfred Lindner, Antoine Collin, B. Rybolt, Abe, Y, Abrahao, T, Almazan, H, Alt, C, Appel, S, Barriere, J, Baussan, E, Bekman, I, Bergevin, M, Bezerra, T, Bezrukov, L, Blucher, E, Brugiere, T, Buck, C, Busenitz, J, Cabrera, A, Camilleri, L, Carr, R, Cerrada, M, Chauveau, E, Chimenti, P, Collin, A, Conover, E, Conrad, J, Crespo-Anadon, J, Crum, K, Cucoanes, A, Damon, E, Dawson, J, De Kerret, H, Dhooghe, J, Dietrich, D, Djurcic, Z, Dos Anjos, J, Dracos, M, Etenko, A, Fallot, M, Felde, J, Fernandes, S, Fischer, V, Franco, D, Franke, M, Furuta, H, Gil-Botella, I, Giot, L, Goger-Neff, M, Gomez, H, Gonzalez, L, Goodenough, L, Goodman, M, Haag, N, Hara, T, Haser, J, Hellwig, D, Hofmann, M, Horton-Smith, G, Hourlier, A, Ishitsuka, M, Jochum, J, Jollet, C, Kaether, F, Kalousis, L, Kamyshkov, Y, Kaneda, M, Kaplan, D, Kawasaki, T, Kemp, E, Kryn, D, Kuze, M, Lachenmaier, T, Lane, C, Lasserre, T, Letourneau, A, Lhuillier, D, Lima, H, Lindner, M, Lopez-Castano, J, Losecco, J, Lubsandorzhiev, B, Lucht, S, Maeda, J, Mariani, C, Maricic, J, Martino, J, Matsubara, T, Mention, G, Meregaglia, A, Miletic, T, Milincic, R, Minotti, A, Nagasaka, Y, Navas-Nicolas, D, Novella, P, Oberauer, L, Obolensky, M, Onillon, A, Osborn, A, Palomares, C, Pepe, I, Perasso, S, Porta, A, Pronost, G, Reichenbacher, J, Reinhold, B, Rohling, M, Roncin, R, Rybolt, B, Sakamoto, Y, Santorelli, R, Schilithz, A, Schonert, S, Schoppmann, S, Shaevitz, M, Sharankova, R, Shrestha, D, Sibille, V, Sinev, V, Skorokhvatov, M, Smith, E, Soiron, M, Spitz, J, Stahl, A, Stancu, I, Stokes, L, Strait, M, Suekane, F, Sukhotin, S, Sumiyoshi, T, Sun, Y, Svoboda, R, Terao, K, Tonazzo, A, Trinh Thi, H, Valdiviesso, G, Vassilopoulos, N, Veyssiere, C, Vivier, M, Von Feilitzsch, F, Wagner, S, Walsh, N, Watanabe, H, Wiebusch, C, Wurm, M, Yang, G, Yermia, F, and Zimmer, V
Subjects: Physics, Semileptonic decay, Particle physics, education.field_of_study, Muon, 010308 nuclear & particles physics, Population, neutrino physic, 01 natural sciences, Muon capture, Nuclear physics, 13. Climate action, 0103 physical sciences, High Energy Physics::Experiment, Neutron, Production (computer science), Neutrino, 010306 general physics, Ground state, education
Abstract: Using the Double Chooz detector, designed to measure the neutrino mixing angle $\theta_{13}$, the products of $\mu^-$ capture on $^{12}$C, $^{13}$C, $^{14}$N and $^{16}$O have been measured. Over a period of 489.5 days, $2.3\times10^6$ stopping cosmic $\mu^-$ have been collected, of which $1.8\times10^5$ captured on carbon, nitrogen, or oxygen nuclei in the inner detector scintillator or acrylic vessels. The resulting isotopes were tagged using prompt neutron emission (when applicable), the subsequent beta decays, and, in some cases, $\beta$-delayed neutrons. The most precise measurement of the rate of $^{12}\mathrm C(\mu^-,\nu)^{12}\mathrm B$ to date is reported: $6.57^{+0.11}_{-0.21}\times10^{3}\,\mathrm s^{-1}$, or $(17.35^{+0.35}_{-0.59})\%$ of nuclear captures. By tagging excited states emitting gammas, the ground state transition rate to $^{12}$B has been determined to be $5.68^{+0.14}_{-0.23}\times10^3\,\mathrm s^{-1}$. The heretofore unobserved reactions $^{12}\mathrm C(\mu^-,\nu\alpha)^{8}\mathrm{Li}$, $^{13}\mathrm C(\mu^-,\nu\mathrm n\alpha)^{8}\mathrm{Li}$, and $^{13}\mathrm C(\mu^-,\nu\mathrm n)^{12}\mathrm B$ are measured. Further, a population of $\beta$n decays following stopping muons is identified with $5.5\sigma$ significance. Statistics limit our ability to identify these decays definitively. Assuming negligible production of $^{8}$He, the reaction $^{13}\mathrm C(\mu^-,\nu\alpha)^{9}\mathrm{Li}$ is found to be present at the $2.7\sigma$ level. Limits are set on a variety of other processes.
Published: 2016

13. The DarkSide awakens

Author: B. Bottino, R. Tartaglia, A. K. Alton, K. Randle, A. Vishneva, Mariano Cadoni, Denis Korablev, P. Cavalcante, P. J. Mosteiro, J. Brodsky, Michele Montuschi, L. Marini, M. Bossa, P. Saggese, I. N. Machulin, Samuele Sangiorgio, B. J. Mount, N. Rossi, L. Agostino, E. Pantic, A. M. Goretti, N. Canci, C. L. Kendziora, Irina James, B. Rossi, M. Orsini, D. Montanari, S. Catalanotti, Marco Pallavicini, D. D'Angelo, M. Cariello, E. Shields, A. G. Cocco, Jingke Xu, Alan Watson, A. Mandarano, P Trinchese, V. N. Muratova, K. Biery, Yanchu Wang, L. Pagani, K. Pelczar, Cristiano Galbiati, S. Perasso, M. D. Skorokhvatov, S. De Cecco, P. D. Meyers, S. Bussino, Nicomede Pelliccia, L. Grandi, K. Arisaka, G. Korga, C. Stanford, B. Vogelaar, G. Fiorillo, Anton Empl, B. Reinhold, M. M. Wojcik, Chung-Yao Yang, E. Edkins, Paolo Musico, A. V. Derbin, A. Razeto, J. Wilhelmi, A. Fan, M. Wada, Y. Guardincerri, D. A. Pugachev, M. D'Incecco, Anselmo Meregaglia, J. Yoo, M. Lissia, H. Qian, F. Gabriele, G. Zuzel, E. V. Hungerford, G. Testera, D. Sablone, A. Candela, O. Smirnov, M. Gromov, G. Di Pietro, Giovanni Covone, A. Sotnikov, Jim Napolitano, A. S. Kubankin, F. Di Eusanio, A. Tonazzo, S. Parmeggiano, J. Maricic, Aldo Romani, E. V. Unzhakov, P. Agnes, S. Walker, Yanhui Ma, C. Savarese, M. De Deo, W. Sands, Thomas Alexander, M. E. Monzani, Andrea Ianni, Sandra Zavatarelli, A. Pocar, M. Cadeddu, Xiujiang Li, D. Franco, Gioacchino Ranucci, K. Herner, T. Miletic, W. Zhong, Griffin Foster, R. Saldanha, J. Tatarowicz, D. A. Semenov, Caoxiang Zhu, H. Cao, S. Luitz, F. Granato, Cécile Jollet, Han Wang, A. Devoto, Y. Suvorov, S. Westerdale, B. Baldin, S. M. Mari, A. S. Chepurnov, S. Davini, Henning O. Back, S. D. Rountree, Paolo Lombardi, E. Segreto, A. Monte, V. V. Kobychev, B. R. Hackett, A. Brigatti, C. J. Martoff, G. Bonfini, K. J. Keeter, Frank Calaprice, X. Xiang, A. Zec, S. Pordes, R. Milincic, G. Koh, A. L. Renshaw, Aldo Ianni, M. Carlini, P. N. Singh, K. Fomenko, F. Budano, C. Giganti, Laura Cadonati, Fausto Ortica, Min-Xin Guan, M. De Vincenzi, Ivone F. M. Albuquerque, Davini, S., Agnes, P., Agostino, L., M. Albuquerque, I. F., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, Federico, Bussino, Severino Angelo Maria, Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., D'Angelo, D., D'Incecco, M., De Cecco, S., De Deo, M., DE VINCENZI, Mario, Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Foster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K. R., Hungerford, E. V., Ianni, Aldo, Ianni, Andrea, James, Irina, Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, Stefano Maria, Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., Gran Sasso Science Institute (GSSI), Istituto Nazionale di Fisica Nucleare (INFN), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), DarkSide, Albuquerque, I. F. M., Back, H., Budano, F., Bussino, S., Catalanotti, Sergio, Cocco, ALFREDO GIUSEPPE, Covone, Giovanni, De Vincenzi, M., Di Pietra, G., Fiorillo, Giuliana, James, I., Mari, S. M., Muratova, N., and Walker, Susan Elizabeth
Subjects: History, chemistry.chemical_element, DarkSide, WIMP Argon Programme, WIMP: detector, 01 natural sciences, Education, Atmosphere, Nuclear physics, Physics and Astronomy (all), 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010303 astronomy & astrophysics, Physics, Argon, 010308 nuclear & particles physics, Astronomy, suppression, time projection chamber: liquid argon, Computer Science Applications, Gran Sasso, chemistry, radioactivity, argon, atmosphere, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: International audience; The DarkSide program at LNGS aims to perform background-free WIMP searches using two phase liquid argon time projection chambers, with the ultimate goal of covering all parameters down to the so-called neutrino floor. One of the distinct features of the program is the use of underground argon with has a reduced content of the radioactive $^{39}$Ar compared to atmospheric argon. The DarkSide Collaboration is currently operating the DarkSide-50 experiment, the first such WIMP detector using underground argon. Operations with underground argon indicate a suppression of $^{39}$Ar by a factor (1.4 ± 0.2) × 10$^3$ relative to atmospheric argon. The new results obtained with DarkSide-50 and the plans for the next steps of the DarkSide program, the 20t fiducial mass DarkSide-20k detector and the 200 t fiducial Argo, are reviewed in this proceedings.
Published: 2016

14. The veto system of the DarkSide-50 experiment

Author: E. Shields, J. Yoo, Nicomede Pelliccia, A. G. Cocco, B. Reinhold, E. Pantic, C. Giganti, Laura Cadonati, Cécile Jollet, Fausto Ortica, Mariano Cadoni, Andrea Ianni, Sandra Zavatarelli, M. Carlini, E. Edkins, P. N. Singh, K. Fomenko, F. Budano, O. Smirnov, K. Biery, Yanchu Wang, M. D. Skorokhvatov, N. Rossi, L. Agostino, Henning O. Back, L. Grandi, Griffin Foster, H. Cao, S. Parmeggiano, B. R. Hackett, B. Baldin, S. Perasso, A. Zec, Paolo Musico, T. Miletic, A. Fan, D. A. Pugachev, E. V. Unzhakov, E. Segreto, J. Tatarowicz, Ivone F. M. Albuquerque, C. Savarese, A. K. Alton, S. Pordes, S. Walker, Hui Wang, L. Pagani, K. Arisaka, P. Trinchese, P. J. Mosteiro, E. V. Hungerford, S. Davini, A. Brigatti, M. Orsini, L. Crippa, G. Fiorillo, D. Sablone, C. J. Martoff, G. Bonfini, R. Saldanha, Michele Montuschi, A. Candela, S. Odrowski, P. D. Meyers, Thomas Alexander, Jingke Xu, S. Westerdale, G. Testera, D. A. Semenov, K. Pelczar, Cristiano Galbiati, Yanhui Ma, G. Di Pietro, Giovanni Covone, J. Wilhelmi, R. Milincic, M. De Deo, A. Nelson, M. Wada, M. D'Incecco, Stefano Maria Mari, A. S. Kubankin, R. Tartaglia, K. J. Keeter, Frank Calaprice, X. Xiang, Severino Angelo Maria Bussino, G. Koh, Anselmo Meregaglia, H. Qian, Y. Guardincerri, A. Sotnikov, A. Mandarano, S. Catalanotti, D. Franco, W. Zhong, B. J. Mount, Y. Suvorov, M. Gromov, S. Luitz, V. N. Muratova, V. V. Kobychev, A. S. Chepurnov, W. Sands, C. Zhu, P. Cavalcante, B. Bottino, M. E. Monzani, A. Devoto, F. Di Eusanio, C. Stanford, A. Pocar, Denis Korablev, Samuele Sangiorgio, Aldo Romani, J. Brodsky, P. Saggese, P. Agnes, S. D. Rountree, D. Montanari, M. Cadeddu, Paolo Lombardi, M. Lissia, A. Monte, A. V. Derbin, S. De Cecco, Chung-Yao Yang, L. Marini, M. Bossa, B. Rossi, Alan Watson, G. Zuzel, Gioacchino Ranucci, K. Herner, F. Gabriele, Jim Napolitano, K. Randle, A. Tonazzo, A. Vishneva, X. Li, C. L. Kendziora, Irina James, J. Maricic, G. Korga, F. Granato, I. N. Machulin, N. Canci, Marco Pallavicini, D. D'Angelo, Anton Empl, M. M. Wojcik, A. L. Renshaw, Aldo Ianni, A. M. Goretti, M. Cariello, A. Razeto, T. N. Johnson, R. B. Vogelaar, Min-Xin Guan, M. De Vincenzi, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), DarkSide, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Agnes, P., Agostino, L., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., De Cecco, S., De Deo, M., De Vincenzi, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Foster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K. R., Hungerford, E. V., Ianni, Aldo, Ianni, Andrea, James, I., Johnson, T., Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, S. M., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Nelson, A., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, R. B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Pluridisciplinaire Hubert Curien ( IPHC ), Centre National de la Recherche Scientifique ( CNRS ) -Université de Strasbourg ( UNISTRA ), Bussino, Severino Angelo Maria, DE VINCENZI, Mario, Fiorillo, G., James, Irina, Mari, Stefano Maria, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANR-10-LABX-0023,UnivEarthS,Earth - Planets - Universe: observation, modeling, transfer(2010), and ANR-11-IDEX-0005,USPC,Université Sorbonne Paris Cité(2011)
Subjects: fast neutrons), Physics - Instrumentation and Detectors, axions, gas and liquid scintillators), Cherenkov detector, Cherenkov and transition radiation, Physics::Instrumentation and Detectors, Cherenkov counter: water, Nuclear Theory, scintillation counter: liquid, FOS: Physical sciences, Scintillator, 01 natural sciences, Particle detector, High Energy Physics - Experiment, law.invention, thermal, Dark Matter detectors (WIMPs, axions, etc.), Nuclear physics, High Energy Physics - Experiment (hep-ex), WIMP, [ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex], law, etc.), 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Neutron detection, Neutron, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Nuclear Experiment, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation, Dark Matter detectors (WIMPs, Mathematical Physics, Event reconstruction, nucleus: recoil, Physics, 010308 nuclear & particles physics, Detector, Instrumentation and Detectors (physics.ins-det), Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators), Neutron detectors (cold, thermal, fast neutrons), Neutron detectors (cold, scintillation and light emission processes (solid, Scintillators, High Energy Physics::Experiment, performance
Abstract: International audience; Nuclear recoil events produced by neutron scatters form one of the most important classes of background in WIMP direct detection experiments, as they may produce nuclear recoils that look exactly like WIMP interactions. In DarkSide-50, we both actively suppress and measure the rate of neutron-induced background events using our neutron veto, composed of a boron-loaded liquid scintillator detector within a water Cherenkov detector. This paper is devoted to the description of the neutron veto system of DarkSide-50, including the detector structure, the fundamentals of event reconstruction and data analysis, and basic performance parameters.
Published: 2016

15. A new anti-neutrino detection technique based on positronium tagging with plastic scintillators

Author: S. Perasso, Giovanni Consolati, A. Tonazzo, D. Franco, A. Minotti, Anselmo Meregaglia, Cécile Jollet, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Consolati, G, Franco, D, Jollet, C, Meregaglia, A, Minotti, A, Perasso, S, and Tonazzo, A
Subjects: Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, Scintillator, Detector, Neutrino, Positronium, Reactor, Instrumentation, 01 natural sciences, 7. Clean energy, Particle detector, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, Neutron, 010306 general physics, ComputingMilieux_MISCELLANEOUS, Physics, [PHYS]Physics [physics], 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), Neutron capture, Neutrino detector, Inverse beta decay, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Radioactive decay
Abstract: The main signature for anti-neutrino detection in reactor and geo-neutrino experiments based on scintillators is provided by the space-time coincidence of positron and neutron produced in the Inverse Beta Decay reaction. Such a signature strongly suppresses backgrounds and allows for measurements performed underground with a relatively high signal-to-background ratio. In an aboveground environment, however, the twofold coincidence technique is not sufficient to efficiently reject the high background rate induced by cosmogenic events. Enhancing the positron-neutron twofold coincidence efficiency has the potential to pave the way future aboveground detectors for reactor monitoring. We propose a new detection scheme based on a threefold coincidence, between the positron ionization, the ortho-positronium (o-Ps) decay, and the neutron capture, in a sandwich detector with alternated layers of plastic scintillator and aerogel powder. We present the results of a set of dedicated measurements on the achievable light yield and on the o-Ps formation and lifetime. The efficiencies for signal detection and background rejection of a preliminary detector design are also discussed., 18 pages, 10 figures
Published: 2015

16. The DarkSide Project

Author: Mariano Cadoni, L. Marini, M. Bossa, E. Shields, N. Rossi, B. Rossi, F. Gabriele, S. Bussino, D. A. Semenov, Jim Napolitano, Giovanni Covone, F. Di Eusanio, Alan Watson, V. N. Muratova, S. Perasso, Aldo Romani, K. Biery, Yanchu Wang, A. Tonazzo, P. Agnes, A. K. Alton, B. R. Hackett, A. M. Goretti, R. Tartaglia, M. Cariello, M. E. Monzani, A. Nelson, Al. Ianni, P. J. Mosteiro, T. Miletic, A. Pocar, Min-Xin Guan, A. Zec, S. Pordes, G. Forster, Sandra Zavatarelli, R. Milincic, Jingke Xu, Stefano Maria Mari, Hui Wang, B. J. Mount, C. Zhu, P. Cavalcante, Thomas Alexander, P. Trinchese, R. Saldanha, G. Koh, K. Pelczar, M. Montuschi, Paolo Musico, A. Fan, D. A. Pugachev, Cristiano Galbiati, B. Baldin, Ivone F. M. Albuquerque, J. Tatarowicz, M. Lissia, D. Montanari, S. Walker, E. Pantic, Samuele Sangiorgio, An. Ianni, Gioacchino Ranucci, C. Savarese, E. Segreto, H. Cao, M. Orsini, B. Bottino, M. De Vincenzi, A. Vishneva, D. Franco, S. Davini, W. Zhong, A. Mandarano, L. Crippa, C. L. Kendziora, M. D. Skorokhvatov, A. Monte, L. Grandi, Irina James, M. Carlini, A. L. Renshaw, Nicomede Pelliccia, V. V. Kobychev, Cécile Jollet, J. Wilhelmi, P. N. Singh, Chung-Yao Yang, A. V. Derbin, B. Reinhold, M. Wada, O. Smirnov, S. Parmeggiano, Y. Guardincerri, K. Fomenko, F. Budano, B. Vogelaar, Yanhui Ma, C. Giganti, Laura Cadonati, S. Odrowski, G. Di Pietro, E. V. Unzhakov, M. De Deo, E. Edkins, A. Brigatti, Fausto Ortica, D. Sablone, C. J. Martoff, G. Bonfini, A. Devoto, G. Testera, L. Agostino, D. Rountree, K. J. Keeter, J. Yoo, Paolo Lombardi, Henning O. Back, M. Gromov, J. Maricic, W. Sands, Frank Calaprice, X. Xiang, Peter Daniel Meyers, A. Kubankin, Y. Suvorov, S. Westerdale, A. Candela, A. S. Chepurnov, C. Stanford, Denis Korablev, J. Brodsky, P. Saggese, K. Randle, X. Li, G. Korga, F. Granato, I. N. Machulin, N. Canci, Marco Pallavicini, D. D'Angelo, Anton Empl, M. M. Wojcik, K. Arisaka, G. Fiorillo, L. Pagani, M. D'Incecco, Anselmo Meregaglia, H. Qian, M. Cadeddu, S. Luitz, A. Razeto, E. V. Hungerford, A. Sotnikov, K. Herner, S. De Cecco, G. Zuzel, S. Catalanotti, A. G. Cocco, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), DarkSide project, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Agnes, P., Agostino, L., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., De Cecco, S., De Deo, M., De Vincenzi, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., James, I., Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, S. M., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Nelson, A., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Romani, A., Rossi, B., Rossi, N., Rountree, D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., Bussino, Severino Angelo Maria, DE VINCENZI, Mario, Fiorillo, G., James, Irina, Mari, Stefano Maria, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: axions, Dark matter, chemistry.chemical_element, DarkSide, Noble liquid detectors (scintillation, ionization, double-phase), WIMP Argon Programme, Scintillator, dark matter: direct detection, 01 natural sciences, argon: nuclide, Dark Matter detectors (WIMPs, axions, etc.), Nuclear physics, Noble liquid detectors (scintillation, etc.), 0103 physical sciences, ionization, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, Dark Matter detectors (WIMPs, Mathematical Physics, Physics, Argon, 010308 nuclear & particles physics, Large detector systems for particle and astroparticle physics, Time projection Chambers (TPC), double-phase), time projection chamber: liquid argon, deep underground detector, Gran Sasso, chemistry, Project based, Large detector systems for particle and astroparticle physic, National laboratory, performance, ArDM
Abstract: International audience; DarkSide is a graded experimental project based on radiopure argon, and is now, and will be, used in direct dark matter searches. The present DarkSide-50 detector, operating at the Gran Sasso National Laboratory, is a dual-phase, 50 kg, liquid argon time-projection-chamber surrounded by an active liquid scintillator veto. It is designed to be background free in 3 years of operation. DS-50 performances, when filled with atmospheric argon, are reported. However DS-50 filled with underground argon, shows impressive reduction of the (39)Ar isotope. The application of this powerful technology in a future generation of the DarkSide program is discussed.
Published: 2015

17. DarkSide search for dark matter

Author: I. N. Machulin, R. Klemmer, Marco Pallavicini, N. Rossi, G. Forster, K. Fomenko, W. Sands, G. Di Pietro, H. Cao, D. D'Angelo, M. Komor, A. Razeto, N. N. Nurakhov, R. Saldanha, S. Parmeggiano, A. Nemtzow, E. Shields, F. Perfetto, Min-Xin Guan, M. Gromov, K. Randle, E. V. Unzhakov, S. Bussino, M. Orsini, M. Montuschi, E. Meroni, G. Korga, Austin P. Lund, Marc S. Seigar, A. Tonazzo, E. de Haas, G. Testera, L. Lukyanchenko, S. Gazzana, M. D. Skorokhvatov, B. Rossi, M. De Vincenzi, J. Maricic, L. Grandi, G. Zuzel, Laura Cadonati, M. E. Monzani, Yanhui Ma, D. Durben, M. Zehfus, B. J. Mount, Chung-Yao Yang, Augusto Brigatti, Lawrence Pinsky, A. Kayunov, R. B. Vogelaar, A. Meregaglia, S. Chidzik, C. Joliet, C. Condon, C. Ghiano, A. Pocar, N. Pelliccia, C. L. Kendziora, P. Saggese, A. Nelson, Sandra Zavatarelli, P. X. Li, O. Smirnov, S. Westerdale, Livia Ludhova, A. M. Goretti, A. S. Chepurnov, Thomas Alexander, S. Pordes, E. V. Hungerford, G. Koh, G. Guray, A. Sotnikov, Fausto Ortica, C. Guo, D. A. Semenov, R. Tartaglia, E. Pantic, K. Arisaka, G. Fiorillo, D. Korablev, I. Dratchnev, C. J. Martoff, Frank Calaprice, J. Brodsky, J. Tatarowicz, K. Keeter, Gioacchino Ranucci, Marcin Wójcik, D. Franco, W. Zhong, P. Cavalcante, Henning O. Back, G. Bonfini, P. Beltrame, P. D. Meyers, J. Thompson, An. Ianni, V. N. Muratova, L. Perasso, D. Alton, C. Salvo, S. Perasso, A.V. Etenko, R. Parsells, S. Davini, A. G. Cocco, Al. Ianni, Stefano Maria Mari, S. Luitz, Han Wang, P. J. Mosteiro, F. Gabriele, Jingke Xu, Cristiano Galbiati, D. Montanari, A. Fan, A. Empl, S. Kidner, S. V. Sukhotin, A. Wright, V. V. Kobychev, K. Lung, C. Love, T. Mohayai, A. Candela, S. D. Rountree, Paolo Lombardi, Aldo Romani, B Loer, A. V. Derbin, Y Suvarov, Jay Burton Benziger, T., Alexander, D., Alton, K., Arisaka, H. O., Back, P., Beltrame, J., Benziger, G., Bonfini, A., Brigatti, J., Brodsky, S., Bussino, L., Cadonati, F., Calaprice, A., Candela, H., Cao, P., Cavalcante, A., Chepurnov, S., Chidzik, A. G., Cocco, C., Condon, D., D'Angelo, S., Davini, M. D., Vincenzi, E. D., Haa, A., Derbin, G. D., Pietro, I., Dratchnev, D., Durben, A., Empl, A., Etenko, A., Fan, Fiorillo, Giuliana, D., Franco, K., Fomenko, G., Forster, F., Gabriele, C., Galbiati, S., Gazzana, C., Ghiano, A., Goretti, L., Grandi, M., Gromov, M., Guan, C., Guo, G., Guray, E. V., Hungerford, A., Ianni, C., Joliet, A., Kayunov, K., Keeter, C., Kendziora, S., Kidner, R., Klemmer, V., Kobychev, G., Koh, M., Komor, D., Korablev, G., Korga, P., Li, B., Loer, P., Lombardi, C., Love, L., Ludhova, S., Luitz, L., Lukyanchenko, A., Lund, K., Lung, Y., Ma, I., Machulin, S., Mari, J., Maricic, C. J., Martoff, A., Meregaglia, E., Meroni, P., Meyer, T., Mohayai, D., Montanari, M., Montuschi, M. E., Monzani, P., Mosteiro, B., Mount, V., Muratova, A., Nelson, A., Nemtzow, N., Nurakhov, M., Orsini, F., Ortica, M., Pallavicini, E., Pantic, S., Parmeggiano, R., Parsell, N., Pelliccia, L., Perasso, S., Perasso, Perfetto, Francesco, L., Pinsky, A., Pocar, S., Porde, K., Randle, G., Ranucci, A., Razeto, A., Romani, B., Rossi, N., Rossi, S. D., Rountree, P., Saggese, R., Saldanha, C., Salvo, W., Sand, M., Seigar, D., Semenov, E., Shield, M., Skorokhvatov, O., Smirnov, A., Sotnikov, S., Sukhotin, Y., Suvarov, R., Tartaglia, J., Tatarowicz, G., Testera, J., Thompson, A., Tonazzo, E., Unzhakov, R. B., Vogelaar, H., Wang, S., Westerdale, M., Wojcik, A., Wright, J., Xu, C., Yang, S., Zavatarelli, M., Zehfu, W., Zhong, G., Zuzel, Physics Department, Amherst U., University of Massachusetts System (UMASS), Biomécanique et Bioingénierie (BMBI), Université de Technologie de Compiègne (UTC)-Centre National de la Recherche Scientifique (CNRS), Régulation de l'expression génétique chez les microorganismes (REGCM), Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire Kastler Brossel (LKB (Jussieu)), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), departement de physique, Albert-Ludwigs-Universität Freiburg, SLAC National Accelerator Laboratory (SLAC), Stanford University, Anhui University [Hefei], Physics Department, Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Department of Geological Sciences, University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), Università degli studi di Genova = University of Genoa (UniGe), Departamento de Engenharia Elétrica [Minas Gerais] (DEE - UFMG), Universidade Federal de Minas Gerais, Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Rhodes University, Grahamstown, EAST CHINA UNIVERSITY, KEY LAB, Institute of Physics, Polish Academy of Sciences, Polska Akademia Nauk = Polish Academy of Sciences (PAN), International Iberian Nanotechnology Laboratory (INL), Centre de Recherche en Information Biomédicale sino-français (CRIBS), Université de Rennes (UR)-Southeast University [Jiangsu]-Institut National de la Santé et de la Recherche Médicale (INSERM), Institut Européen des membranes (IEM), Université Montpellier 2 - Sciences et Techniques (UM2)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Alexander, T, Alton, D, Arisaka, K, Back, Ho, Beltrame, P, Benziger, J, Bonfini, G, Brigatti, A, Brodsky, J, Bussino, Severino Angelo Maria, Cadonati, L, Calaprice, F, Candela, A, Cao, H, Cavalcante, P, Chepurnov, A, Chidzik, S, Cocco, Ag, Condon, C, D'Angelo, D, Davini, S, DE VINCENZI, Mario, De Haas, E, Derbin, A, Di Pietro, G, Dratchnev, I, Durben, D, Empl, A, Etenko, A, Fan, A, Fiorillo, G, Franco, D, Fomenko, K, Forster, G, Gabriele, F, Galbiati, C, Gazzana, S, Ghiano, C, Goretti, A, Grandi, L, Gromov, M, Guan, M, Guo, C, Guray, G, Hungerford, Ev, Ianni, Al, Ianni, An, Joliet, C, Kayunov, A, Keeter, K, Kendziora, C, Kidner, S, Klemmer, R, Kobychev, V, Koh, G, Komor, M, Korablev, D, Korga, G, Li, P, Loer, B, Lombardi, P, Love, C, Ludhova, L, Luitz, S, Lukyanchenko, L, Lund, A, Lung, K, Ma, Y, Machulin, I, Mari, Stefano Maria, Maricic, J, Martoff, Cj, Meregaglia, A, Meroni, E, Meyers, P, Mohayai, T, Montanari, D, Montuschi, M, Monzani, Me, Mosteiro, P, Mount, B, Muratova, V, Nelson, A, Nemtzow, A, Nurakhov, N, Orsini, M, Ortica, F, Pallavicini, M, Pantic, E, Parmeggiano, S, Parsells, R, Pelliccia, N, Perasso, L, Perasso, S, Perfetto, F, Pinsky, L, Pocar, A, Pordes, S, Randle, K, Ranucci, G, Razeto, A, Romani, A, Rossi, B, Rossi, N, Rountree, Sd, Saggese, P, Saldanha, R, Salvo, C, Sands, W, Seigar, M, Semenov, D, Shields, E, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Sukhotin, S, Suvarov, Y, Tartaglia, R, Tatarowicz, J, Testera, G, Thompson, J, Tonazzo, A, Unzhakov, E, Vogelaar, Rb, Wang, H, Westerdale, S, Wojcik, M, Wright, A, Xu, J, Yang, C, Zavatarelli, S, Zehfus, M, Zhong, W, Zuzel, G., Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Dip. di Fisica dell'Università di Genova - Italy, Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Southeast University [Jiangsu]-Institut National de la Santé et de la Recherche Médicale (INSERM), and Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut de Chimie du CNRS (INC)-Université de Montpellier (UM)
Subjects: Physics::Instrumentation and Detectors, Dark matter, chemistry.chemical_element, 7. Clean energy, 01 natural sciences, Nuclear physics, 0103 physical sciences, Neutron, Dark Matter detector, 010306 general physics, Instrumentation, Mathematical Physics, ComputingMilieux_MISCELLANEOUS, Event reconstruction, Physics, [PHYS]Physics [physics], Scintillation, Argon, Time projection chamber, 010308 nuclear & particles physics, Detector, chemistry, Scintillation counter, High Energy Physics::Experiment, Noble liquid detector, DarkSide detector, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: "The DarkSide staged program utilizes a two-phase time projection chamber (TPC) with liquid argon as the target material for the scattering of dark matter particles. Efficient background reduction is achieved using low radioactivity underground argon as well as several experimental handles such as pulse shape, ratio of ionization over scintillation signal, 3D event reconstruction, and active neutron and muon vetos. The DarkSide-10 prototype detector has proven high scintillation light yield, which is a particularly important parameter as it sets the energy threshold for the pulse shape discrimination technique. The DarkSide-50 detector system, currently in commissioning phase at the Gran Sasso Underground Laboratory, will reach a sensitivity to dark matter spin-independent scattering cross section of 10(-45) cm(2) within 3 years of operation."
Published: 2013

18. DarkSide-50 : a WIMP search with a two-phase argon TPC

Author: P.D. Meyers, P. Agnes, D. Alton, K. Arisaka, H.O. Back, B. Baldin, K. Biery, G. Bonfini, M. Bossa, A. Brigatti, J. Brodsky, F. Budano, L. Cadonati, F. Calaprice, N. Canci, A. Candela, H. Cao, M. Cariello, P. Cavalcante, A. Chavarria, A. Chepurnov, A.G. Cocco, L. Crippa, D. DAngelo, M. D’Incecco, S. Davini, M. De Deo, A. Derbin, F. Di Eusanio, G. Di Pietro, E. Edkins, A. Empl, A. Fan, G. Fiorillo, K. Fomenko, G. Forster, D. Franco, F. Gabriele, C. Galbiati, A. Goretti, L. Grandi, M. Gromov, M. Guan, Y. Guardincerri, B. Hackett, K. Herner, P. Humble, E.V. Hungerford, Al. Ianni, An. Ianni, C. Joliet, K. Keeter, C. Kendziora, S. Kidner, V. Kobychev, G. Koh, D. Korablev, G. Korga, A. Kurlej, P. Li, B. Loer, P. Lombardi, C. Love, L. Ludhova, S. Luitz, Y. Ma, I. Machulin, A. Mandarano, S. Mari, J. Maricic, C.J. Martoff, A. Meregaglia, E. Meroni, R. Milincic, D. Montanari, M. Montuschi, M.E. Monzani, P. Mosteiro, B. Mount, V. Muratova, P. Musico, A. Nelson, M. Okounkova, M. Orsini, F. Ortica, L. Pagani, M. Pallavicini, E. Pantic, L. Papp, S. Parmeggiano, R. Parsells, K. Pelczar, N. Pelliccia, S. Perasso, F. Perfetto, A. Pocar, S. Pordes, H. Qian, K. Randle, G. Ranucci, A. Razeto, B. Reinhold, A. Romani, B. Rossi, N. Rossi, S.D. Rountree, D. Sablone, P. Saggese, R. Saldanha, W. Sands, E. Segreto, D. Semenov, E. Shields, M. Skorokhvatov, O. Smirnov, A. Sotnikov, Y. Suvarov, R. Tartaglia, J. Tatarowicz, G. Testera, A. Tonazzo, E. Unzhakov, R.B. Vogelaar, M. Wada, H. Wang, Y. Wang, A. Watson, R. Westerdale, M. Wojcik, A. Wright, J. Xu, C. Yang, J. Yoo, S. Zavatarelli, G. Zuzel, Agnes, P., Alton, D., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Cadonati, L., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Cavalcante, P., Chavarria, A., Chepurnov, A., Cocco, A. G., Crippa, L., Dangelo, D., D’Incecco, M., Davini, S., De Deo, M., Derbin, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B., Herner, K., Humble, P., Hungerford, E. V., Ianni, A., Joliet, C., Keeter, K., Kendziora, C., Kidner, S., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P., Loer, B., Lombardi, P., Love, C., Ludhova, L., Luitz, S., Ma, Y., Machulin, I., Mandarano, A., Mari, S., Maricic, J., Martoff, C. J., Meregaglia, A., Meroni, E., Meyers, P. D., Milincic, R., Montanari, D., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B., Muratova, V., Musico, P., Nelson, A., Okounkova, M., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Papp, L., Parmeggiano, S., Parsells, R., Pelczar, K., Pelliccia, N., Perasso, S., Perfetto, F., Pocar, A., Pordes, S., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Segreto, E., Semenov, D., Shields, E., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Suvarov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Wang, H., Wang, Y., Watson, A., Westerdale, R., Wojcik, M., Wright, A., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zuzel, G., Mari, Stefano Maria, and The Darkside, Collaboration
Subjects: Physics, Cryostat, Argon, Time projection chamber, chemistry.chemical_element, WIMP Argon Programme, Scintillator, Physics and Astronomy(all), Nuclear physics, Physics and Astronomy (all), chemistry, WIMP, pacs:95.35.+d, 29.40.Mc, Neutron, Cherenkov radiation
Abstract: DarkSide-50 is a two phase argon TPC for direct dark matter detection which is installed at the Gran Sasso underground laboratory, Italy. DarkSide-50 has a 50-kg active volume and will make use of underground argon low in 39 Ar. The TPC is installed inside an active neutron veto made with boron-loaded high radiopurity liquid scintillator. The neutron veto is installed inside a 1000 m 3 water Cherenkov muon veto. The DarkSide-50 TPC and cryostat are assembled in two radon-free clean rooms to reduce radioactive contaminants. The overall design aims for a background free exposure after selection cuts are applied. The expected sensitivity for WIMP-nucleon cross section is of the order of 10 −45 cm 2 for WIMP masses around 100 GeV/c 2 . The commissioning and performance of the detector are described. Details of the low-radioactivity underground argon and other unique features of the projects are reported.
Published: 2015

19. Advances in High Energy Physics

Author: Jilei Xu, O. Smirnov, A. Alton, Y. Suvurov, Nicomede Pelliccia, B. Reinhold, N. Canci, D. A. Semenov, D. Sablone, M. D. Skorokhvatov, L. Grandi, M. Montuschi, An. Ianni, Mariano Cadoni, E. Pantic, K. Herner, P. J. Mosteiro, L. Crippa, I. N. Machulin, A. Nelson, Bob Parsells, G. Lukyachenko, Al. Ianni, Y. Q. Ma, L. Marini, M. Bossa, Peter Daniel Meyers, John L. Orrell, V. N. Muratova, E. Segreto, D. M. Asner, G. Zuzel, N. Rossi, A. Mandarano, R. Milincic, Hui Wang, Henning O. Back, M. Wada, K. Biery, J. Yoo, Marco Pallavicini, Stefano Maria Mari, S. Westerdale, Y. Guardincerri, E. Edkins, A. Fan, S. Parmeggiano, D. A. Pugachev, D. D'Angelo, F. Budano, Livia Ludhova, L. Perasso, A. Kurlej, R. Tartaglia, Alan Watson, V. V. Kobychev, A. M. Goretti, A. S. Chepurnov, G. Forster, M. Orsini, D. E. Jaffe, F. Di Eusanio, M. De Deo, K. Arisaka, E. Meroni, J. Tatarowicz, Aldo Romani, A. V. Derbin, G. Fiorillo, K. Fomenko, P. Humble, S. Kidner, P. Agnes, Gioacchino Ranucci, D. Franco, S. Davini, Marcin Wójcik, E. V. Unzhakov, E. V. Hungerford, W. Zhong, Cécile Jollet, A. Devoto, Samuele Sangiorgio, Sandra Zavatarelli, M. Cariello, L. Pagani, C. L. Kendziora, M. D'Incecco, Anselmo Meregaglia, P. X. Li, T. Miletic, H. Qian, A. Sotnikov, P. Saggese, J. Brodsky, E. Shields, Craig E. Aalseth, W. Sands, S. Perasso, B. Rossi, G. Bonfini, B. Yu, K. Recine, H. Cao, K. Randle, B. Baldin, Andrzej Odrzywolek, R. Saldanha, S. Walker, R. Williams, Marcello Lissia, S. D. Rountree, S. Pordes, F. Gabriele, Michael Foxe, Paolo Lombardi, D. Markov, B. R. Hackett, G. Koh, A. Empl, S. Odrowski, M. E. Monzani, A. Tonazzo, Yanchu Wang, A. Pocar, A. Candela, Chung-Yao Yang, G. Testera, Augusto Brigatti, C. Condon, K. Pelczar, Cristiano Galbiati, P. Musico, J. Martoff, M. Gromov, D. Montanari, Andrew Hime, M. Smallcomb, J. Maricic, S. Luitz, A. Razeto, B. J. Mount, A. G. Cocco, D. Korablev, K. J. Keeter, Frank Calaprice, R. B. Vogelaar, Laura Cadonati, A. L. Renshaw, Fausto Ortica, P. Cavalcante, Min-Xin Guan, G. Korga, Aalseth, Ce, Agnes, P, Alton, A, Arisaka, K, Asner, Dm, Back, Ho, Baldin, B, Biery, K, Bonfini, G, Bossa, M, Brigatti, A, Brodsky, J, Budano, F, Cadonati, L, Cadoni, M, Calaprice, F, Canci, N, Candela, A, Cao, H, Cariello, M, Cavalcante, P, Chepurnov, A, Cocco, Ag, Condon, C, Crippa, L, D'Angelo, D, D'Incecco, M, Davini, S, De Deo, M, Derbin, A, Devoto, A, Di Eusanio, F, Edkins, E, Empl, A, Fan, A, Fiorillo, Giuliana, Fomenko, K, Forster, G, Foxe, M, Franco, D, Gabriele, F, Galbiati, C, Goretti, A, Grandi, L, Gromov, M, Guan, My, Guardincerri, Y, Hackett, B, Herner, K, Hime, A, Humble, P, Hungerford, E, Ianni, A, Jaffe, De, Jollet, C, Keeter, K, Kendziora, C, Kidner, S, Kobychev, V, Koh, G, Korablev, D, Korga, G, Kurlej, A, Li, Px, Lissia, M, Lombardi, P, Ludhova, L, Luitz, S, Lukyachenko, G, Ma, Yq, Machulin, I, Mandarano, A, Mari, Sm, Maricic, J, Marini, L, Markov, D, Martoff, J, Meregaglia, A, Meroni, E, Meyers, Pd, Miletic, T, Milincic, R, Montuschi, M, Monzani, Me, Mosteiro, P, Mount, B, Muratova, V, Musico, P, Montanari, D, Nelson, A, Odrowski, S, Odrzywolek, A, Orrell, Jl, Orsini, M, Ortica, F, Pagani, L, Pallavicini, M, Pantic, E, Parmeggiano, S, Parsells, B, Pelczar, K, Pelliccia, N, Perasso, S, Perasso, L, Pocar, A, Pordes, S, Pugachev, D, Qian, H, Randle, K, Ranucci, G, Razeto, A, Recine, K, Reinhold, B, Renshaw, A, Romani, A, Rossi, N, Rossi, B, Rountree, Sd, Sablone, D, Saggese, P, Saldanha, R, Sands, W, Sangiorgio, S, Segreto, E, Semenov, D, Shields, E, Skorokhvatov, M, Smallcomb, M, Smirnov, O, Sotnikov, A, Suvurov, Y, Tartaglia, R, Tatarowicz, J, Testera, G, Tonazzo, A, Unzhakov, E, Vogelaar, Rb, Wada, M, Walker, Susan Elizabeth, Wang, H, Wang, Y, Watson, Aw, Westerdale, S, Williams, R, Wojcik, M, Xu, J, Yang, Cg, Yoo, J, Yu, B, Zavatarelli, S, Zhong, Wl, Zuzel, G., Aalseth, C. E., Agnes, P., Alton, A., Arisaka, K., Asner, D. M., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, Maria, Brigatti, A., Brodsky, J., Budano, Federico, Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Cavalcante, P., Chepurnov, A., Cocco, A. G., Condon, C., Crippa, L., D’Angelo, D., D’Incecco, M., Davini, S., De Deo, M., Derbin, A., Devoto, A., Di Eusanio, F., Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Forster, G., Foxe, M., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Gromov, M., Guan, M. Y., Guardincerri, Y., Hackett, B., Herner, K., Hime, A., Humble, P., Hungerford, E., Ianni, A. l., Ianni, A. n., Jaffe, D. E., Jollet, C., Keeter, K., Kendziora, C., Kidner, S., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P. X., Lissia, M., Lombardi, P., Ludhova, L., Luitz, S., Lukyachenko, G., Ma, Y. Q., Machulin, I., Mandarano, A., Mari, S. M., Maricic, J., Marini, L., Markov, D., Martoff, J., Meregaglia, A., Meroni, E., Meyers, P. D., Miletic, T., Milincic, R., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B., Muratova, V., Musico, P., Montanari, D., Nelson, A., Odrowski, S., Odrzywolek, A., Orrell, J. L., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Parsells, B., Pelczar, K., Pelliccia, N., Perasso, S., Perasso, L., Pocar, A., Pordes, S., Pugachev, D., Qian, H., Randle, K., Ranucci, G., Razeto, A., Recine, K., Reinhold, B., Renshaw, A., Romani, A., Rossi, N., Rossi, B., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Segreto, E., Semenov, D., Shields, E., Skorokhvatov, M., Smallcomb, M., Smirnov, O., Sotnikov, A., Suvurov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Walker, S. E., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Williams, R., Wojcik, M., Xu, J., Yang, C. G., Yoo, J., Yu, B., Zavatarelli, S., Zhong, W. L., and Physics
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, GRAN SASSO, Time projection chamber, Article Subject, Detector, Dark matter, Observable, DarkSide, Scintillator, 7. Clean energy, lcsh:QC1-999, WIMP, Weakly interacting massive particles, LIQUID ARGON, lcsh:Physics
Abstract: Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (ud_less_than100 keV) nuclear recoils. The DarkSide program aims at the WIPMs detection using a liquid argon time projection chamber (LAr-TPC). In this paper we quickly review the DarkSide program focusing in particular on the next generation experiment DarkSide-G2, a 3.6-ton LAr-TPC. The different detector components are described as well as the improvements needed to scale the detector from DarkSide-50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented. Published version
Published: 2015

20. Precision Muon Reconstruction in Double Chooz

Author: Stefan Schoppmann, Yuri Kamyshkov, P.-J. Chang, M. Obolensky, H. de Kerret, M. Vivier, Kazuhiro Terao, L. N. Kalousis, J. Maricic, Marcos Cerrada, N. Vassilopoulos, M. Elnimr, Christopher Wiebusch, C. Grant, S. Shimojima, M. D. Skorokhvatov, Michael Wurm, Cécile Jollet, B. Reinhold, H. Watanabe, V. Zimmer, G. A. Valdiviesso, BayarJon Paul Lubsandorzhiev, S. Perasso, G. A. Horton-Smith, M. C. Goodman, J.V. Dawson, A. S. Cucoanes, E. Blucher, A. Osborn, E. Chauveau, Daniel M. Kaplan, T. Miletic, Zelimir Djurcic, R. Milincic, R. Carr, R. Roncin, G. Yang, L. Goodenough, R. Santorelli, M. Kuze, Christian Buck, Ying Sun, B. Rybolt, E. Damon, V. Sibille, J. Reichenbacher, A. Tonazzo, D. Kryn, S. Roth, A.V. Etenko, Eric Baussan, P. Novella, Luis González, G. Pronost, D. Dietrich, Thierry Lasserre, J. M. LoSecco, M. Franke, A. Hourlier, Lydie Giot, Anselmo Meregaglia, T. Hara, J. Maeda, J. C. Barriere, I. M. Pepe, J. Martino, P. Chimenti, Tobias Lachenmaier, Y. Sakamoto, T.J.C. Bezerra, J. C. dos Anjos, G. Mention, S. Lucht, T. Matsubara, David Lhuillier, Marcos Dracos, I. Stancu, A.C. Schilithz, Yoshio Abe, Janet Conrad, J. M. López-Castaño, Lothar Oberauer, S. Schönert, S. M. Fernandes, H. Furuta, Anatael Cabrera, P. Pfahler, C. E. Lane, I. Bekman, Achim Stahl, R. Sharankova, S. V. Sukhotin, E. Smith, J. Dhooghe, L. B. Bezrukov, M. Röhling, Muriel Fallot, E. Caden, J. Haser, E. Conover, M. H. Shaevitz, A. Onillon, L. Camilleri, T. Kawasaki, A. Stüken, A. Minotti, C. Palomares, V. Fischer, N. Haag, M. Göger-Neff, Florian Kaether, C. Veyssiere, Michael Hofmann, J. Felde, D. Franco, V. V. Sinev, Masaki Ishitsuka, Audrey Letourneau, Lindley Winslow, Yasushi Nagasaka, E. Kemp, D. Shrestha, M. Bergevin, F. Suekane, L.F.F. Stokes, T. Sumiyoshi, K. Crum, J. I. Crespo-Anadón, Amanda Porta, J. Spitz, Y. Nikitenko, I. Gil-Botella, C. Mariani, Josef Jochum, F. Yermia, Matthew L Strait, Robert Svoboda, F. von Feilitzsch, H. P. Lima, J. Busenitz, Sebastian Wagner, Manfred Lindner, Antoine Collin, N. Walsh, H. H. Trinh Thi, Double Chooz Collaboration, Département d'Ingénierie des Systèmes (ex SIS) (DIS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Max-Planck-Institut, Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Département de Physique des Particules (ex SPP) (DPP), Département de Physique Nucléaire (ex SPhN) (DPHN), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Double Chooz, Massachusetts Institute of Technology. Department of Physics, Massachusetts Institute of Technology. Laboratory for Nuclear Science, Conrad, Janet Marie, Spitz, Joshua B., Terao, Kazuhiro, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Double-CHOOZ, Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Abe, Y, Dos Anjos, J, Barriere, J, Baussan, E, Bekman, I, Bergevin, M, Bezerra, T, Bezrukov, L, Blucher, E, Buck, C, Busenitz, J, Cabrera, A, Caden, E, Camilleri, L, Carr, R, Cerrada, M, Chang, P, Chauveau, E, Chimenti, P, Collin, A, Conover, E, Conrad, J, Crespo-Anadon, J, Crum, K, Cucoanes, A, Damon, E, Dawson, J, Dhooghe, J, Dietrich, D, Djurcic, Z, Dracos, M, Elnimr, M, Etenko, A, Fallot, M, Von Feilitzsch, F, Felde, J, Fernandes, S, Fischer, V, Franco, D, Franke, M, Furuta, H, Gil-Botella, I, Giot, L, Goger-Neff, M, Gonzalez, L, Goodenough, L, Goodman, M, Grant, C, Haag, N, Hara, T, Haser, J, Hofmann, M, Horton-Smith, G, Hourlier, A, Ishitsuka, M, Jochum, J, Jollet, C, Kaether, F, Kalousis, L, Kamyshkov, Y, Kaplan, D, Kawasaki, T, Kemp, E, De Kerret, H, Kryn, D, Kuze, M, Lachenmaier, T, Lane, C, Lasserre, T, Letourneau, A, Lhuillier, D, Lima, J, Lindner, M, Lopez-Castano, J, Losecco, J, Lubsandorzhiev, B, Lucht, S, Maeda, J, Mariani, C, Maricic, J, Martino, J, Matsubara, T, Mention, G, Meregaglia, A, Miletic, T, Milincic, R, Minotti, A, Nagasaka, Y, Nikitenko, Y, Novella, P, Oberauer, L, Obolensky, M, Onillon, A, Osborn, A, Palomares, C, Pepe, I, Perasso, S, Pfahler, P, Porta, A, Pronost, G, Reichenbacher, J, Reinhold, B, Rohling, M, Roncin, R, Roth, S, Rybolt, B, Sakamoto, Y, Santorelli, R, Schilithz, A, Schonert, S, Schoppmann, S, Shaevitz, M, Sharankova, R, Shimojima, S, Shrestha, D, Sibille, V, Sinev, V, Skorokhvatov, M, Smith, E, Spitz, J, Stahl, A, Stancu, I, Stokes, L, Strait, M, Stuken, A, Suekane, F, Sukhotin, S, Sumiyoshi, T, Sun, Y, Svoboda, R, Terao, K, Tonazzo, A, Trinh Thi, H, Valdiviesso, G, Vassilopoulos, N, Veyssiere, C, Vivier, M, Wagner, S, Walsh, N, Watanabe, H, Wiebusch, C, Winslow, L, Wurm, M, Yang, G, Yermia, F, and Zimmer, V
Subjects: Nuclear and High Energy Physics, Particle physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, STRIPS, Double Chooz, Muon reconstruction, Neutrino detector, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], CHOOZ, Scintillator, High Energy Physics - Experiment, law.invention, NO, Nuclear physics, High Energy Physics - Experiment (hep-ex), law, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation, Image resolution, Physics, Muon, Detector, Reconstruction algorithm, Instrumentation and Detectors (physics.ins-det), Physics::Accelerator Physics, High Energy Physics::Experiment
Abstract: We describe a muon track reconstruction algorithm for the reactor anti-neutrino experiment Double Chooz. The Double Chooz detector consists of two optically isolated volumes of liquid scintillator viewed by PMTs, and an Outer Veto above these made of crossed scintillator strips. Muons are reconstructed by their Outer Veto hit positions along with timing information from the other two detector volumes. All muons are fit under the hypothesis that they are through-going and ultrarelativistic. If the energy depositions suggest that the muon may have stopped, the reconstruction fits also for this hypothesis and chooses between the two via the relative goodness-of-fit. In the ideal case of a through-going muon intersecting the center of the detector, the resolution is ∼40 mm in each transverse dimension. High quality muon reconstruction is an important tool for reducing the impact of the cosmogenic isotope background in Double Chooz., National Science Foundation (U.S.), United States. Department of Energy
Published: 2014

21. Ortho-positronium observation in the Double Chooz experiment

Author: R. Milincic, Christian Buck, B. Rybolt, S. V. Sukhotin, A. Minotti, Ernesto Kemp, Cécile Jollet, D. Dietrich, M. Röhling, Matthew L Strait, N. Haag, G. Pronost, E. Damon, J. Martino, E. Caden, S. Lucht, A.V. Etenko, Masahiro Kuze, Eric Baussan, E. Chauveau, L. B. Bezrukov, Michael Wurm, H. Watanabe, M. Obolensky, Kazuhiro Terao, G. Mention, Christopher Wiebusch, G. A. Valdiviesso, P. Novella, R. Sharankova, Lydie Giot, L.N. Kalousis, S. Shimojima, Achim Stahl, Michael H. Shaevitz, M. Göger-Neff, Takeo Kawasaki, V. Zimmer, I. Stancu, K. Crum, Z. Djurcic, D. Lhuillier, M. Cerrada, P. Chimenti, V. Sinev, A. S. Cucoanes, G. A. Horton-Smith, M. Skorokhvatov, R. Carr, Bayarto Lubsandorzhiev, H. Furuta, A. Tonazzo, C. Mariani, Thierry Lasserre, A. Onillon, Josef Jochum, J. I. Crespo-Anadón, Y. Kamyshkov, J. Busenitz, L. Camilleri, C. Palomares, J. C. Barriere, J. Reichenbacher, Lindley Winslow, H. H. Trinh Thi, F. von Feilitzsch, Anatael Cabrera, Luis González, N. Vassilopoulos, J.V. Dawson, Yasushi Nagasaka, J. Dhooghe, E. Conover, R. Santorelli, T.J.C. Bezerra, V. Fischer, J. Haser, J. Maricic, M. Franke, M. Vivier, Stefan Schoppmann, I. M. Pepe, Eluned Smith, D. Kryn, T. Sumiyoshi, Y. Sakamoto, C. E. Lane, T. Miletic, A. Osborn, M. Ishitsuka, F. Suekane, F. Yermia, L.F.F. Stokes, Sebastian Wagner, Manfred Lindner, Antoine Collin, Y. Nikitenko, P. Pfahler, V. Sibille, T. Hara, Alain Letourneau, E. Blucher, N. Walsh, J. Maeda, L. Goodenough, S. M. Fernandes, I. Gil-Botella, L. Oberauer, C. Veyssiere, J. C. dos Anjos, Amanda Porta, Maury Goodman, Tobias Lachenmaier, Yoshio Abe, A. Hourlier, Daniel M. Kaplan, Janet Conrad, S. Perasso, Anselmo Meregaglia, H. de Kerret, R. Roncin, T. Matsubara, Ying Sun, B. Reinhold, Stefan Schönert, John M. LoSecco, M. Elnimr, Michael Hofmann, C. Grant, D. Shrestha, J. Spitz, M. Bergevin, Stefan Roth, A.C. Schilithz, I. Bekman, A. Stüken, P.-J. Chang, J. M. López-Castaño, Muriel Fallot, Florian Kaether, J. Felde, D. Franco, Robert Svoboda, H. P. Lima, M. Dracos, G. Yang, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Département de Physique Nucléaire (ex SPhN) (DPHN), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Département d'Ingénierie des Systèmes (ex SIS) (DIS), Massachusetts Institute of Technology. Department of Physics, Massachusetts Institute of Technology. Laboratory for Nuclear Science, Conrad, Janet, Spitz, Joshua B., Terao, K., Winslow, Lindley, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Center for Neutrino Physics, Abe, Y, Dos Anjos, J, Barriere, J, Baussan, E, Bekman, I, Bergevin, M, Bezerra, T, Bezrukov, L, Blucher, E, Buck, C, Busenitz, J, Cabrera, A, Caden, E, Camilleri, L, Carr, R, Cerrada, M, Chang, P, Chauveau, E, Chimenti, P, Collin, A, Conover, E, Conrad, J, Crespo-Anado, J, Crum, K, Cucoanes, A, Damon, E, Dawson, J, Dhooghe, J, Dietrich, D, Djurcic, Z, Dracos, M, Elnimr, M, Etenko, A, Fallot, M, Von Feilitzsch, F, Felde, J, Fernandes, S, Fischer, V, Franco, D, Franke, M, Furuta, H, Gil-Botella, I, Giot, L, Goger-Neff, M, Gonzalez, L, Goodenough, L, Goodman, M, Grant, C, Haag, N, Hara, T, Haser, J, Hofmann, M, Horton-Smith, G, Hourlier, A, Ishitsuka, M, Jochum, J, Jollet, C, Kaether, F, Kalousis, L, Kamyshkov, Y, Kaplan, D, Kawasaki, T, Kemp, E, De Kerret, H, Kryn, D, Kuze, M, Lachenmaier, T, Lane, C, Lasserre, T, Letourneau, A, Lhuillier, D, Lima, H, Lindner, M, Lopez-Castano, J, Losecco, J, Lubsandorzhiev, B, Lucht, S, Maeda, J, Mariani, C, Maricic, J, Martino, J, Matsubara, T, Mention, G, Meregaglia, A, Miletic, T, Milincic, R, Minotti, A, Nagasaka, Y, Nikitenko, Y, Novella, P, Oberauer, L, Obolensky, M, Onillon, A, Osborn, A, Palomares, C, Pepe, I, Perasso, S, Pfahler, P, Porta, A, Pronost, G, Reichenbacher, J, Reinhold, B, Rohling, M, Roncin, R, Roth, S, Rybolt, B, Sakamoto, Y, Santorelli, R, Schilithz, A, Schonert, S, Schoppmann, S, Shaevitz, M, Sharankova, R, Shimojima, S, Shrestha, D, Sibille, V, Sinev, V, Skorokhvatov, M, Smith, E, Spitz, J, Stahl, A, Stancu, I, Stokes, L, Strait, M, Stuken, A, Suekane, F, Sukhotin, S, Sumiyoshi, T, Sun, Y, Svoboda, R, Terao, K, Tonazzo, A, Thi, H, Valdiviesso, G, Vassilopoulos, N, Veyssiere, C, Vivier, M, Wagner, S, Walsh, N, Watanabe, H, Wiebusch, C, Winslow, L, Wurm, M, Yang, G, Yermia, F, Zimmera, V, Double Chooz Collaboration, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: Physics, Neutrino Detectors and Telescopes, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Neutrino Detectors and Telescope, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Electron, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Scintillator, CHOOZ, Particle identification, High Energy Physics - Experiment, Positronium, Nuclear physics, High Energy Physics - Experiment (hep-ex), Positron, Inverse beta decay, High Energy Physics::Experiment, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: The Double Chooz experiment measures the neutrino mixing angle θ13 by detecting reactor ν¯e via inverse beta decay. The positron-neutron space and time coincidence allows for a sizable background rejection, nonetheless liquid scintillator detectors would profit from a positron/electron discrimination, if feasible in large detector, to suppress the remaining background. Standard particle identification, based on particle dependent time profile of photon emission in liquid scintillator, can not be used given the identical mass of the two particles. However, the positron annihilation is sometimes delayed by the ortho-positronium (o-Ps) metastable state formation, which induces a pulse shape distortion that could be used for positron identification. In this paper we report on the first observation of positronium formation in a large liquid scintillator detector based on pulse shape analysis of single events. The o-Ps formation fraction and its lifetime were measured, finding the values of 44% ± 12% (sys.) ± 5% (stat.) and 3.68ns ± 0.17ns (sys.) ± 0.15ns (stat.) respectively, in agreement with the results obtained with a dedicated positron annihilation lifetime spectroscopy setup., National Science Foundation (U.S.), United States. Dept. of Energy
Published: 2014

22. Journal of High Energy Physics

Author: G. Mention, R. Svoboda, T. Kawasaki, P. Novella, J. Dhooghe, N. Vassilopoulos, Amanda Porta, D. Kryn, Zelimir Djurcic, N. Walsh, J. Reichenbacher, J. M. López-Castaño, H. de Kerret, H. H. Trinh Thi, R. Milincic, Yuri Kamyshkov, Muriel Fallot, J. Martino, A. Cucoanes, S. Shimojima, A.C. Schilithz, P.-J. Chang, A. Onillon, L. B. Bezrukov, I. Bekman, J.V. Dawson, G. A. Horton-Smith, M. Franke, Anatael Cabrera, R. Carr, A. Stüken, S. M. Fernandes, K. Crum, Florian Kaether, E. Blucher, J. I. Crespo-Anadón, Y. Nikitenko, T. Sumiyoshi, S. Perasso, A. Minotti, Alain Letourneau, J. Felde, D. Franco, Marcos Cerrada, M. Elnimr, V. V. Sinev, Eric Baussan, Marcos Dracos, David Lhuillier, Ernesto Kemp, L. Camilleri, E. Damon, R. Sharankova, V. Fischer, J. Maricic, Manfred Lindner, J. C. dos Anjos, Antoine Collin, D. Shrestha, M. Obolensky, R. Santorelli, Luis González, Cécile Jollet, B. Reinhold, E. Conover, M. Bergevin, Yoshio Abe, L. N. Kalousis, T.J.C. Bezerra, S. Lucht, S. Roth, J. M. LoSecco, Anselmo Meregaglia, J. Spitz, Lothar Oberauer, Daniel M. Kaplan, C. Palomares, A. Stahl, Y. Sakamoto, I. Gil-Botella, V. Zimmer, C. Grant, C. Veyssiere, Tobias Lachenmaier, V. Sibille, S. V. Sukhotin, E. Smith, H. P. Lima, A. Osborn, M. Kuze, N. Haag, Christian Buck, B. Rybolt, R. Roncin, J. C. Barriere, J. Busenitz, Ying Sun, C. Mariani, A. Hourlier, Lydie Giot, M. Röhling, Josef Jochum, Junpei Maeda, L. Goodenough, F. von Feilitzsch, D. Dietrich, Michael Hofmann, Stefan Wagner, Matthew L Strait, Janet Conrad, T. Hara, A. Tonazzo, M. Göger-Neff, Kazuhiro Terao, Christopher Wiebusch, Yasushi Nagasaka, G. A. Valdiviesso, S. Schönert, M. C. Goodman, T. Miletic, F. Yermia, I. M. Pepe, P. Chimenti, G. Pronost, P. Pfahler, C. E. Lane, T. Matsubara, E. Chauveau, M. H. Shaevitz, E. Caden, Masaki Ishitsuka, Lindley Winslow, Stefan Schoppmann, J. Haser, M. Vivier, M. D. Skorokhvatov, Michael Wurm, H. Watanabe, G. Yang, Bayarto Lubsandorzhiev, Thierry Lasserre, F. Suekane, L.F.F. Stokes, A.V. Etenko, I. Stancu, H. Furuta, Double Chooz Collaboration, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Double-CHOOZ, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Abe, Y, dos Anjos, J, Barriere, J, Baussan, E, Bekman, I, Bergevin, M, Bezerra, T, Bezrukov, L, Blucher, E, Buck, C, Busenitz, J, Cabrera, A, Caden, E, Camilleri, L, Carr, R, Cerrada, M, Chang, P, Chauveau, E, Chimenti, P, Collin, A, Conover, E, Conrad, J, Crespo-Anadon, J, Crum, K, Cucoanes, A, Damon, E, Dawson, J, Dhooghe, J, Dietrich, D, Djurcic, Z, Dracos, M, Elnimr, M, Etenko, A, Fallot, M, von Feilitzsch, F, Felde, J, Fernandes, S, Fischer, V, Franco, D, Franke, M, Furuta, H, Gil-Botella, I, Giot, L, Goger-Neff, M, Gonzalez, L, Goodenough, L, Goodman, M, Grant, C, Haag, N, Hara, T, Haser, J, Hofmann, M, Horton-Smith, G, Hourlier, A, Ishitsuka, M, Jochum, J, Jollet, C, Kaether, F, Kalousis, L, Kamyshkov, Y, Kaplan, D, Kawasaki, T, Kemp, E, de Kerret, H, Kryn, D, Kuze, M, Lachenmaier, T, Lane, C, Lasserre, T, Letourneau, A, Lhuillier, D, Lima, H, Lindner, M, Lopez-Castano, J, Losecco, J, Lubsandorzhiev, B, Lucht, S, Maeda, J, Mariani, C, Maricic, J, Martino, J, Matsubara, T, Mention, G, Meregaglia, A, Miletic, T, Milincic, R, Minotti, A, Nagasaka, Y, Nikitenko, Y, Novella, P, Oberauer, L, Obolensky, M, Onillon, A, Osborn, A, Palomares, C, Pepe, I, Perasso, S, Pfahler, P, Porta, A, Pronost, G, Reichenbacher, J, Reinhold, B, Rohling, M, Roncin, R, Roth, S, Rybolt, B, Sakamoto, Y, Santorelli, R, Schilithz, A, Schonert, S, Schoppmann, S, Shaevitz, M, Sharankova, R, Shimojima, S, Shrestha, D, Sibille, V, Sinev, V, Skorokhvatov, M, Smith, E, Spitz, J, Stahl, A, Stancu, I, Stokes, L, Strait, M, Stuken, A, Suekane, F, Sukhotin, S, Sumiyoshi, T, Sun, Y, Svoboda, R, Terao, K, Tonazzo, A, Trinh Thi, H, Valdiviesso, G, Vassilopoulos, N, Veyssiere, C, Vivier, M, Wagner, S, Walsh, N, Watanabe, H, Wiebusch, C, Winslow, L, Wurm, M, Yang, G, Yermia, F, Zimmer, V, Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Center for Neutrino Physics
Subjects: Nuclear and High Energy Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Physics - Instrumentation and Detectors, Neutrino Detectors and Telescope, FOS: Physical sciences, CHOOZ, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Experiment, Distortion, 0103 physical sciences, Energy spectrum, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], High Energy Physics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Mixing (physics), Physics, Neutrino Detectors and Telescopes, 010308 nuclear & particles physics, Oscillation, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Detector, Function (mathematics), Instrumentation and Detectors (physics.ins-det), Neutrino, Instrumentation and Detectors
Abstract: The Double Chooz experiment presents improved measurements of the neutrino mixing angle $\theta_{13}$ using the data collected in 467.90 live days from a detector positioned at an average distance of 1050 m from two reactor cores at the Chooz nuclear power plant. Several novel techniques have been developed to achieve significant reductions of the backgrounds and systematic uncertainties with respect to previous publications, whereas the efficiency of the $\bar\nu_{e}$ signal has increased. The value of $\theta_{13}$ is measured to be $\sin^{2}2\theta_{13} = 0.090 ^{+0.032}_{-0.029}$ from a fit to the observed energy spectrum. Deviations from the reactor $\bar\nu_{e}$ prediction observed above a prompt signal energy of 4 MeV and possible explanations are also reported. A consistent value of $\theta_{13}$ is obtained from a fit to the observed rate as a function of the reactor power independently of the spectrum shape and background estimation, demonstrating the robustness of the $\theta_{13}$ measurement despite the observed distortion., Comment: 44 pages, 25 figures. Figures 21 and 22 have been replaced (statistical error bars for bins above 8 MeV have become smaller). No other changes in the results of the paper; an Erratum submitted to JHEP
Published: 2014

23. The DarkSide Program

Author: Giovanni Covone, Min-Xin Guan, A. V. Derbin, G. Korga, L. Grandi, S. Luitz, B. Reinhold, K. Fomenko, M. Orsini, N. Rossi, Jingke Xu, A. L. Renshaw, G. Testera, Cristiano Galbiati, J. Yoo, Michele Montuschi, S. Catalanotti, I. N. Machulin, D. Korablev, A. G. Cocco, Marco Pallavicini, M. E. Monzani, L. Marini, M. Bossa, D. D'Angelo, G. Bonfini, K. Randle, S. Perasso, M. Cariello, L. Pagani, P. Cavalcante, A. Zec, Nicomede Pelliccia, A. Pocar, Anton Empl, S. Pordes, A. Kurlej, C. J. Martoff, B. Rossi, S. Parmeggiano, O. Smirnov, Paolo Musico, A. Fan, Hui Wang, A. Candela, Stuart Derek Walker, D. Montanari, Alan Watson, Frank Calaprice, X. Xiang, K. Arisaka, R. B. Vogelaar, J. Tatarowicz, G. Fiorillo, F. Di Eusanio, A. Razeto, J. Maricic, E. Segreto, C. L. Kendziora, A. Mandarano, Aldo Romani, Gioacchino Ranucci, Henning O. Back, P. D. Meyers, P. Agnes, F. Budano, R. Tartaglia, M. Wada, M. D'Incecco, M. De Deo, D. Franco, H. Qian, Y. Guardincerri, Marcin Wójcik, A. Devoto, L. Papp, C. Zhu, R. Saldanha, K. Biery, S. D. Rountree, Sandra Zavatarelli, P. X. Li, Paolo Lombardi, W. Sands, A. Tonazzo, Fausto Ortica, B. R. Hackett, G. Koh, F. Gabriele, D. Sablone, An. Ianni, A. K. Alton, A. E. Chavarria, B. Baldin, Chung-Yao Yang, Augusto Brigatti, E. Pantic, Al. Ianni, E. Edkins, Stefano Maria Mari, E. V. Unzhakov, C. Stanford, J. Brodsky, K. Herner, E. Shields, N. Canci, T. Alexander, S. Odrowski, Y. Suvorov, S. Westerdale, G. Zuzel, A. M. Goretti, A. S. Chepurnov, E. V. Hungerford, A. Sotnikov, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Piattelli, P., Rossi, B., Agnes, P., Alexander, T., Alton, A., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Calaprice, F., Canci, N., Candela, A., Cariello, M., Cavalcante, P., Catalanotti, S., Chavarria, A., Chepurnov, A., Cocco, A. G., Covone, G., D'Angelo, D., D'Incecco, M., Deo, M. De, Derbin, A., Devoto, A., Eusanio, F. Di, Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Guan, M. Y., Guardincerri, Y., Hackett, B., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., Kendziora, C., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P. X., Lombardi, P., Luitz, S., Machulin, I., Mandarano, A., Mari, S., Maricic, J., Marini, L., Martoff, C. J., Meyers, P. D., Montanari, D., Montuschi, M., Monzani, M. E., Musico, P., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Papp, L., Parmeggiano, S., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A., Romani, A., Rossi, N., Rountree, S. D., Sablone, D., Saldanha, R., Sands, W., Segreto, E., Shields, E., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Walker, S., Wang, H., Watson, A., Westerdale, S., Wojcik, M., Xiang, X., Xu, J., Yang, C. G., Yoo, J., Zavatarelli, S., Zec, A., Zhu, C., and Zuzel, G.
Subjects: Particle physics, Physics::Instrumentation and Detectors, QC1-999, Dark matter, chemistry.chemical_element, Cryogenics, DarkSide, dark matter: direct detection, 01 natural sciences, Nuclear physics, Physics and Astronomy (all), 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment, 010303 astronomy & astrophysics, Physics, Time projection chamber, Argon, 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, time projection chamber: liquid argon, Gran Sasso, chemistry, Liquid argon, Underground laboratory, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], performance, experimental results
Abstract: International audience; DarkSide-50 at Gran Sasso underground laboratory (LNGS), Italy, is a direct dark matter search experiment based on a liquid argon TPC. DS-50 has completed its first dark matter run using atmospheric argon as target. The detector performances and the results of the first physics run are presented in this proceeding.
Published: 2014

24. Neutrinos from the primary proton–proton fusion process in the Sun

Author: E. Litvinovich, N. Rossi, F. Mantovani, S. Perasso, S. V. Sukhotin, G. Korga, B. Caccianiga, A. Wright, O. Zaimidoroga, V. V. Kobychev, Matthias Laubenstein, I. N. Machulin, Marco Pallavicini, D. D'Angelo, M. D. Skorokhvatov, Michael Wurm, G. Bonfini, M. Buizza Avanzini, Frank Calaprice, Paolo Lombardi, T. Lewke, E. Meroni, Jay Burton Benziger, Q. Meindl, Hardy Simgen, S. Gazzana, P. Cavalcante, S. Nisi, Denis Korablev, D. Kryn, Aldo Ianni, P. J. Mosteiro, M. Misiaszek, R. Tartaglia, E. Guardincerri, A. Pocar, S. Davini, L. Grandi, G. Bellini, S. Hardy, V. Chubakov, Lothar Oberauer, M. Obolensky, W. Maneschg, S. Manecki, O. Smirnov, G. Testera, K. Otis, Jingke Xu, Cristiano Galbiati, Marcello Lissia, J. Winter, R. Saldanha, Y. Suvorov, C. Ghiano, Livia Ludhova, Lino Miramonti, A. M. Goretti, A. S. Chepurnov, Marcin Wójcik, D. Franco, R. B. Vogelaar, Alessandra Re, Marco Giammarchi, Andrea Ianni, D. Bick, Sandra Zavatarelli, S. Schönert, A. A. Sabelnikov, G. Xhixha, A. V. Derbin, D. Montanari, B. Loer, Gioacchino Ranucci, Aldo Romani, V. N. Muratova, M. Göger-Neff, A. E. Chavarria, L. Perasso, A.V. Etenko, D. Bravo, C. Salvo, F. von Feilitzsch, Laura Cadonati, L. Papp, Fausto Ortica, K. Fomenko, G. Manuzio, F. Lombardi, A. Razeto, Yusuke Koshio, G. Zuzel, A. Sotnikov, C. Carraro, Borexino Collaboration, Bellini, G., Suvorov, Y., Et, Al., Dipartimento di Fisica, Universita degli Studi e INFN, 20133 Milano, Italy., Chemical Engineering Department, Princeton University, Institut für Theoretische Physik, Universität Hamburg, Istituto Nazionale di Fisica Nucleare, Sezione di L'Aquila (INFN), Physics Department, Virginia Polytechnic Institute and State University, Blacksburg, Physics Department, University of Massachusetts, Amherst, Massachusetts 01003, USA., Princeton University Observatory, Dipartimento di Fisica, Università di Genova e Sezione INFN, Lomonosov Moscow State University Skobeltsyn Institute of Nuclear Physics, 119234 Moscow, Russia., Department of Physics, University of Houston, St Petersburg Nuclear Physics Institute, 188350 Gatchina, Russia., National Research Centre Kurchatov Institute, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Physik-Department and Excellence Cluster Universe, Technische Universitat Munchen, 85748 Garching, Germany., Kiev Institute for Nuclear Research, Joint Institute for Nuclear Research (JINR), Department of Physics, Technische Universitat Dresden, 01062 Dresden, Germany., Max-Planck-Institut fur Kernphysik, 69117 Heidelberg, Germany., Gran Sasso Science Institute, M. Smoluchowski Institute of Physics, Jagellonian University, Dipartimento di Chimica, Biologia e Biotecnologie, Universita degli Studi e INFN, 06123 Perugia, Italy., University of California, Los Angeles (UCLA), and Johannes Gutenberg - Universität Mainz = Johannes Gutenberg University (JGU)
Subjects: Physics, Particle physics, Multidisciplinary, Proton, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Solar neutrino problem, Nuclear physics, Neutrino detector, Physics::Space Physics, Astrophysics::Solar and Stellar Astrophysics, Measurements of neutrino speed, Astrophysics::Earth and Planetary Astrophysics, Neutrino astronomy, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Nuclear Experiment, Borexino
Abstract: International audience; In the core of the Sun, energy is released through sequences of nuclear reactions that convert hydrogen into helium. The primary reaction is thought to be the fusion of two protons with the emission of a low-energy neutrino. These so-called pp neutrinos constitute nearly the entirety of the solar neutrino flux, vastly outnumbering those emitted in the reactions that follow. Although solar neutrinos from secondary processes have been observed, proving the nuclear origin of the Sun's energy and contributing to the discovery of neutrino oscillations, those from proton-proton fusion have hitherto eluded direct detection. Here we report spectral observations of pp neutrinos, demonstrating that about 99 per cent of the power of the Sun, 3.84 × 1033 ergs per second, is generated by the proton-proton fusion process.
Published: 2014

25. A first walk on the DarkSide

Author: K. Arisaka, Hui Wang, G. Fiorillo, Thomas Alexander, C. J. Martoff, G. Bonfini, Frank Calaprice, M. D'Incecco, X. Xiang, H. Qian, M. Orsini, W. Sands, D. Franco, E. Shields, Y. Suvorov, S. Westerdale, L. Marini, M. Bossa, A. M. Goretti, A. S. Chepurnov, E. Pantic, B. Rossi, P. D. Meyers, G. Korga, N. Rossi, E. Segreto, Nicomede Pelliccia, Al. Ianni, E. Edkins, E. V. Hungerford, A. Candela, A. Mandarano, M. Wada, Alan Watson, Jingke Xu, Cristiano Galbiati, R. B. Vogelaar, L. Papp, S. Odrowski, Stefano Maria Mari, Anton Empl, Y. Guardincerri, S. Parmeggiano, G. Testera, Fausto Ortica, M. Cariello, B. R. Hackett, M. M. Wojcik, S. Luitz, A. L. Renshaw, G. Koh, A. Sotnikov, J. Yoo, A. Zec, K. Randle, D. Sablone, S. Pordes, C. Stanford, Denis Korablev, Henning O. Back, J. Brodsky, An. Ianni, I. N. Machulin, M. E. Monzani, K. Fomenko, F. Budano, A. Pocar, B. Baldin, A. Devoto, R. Saldanha, Min-Xin Guan, O. Smirnov, D. D'Angelo, Sandra Zavatarelli, P. X. Li, S. Davini, S. D. Rountree, Michele Montuschi, B. Reinhold, E. V. Unzhakov, Paolo Lombardi, J. Tatarowicz, A. E. Chavarria, J. Maricic, M. De Deo, K. Herner, N. Canci, A. Kurlej, G. Zuzel, Gioacchino Ranucci, F. Gabriele, K. Biery, A. Tonazzo, Stuart Derek Walker, C. L. Kendziora, D. Montanari, F. Di Eusanio, Aldo Romani, P. Agnes, Paolo Musico, A. Fan, A. Razeto, A. G. Cocco, A. K. Alton, Chung-Yao Yang, A. V. Derbin, Augusto Brigatti, C. Zhu, L. Grandi, L. Pagani, P. Cavalcante, S. Perasso, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Davini, S, Agnes, P., Alexander, T., Alton, A., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Calaprice, F., Canci, N., Candela, A., Cariello, M., Cavalcante, P., Chavarria, A., Chepurnov, A., Cocco, A. G., D'Angelo, D., D'Incecco, M., De Deo, M., Derbin, A., Devoto, A., Di Eusanio, F., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Guan, M. Y., Guardincerri, Y., Hackett, B., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., Kendziora, C., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P. X., Lombardi, P., Luitz, S., Machulin, I., Mandarano, A., Mari, S., Maricic, J., Marini, L., Martoff, C. J., Meyers, P. D., Montanari, D., Montuschi, M., Monzani, M. E., Musico, P., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pantic, E., Papp, L., Parmeggiano, S., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saldanha, R., Sands, W., Segreto, E., Shields, E., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Walker, S., Wang, H., Watson, A., Westerdale, S., Wojcik, M., Xiang, X., Xu, J., Yang, C. G., Yoo, J., Zavatarelli, S., Zec, A., Zhu, C., Zuzel, G., and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: Particle physics, Nuclear and High Energy Physics, Large Underground Xenon experiment, detector: performance, scintillation detectors, Dark matter, talk: Valencia 2014/07/02, chemistry.chemical_element, DarkSide, Scintillation detectors, 01 natural sciences, dark matter, argon: target, Nuclear physics, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, Physics, Argon, Time projection chamber, 010308 nuclear & particles physics, Detector, liquid argon, time projection chamber, Gran Sasso, Scintillation detector, chemistry, atmosphere, Cryogenic Dark Matter Search, Dark Matter Time Projection Chamber, experimental results
Abstract: International audience; DarkSide-50 (DS-50) at Gran Sasso underground laboratory (LNGS), Italy, is a direct dark matter search experiment based on a TPC with liquid argon. DS-50 has completed its first dark matter run using atmospheric argon as target. The DS-50 detector performances and the results of the first physics run are reviewed in this proceeding.
Published: 2014

26. Lifetimes of 214Po and 212Po measured with Counting Test Facility at Gran Sasso National Laboratory

Author: C. Carraro, G. Testera, A. V. Derbin, Denis Korablev, Livia Ludhova, A. M. Goretti, E. Guardincerri, R. Saldanha, A. E. Chavarria, L. Perasso, B. Loer, M. Buizza Avanzini, A.V. Etenko, A. Chepurnov, Marco Giammarchi, S. Gazzana, Y. Suvorov, D. Bravo, G. Bonfini, M. M. Wojcik, Yusuke Koshio, M. D. Skorokhvatov, Michael Wurm, Frank Calaprice, L. Grandi, J. Winter, Aldo Romani, V. Chubakov, Hardy Simgen, M. Obolensky, Lothar Oberauer, S. Davini, Andrea Ianni, D. Bick, Sandra Zavatarelli, P. J. Mosteiro, Matthias Laubenstein, G. Korga, T. Lewke, K. Fomenko, D. Kryn, Laura Cadonati, L. Papp, S. Sch ̈onert, S. Perasso, C. Salvo, V. N. Muratova, M. G ̈oger-Neff, A. A. Sabelnikov, E. Meroni, Fausto Ortica, E. Litvinovich, N. Rossi, F. Lombardi, B. Caccianiga, A. Razeto, I. N. Machulin, Marco Pallavicini, D. D'Angelo, S. V. Sukhotin, A. Wright, Gioacchino Ranucci, O. Zaimidoroga, Q. Meindl, F. von Feilitzsch, Fabio Mantovani, D. Montanari, V. V. Kobychev, Paolo Lombardi, C. Ghiano, R. Tartaglia, A. Pocar, Gerti Xhixha, O. Smirnov, K. Otis, P. Cavalcante, M. Misiaszek, W. Maneschg, Stefano Nisi, G. Zuzel, A. Sotnikov, Jingke Xu, Cristiano Galbiati, Alessandra Re, Aldo Ianni, R. B. Vogelaar, G. Manuzio, S. Manecki, Jay Burton Benziger, S. Hardy, Marcello Lissia, D. Franco, G. Bellini, and Lino Miramonti
Subjects: Polonium, Physics, Test facility, Health, Toxicology and Mutagenesis, Lead Radioisotopes, General Medicine, Alfa-decay lifetime, Alpha Particles, Pollution, Bi–Po coincidence, Nuclear physics, ^{214}Po, Radiation Monitoring, ^{212}Po, natural radioactivity, Underground laboratory, Environmental Chemistry, Laboratories, National laboratory, Waste Management and Disposal, Half-Life, Radioactive Pollutants
Abstract: The decays of 214 Po into 210 Pb and of 212 Po into 208 Pb tagged by the previous decays from 214 Bi and 212 Bi have been studied inserting quartz vials inside the Counting Test Facility (CTF) at the underground laboratory in Gran Sasso (LNGS). We find that the mean lifetime of 214 Po is (236.00 ± 0.42(stat) ± 0.15(syst)) μs and that of 212 Po is (425.1 ± 0.9(stat) ± 1.2(syst)) ns. Our results are compatible with previous measurements, have a much better signal to background ratio, and reduce the overall uncertainties.
Published: 2014

27. New limits on heavy sterile neutrino mixing inB8decay obtained with the Borexino detector

Author: A. M. Goretti, Aldo Ianni, Anton Empl, R. Tartaglia, S. V. Sukhotin, A. Wright, O. Zaimidoroga, A.V. Etenko, Jingke Xu, S. Schönert, Cristiano Galbiati, D. Bravo, V. V. Kobychev, E. V. Hungerford, C. Ghiano, Caren Hagner, P. Cavalcante, I. S. Drachnev, M. Misiaszek, W. Maneschg, P. J. Mosteiro, A. Sotnikov, Gioacchino Ranucci, Laura Cadonati, L. Papp, G. Bellini, D. Franco, M. D. Skorokhvatov, Michael Wurm, L. Grandi, Lothar Oberauer, Paolo Lombardi, Fausto Ortica, Matthias Laubenstein, B. Caccianiga, Andrea Ianni, D. Bick, Sandra Zavatarelli, Y. Suvorov, T. Lewke, D. Kryn, A. V. Derbin, F. Lombardi, Ben Loer, M. Obolensky, Q. Meindl, A. Razeto, G. Lukyanchenko, A. E. Chavarria, L. Perasso, S. Manecki, E. Meroni, M. Buizza Avanzini, V. N. Muratova, S. Gazzana, Lino Miramonti, S. Davini, G. Zuzel, E. Litvinovich, C. Salvo, G. Korga, K. Fomenko, D. Vignaud, N. Rossi, G. Manuzio, G. Bonfini, F. von Feilitzsch, Frank Calaprice, Hardy Simgen, R. Saldanha, J. Winter, M. Göger-Neff, Marco Giammarchi, A. Pocar, O. Smirnov, K. Otis, S. Perasso, M. M. Wojcik, Aldo Romani, Jay Burton Benziger, I. N. Machulin, Livia Ludhova, A. S. Chepurnov, Marco Pallavicini, D. D'Angelo, Denis Korablev, G. Testera, Alessandra Re, and R. B. Vogelaar
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Sterile neutrino, 010308 nuclear & particles physics, 7. Clean energy, 01 natural sciences, Side branch, 0103 physical sciences, High Energy Physics::Experiment, Heavy neutrino, Neutrino, 010306 general physics, Mixing (physics), Borexino
Abstract: If heavy neutrinos with mass ${m}_{{\ensuremath{\nu}}_{H}}\ensuremath{\ge}2{m}_{e}$ are produced in the Sun via the decay $^{8}\mathrm{B}\ensuremath{\rightarrow}^{8}\mathrm{Be}+{e}^{+}+{\ensuremath{\nu}}_{H}$ in a side branch of the $pp$ chain, they would undergo the observable decay into an electron, a positron and a light neutrino ${\ensuremath{\nu}}_{H}\ensuremath{\rightarrow}{\ensuremath{\nu}}_{L}+{e}^{+}+{e}^{\ensuremath{-}}$. In the present work Borexino data are used to set a bound on the existence of such decays. We constrain the mixing of a heavy neutrino with mass $1.5\text{ }\text{ }\mathrm{MeV}\ensuremath{\le}{m}_{{\ensuremath{\nu}}_{H}}\ensuremath{\le}14\text{ }\text{ }\mathrm{MeV}$ to be $|{U}_{eH}{|}^{2}\ensuremath{\le}({10}^{\ensuremath{-}3}\ensuremath{-}4\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}6})$, respectively. These are tighter limits on the mixing parameters than obtained in previous experiments at nuclear reactors and accelerators.
Published: 2013

28. The Waveform Digitiser of the Double Chooz Experiment: Performance and Quantisation Effects on PhotoMultiplier Tube Signals

Author: M. Ishitsuka, R. Roncin, P. Novella, J.V. Dawson, T. Akiri, Anatael Cabrera, B. Courty, A. Hourlier, S. Perasso, M. Obolensky, Yoshio Abe, H. de Kerret, D. Kryn, Luis González, A. Remoto, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Double-CHOOZ, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
Subjects: Physics, Photomultiplier, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, Firmware, business.industry, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), CHOOZ, computer.software_genre, 01 natural sciences, 3. Good health, Pulse charge, Optics, Low light level, 0103 physical sciences, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Waveform, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, business, Instrumentation, computer, Mathematical Physics
Abstract: We present the waveform digitiser used in the Double Chooz experiment. We describe the hardware and the custom-built firmware specifically developed for the experiment. The performance of the device is tested with regards to digitising low light level signals from photomultiplier tubes and measuring pulse charge. This highlights the role of quantisation effects and leads to some general recommendations on the design and use of waveform digitisers., Comment: 14 pages, 8 figures, accepted for publication in JINST
Published: 2013

29. Measurement of ortho-Positronium Properties in Liquid Scintillators

Author: S. Hans, D. Franco, Cécile Jollet, Giovanni Consolati, A. Tonazzo, Anselmo Meregaglia, S. Perasso, Minfang Yeh, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: gas and liquid scintillators), Materials science, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, Phosphor, 02 engineering and technology, Electron, Scintillator, 01 natural sciences, Particle detector, Positronium, High Energy Physics - Experiment, Particle identification methods, High Energy Physics - Experiment (hep-ex), Double beta decay, 0103 physical sciences, 0202 electrical engineering, electronic engineering, information engineering, Neutron detection, Neutrino detectors, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, Mathematical Physics, Physics, Dopant, 010308 nuclear & particles physics, Doping, 020206 networking & telecommunications, Instrumentation and Detectors (physics.ins-det), Particle identification methods, Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators), Neutrino detectors, scintillation and light emission processes (solid, Scintillators, Scintillation counter, 020201 artificial intelligence & image processing, High Energy Physics::Experiment, Atomic physics, Radioactive decay
Abstract: Pulse shape discrimination in liquid scintillator detectors is a well-established technique for the discrimination of heavy particles from light particles. Nonetheless, it is not efficient in the separation of electrons and positrons, as they give rise to indistinguishable scintillator responses. This inefficiency can be overtaken through the exploitation of the formation of ortho-Positronium (o-Ps), which alters the time profile of light pulses induced by positrons. We characterized the o-Ps properties in the most commonly used liquid scintillators, i.e. PC, PXE, LAB, OIL and PC + PPO. In addition, we studied the effects of scintillator doping on the o-Ps properties for dopants currently used in neutrino experiments, Gd and Nd. Further measurements for Li-loaded and Tl-loaded liquid scintillators are foreseen. We found that the o-Ps properties are suitable for enhancing the electron-positron discrimination., 4 pages, 1 figure. Contribution to proceedings of the Low Radioactivity Techniques 2013 Workshop at LNGS, Assergi (AQ), Italy, April 10-12 2013
Published: 2013

30. Cosmogenic Backgrounds in Borexino at 3800 m water-equivalent depth

Author: L. Oberauer, V. N. Muratova, A. E. Chavarria, L. Perasso, A.V. Etenko, D. Bravo, C. Salvo, O. Zaimidoroga, Michael Wurm, L. Grandi, M. Göger-Neff, R. Möllenberg, S. Perasso, R. Tartaglia, S. V. Sukhotin, Laura Cadonati, G. Korga, Andrea Ianni, A. Wright, Jilei Xu, Y. Suvorov, D. Franco, G. Zuzel, Livia Ludhova, G. Testera, Fausto Ortica, A. M. Goretti, V. V. Kobychev, A. S. Chepurnov, A. V. Derbin, K. Otis, I. Machulin, A. Sotnikov, Aldo Ianni, Gioacchino Ranucci, A. Empl, Stefan Schönert, G. Bonfini, P. Cavalcante, S. Davini, Q. Meindl, C. Ghiano, M. Obolensky, W. Maneschg, G. Lukyanchenko, R. Saldanha, P. J. Mosteiro, E. Litvinovich, S. Manecki, G. Bellini, K. Fomenko, F. von Feilitzsch, B. Caccianiga, D. Bick, Sandra Zavatarelli, Marco Giammarchi, J. Winter, Aldo Romani, L. Papp, F. Calaprice, Lino Miramonti, S. Gazzana, Cristiano Galbiati, Oleg Smirnov, N. Rossi, A. Pocar, Caren Hagner, D. Vignaud, Marco Pallavicini, D. D'Angelo, D. Korablev, T. Lewke, E. Hungerford, M. Misiaszek, M. Skorokhvatov, Marcin Wójcik, M. Buizza Avanzini, R. B. Vogelaar, Hardy Simgen, Paolo Lombardi, Alessandra Re, Matthias Laubenstein, A. Razeto, G. Manuzio, D. Kryn, B. Loer, J. Benziger, F. Lombardi, E. Meroni, Physics Department, Amherst U., University of Massachusetts System (UMASS), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratori Nazionali del Gran Sasso (LNGS), Istituto Nazionale di Fisica Nucleare (INFN), Laboratoire Kastler Brossel (LKB (Jussieu)), Université Pierre et Marie Curie - Paris 6 (UPMC)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Dept. Microelectronics and Nanoscience, Chalmers University of Technology [Göteborg], departement de physique, Albert-Ludwigs-Universität Freiburg, Dip. di Fisica dell'Università di Genova - Italy, Università degli studi di Torino (UNITO), Departamento de Engenharia Elétrica [Minas Gerais] (DEE - UFMG), Universidade Federal de Minas Gerais, Rhodes University, Grahamstown, Laboratoire de Spectroscopie Hertzienne de l'ENS (LSH-ENS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Institute of Physics, Polish Academy of Sciences, Polska Akademia Nauk = Polish Academy of Sciences (PAN), International Iberian Nanotechnology Laboratory (INL), Bellini, G., Suvorov, Y., Et, Al., Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Università degli studi di Genova = University of Genoa (UniGe), and Università degli studi di Torino = University of Turin (UNITO)
Subjects: Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Solar neutrino, Monte Carlo method, dark matter experiment, cosmic ray experiment, FOS: Physical sciences, Scintillator, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), neutrino experiments, 0103 physical sciences, Neutron, 010306 general physics, Borexino, ComputingMilieux_MISCELLANEOUS, Physics, [PHYS]Physics [physics], Muon, 010308 nuclear & particles physics, dark matter experiments, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), Neutron capture, Neutrino detector, neutrino experiment, High Energy Physics::Experiment, cosmic ray experiments, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: The solar neutrino experiment Borexino, which is located in the Gran Sasso underground laboratories, is in a unique position to study muon-induced backgrounds in an organic liquid scintillator. In this study, a large sample of cosmic muons is identified and tracked by a muon veto detector external to the liquid scintillator, and by the specific light patterns observed when muons cross the scintillator volume. The yield of muon-induced neutrons is found to be Yn =(3.10+-0.11)10-4 n/({\mu} (g/cm2)). The distance profile between the parent muon track and the neutron capture point has the average value {\lambda} = (81.5 +- 2.7)cm. Additionally the yields of a number of cosmogenic radioisotopes are measured for 12N, 12B, 8He, 9C, 9Li, 8B, 6He, 8Li, 11Be, 10C and 11C. All results are compared with Monte Carlo simulation predictions using the Fluka and Geant4 packages. General agreement between data and simulation is observed for the cosmogenic production yields with a few exceptions, the most prominent case being 11C yield for which both codes return about 50% lower values. The predicted {\mu}-n distance profile and the neutron multiplicity distribution are found to be overall consistent with data., Comment: 26 pages, 13 figures (in 14 files), 4 tables. 3 extra data files. accepted by JCAP
Published: 2013

31. Mass hierarchy discrimination with atmospheric neutrinos in large volume ice/water Cherenkov detectors

Author: V. Kulikovskiy, T. Pradier, A. Tonazzo, Antoine Kouchner, V. Van Elewyck, D. Franco, S. Perasso, Cécile Jollet, A. Meregaglia, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, and Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)
Subjects: Normalization (statistics), Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, FOS: Physical sciences, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), Effective mass (solid-state physics), 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, Cherenkov radiation, Physics, 010308 nuclear & particles physics, Detector, High Energy Physics - Phenomenology, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], Likelihood-ratio test, High Energy Physics::Experiment, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Mass hierarchy
Abstract: Large mass ice/water Cherenkov experiments, optimized to detect low energy (1-20 GeV) atmospheric neutrinos, have the potential to discriminate between normal and inverted neutrino mass hierarchies. The sensitivity depends on several model and detector parameters, such as the neutrino flux profile and normalization, the Earth density profile, the oscillation parameter uncertainties, and the detector effective mass and resolution. A proper evaluation of the mass hierarchy discrimination power requires a robust statistical approach. In this work, the Toy Monte Carlo, based on an extended unbinned likelihood ratio test statistic, was used. The effect of each model and detector parameter, as well as the required detector exposure, was then studied. While uncertainties on the Earth density and atmospheric neutrino flux profiles were found to have a minor impact on the mass hierarchy discrimination, the flux normalization, as well as some of the oscillation parameter (\Delta m^2_{31}, \theta_{13}, \theta_{23}, and \delta_{CP}) uncertainties and correlations resulted critical. Finally, the minimum required detector exposure, the optimization of the low energy threshold, and the detector resolutions were also investigated., Comment: 23 pages, 16 figures
Published: 2013

32. Neutrinos from the sun and from radioactive sources

Author: D. Bravo, S. Schoenert, G. Bellini, F. Lombardi, S. Hardy, S. Perasso, Lino Miramonti, A. Razeto, S. Gazzana, J. Winter, Marco Pallavicini, O. Zaimidoroga, C. Ghiano, C. Salvo, Andrea Ianni, D. Bick, Sandra Zavatarelli, R. S. Raghavan, G. Manuzio, A. V. Derbin, E. Litvinovich, Matthias Laubenstein, A. Kayunov, G. Korga, R. Tartaglia, M. Göger-Neff, R. Saldanha, A. Pocar, E. Guardincerri, An. Ianni, Paolo Lombardi, O. Smirnov, Marco Giammarchi, M. Obolensky, Jay Burton Benziger, S. V. Sukhotin, A. Wright, K. Otis, I. N. Machulin, D. Franco, A. E. Chavarria, G. Zuzel, S. Manecki, V. V. Kobychev, D. Kryn, D. Montanari, B. Loer, D. D'Angelo, L. Perasso, P. J. Mosteiro, E. Meroni, A. A. Sabelnikov, A. Sotnikov, T. Lewke, R. B. Vogelaar, Y. Suvorov, V. N. Muratova, P. Cavalcante, Yusuke Koshio, M. Misiaszek, W. Maneschg, Gioacchino Ranucci, S. Davini, M. D. Skorokhvatov, Michael Wurm, L. Grandi, Jingke Xu, Q. Meindl, Cristiano Galbiati, Alessandra Re, Lothar Oberauer, B. Caccianiga, M. M. Wojcik, D. Vignaud, K. Fomenko, Laura Cadonati, L. Papp, Fausto Ortica, G. Bonfini, M. Buizza Avanzini, Frank Calaprice, Hardy Simgen, F. von Feilitzsch, C. Carraro, P. A. Romani, G. Testera, Denis Korablev, Livia Ludhova, A. M. Goretti, A.V. Etenko, Ianni, A., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Avanzini, M. Buizza, Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Cavalcante, P., Chavarria, A., D'Angelo, D., Davini, S., Derbin, A., Etenko, A., Franco, D., Fomenko, K., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., GOeger-Neff, M., Goretti, A., Grandi, L., Guardincerri, E., Hardy, S., Ianni, Andrea, Kayunov, A., Kobychev, V., Korablev, D., Korga, G., Koshio, Y., Kryn, D., Laubenstein, M., Lewke, T., Litvinovich, E., Ludhova, L., Loer, B., Lombardi, F., Lombardi, P., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Meindl, Q., Meroni, E., Miramonti, L., Misiaszek, M., Montanari, D., Mosteiro, P., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Perasso, L., Perasso, S., Pocar, A., Raghavan, R. S., Ranucci, G., Razeto, A., Re, A., Romani, P. A., Sabelnikov, A., Saldanha, R., Salvo, C., Schoeenert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., Von Feilitzsch, F., Winter, J., Wojcik, M., Wright, A., Wurm, M., Xu, J., Zaimidoroga, O., Zavatarelli, S., and Zuzel, G.
Subjects: Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, neutrino, OSCILLATIONS, Neutrino oscillation, DETECTOR, SOLAR MODELS, Physics, GALLEX, solar neutrino, neutrino oscillations, High Energy Physics::Phenomenology, Astronomy, oscillation, Solar neutrino problem, Atomic and Molecular Physics, and Optics, Cosmic neutrino background, Neutrino detector, sterile neutrino, solar neutrinos, Physics::Space Physics, neutrino source, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Neutrino astronomy, solar standard model
Abstract: A brief review of the solar neutrino observations is given. Future solar neutrino measurements are discussed. The use of an artificial neutrino source to be used with low threshold solar neutrino detectors is presented. At present the neutrino source is mainly planned for short baseline neutrino studies.
Published: 2013

33. Solar neutrino results from Borexino

Author: A. V. Derbin, M. Göger-Neff, A. Kayunov, E. Guardincerri, O. Smirnov, Livia Ludhova, C. Salvo, Matthias Laubenstein, A. M. Goretti, K. Otis, R. B. Vogelaar, Denis Korablev, A. Sotnikov, J. Winter, K. Fomenko, C. Ghiano, E. Meroni, Laura Cadonati, L. Papp, A. Pocar, Marco Pallavicini, P. Cavalcante, Fausto Ortica, C. Carraro, M. Misiaszek, P. A. Romani, K. Simgen, A. A. Sabelnikov, A. E. Chavarria, L. Perasso, R. S. Raghavan, S. Perasso, G. Bellini, G. Manuzio, S. Davini, Gioacchino Ranucci, I. N. Machulin, G. Testera, Lothar Oberauer, Alessandra Re, G. Korga, Lino Miramonti, S. Schönert, D. Kryn, P. J. Mosteiro, Andrea Ianni, Aldo Ianni, S. Gazzana, D. Bick, Sandra Zavatarelli, S. Manecki, G. Zuzel, D. Vignaud, D. Montanari, M. M. Wojcik, Y. Suvorov, V. N. Muratova, M. Buizza Avanzini, D. DʼAngelo, R. Saldanha, Marco Giammarchi, B. Caccianiga, G. Bonfini, D. Franco, Frank Calaprice, Jingke Xu, Cristiano Galbiati, R. Tartaglia, F. von Feilitzsch, A.V. Etenko, D. Bravo, W. Maneschg, M. D. Skorokhvatov, Michael Wurm, L. Grandi, Q. Meindl, S. Hardy, S. V. Sukhotin, A. Wright, O. Zaimidoroga, V. V. Kobychev, M. Obolensky, Paolo Lombardi, F. Lombardi, T. Lewke, A. Razeto, Jay Burton Benziger, E. Litvinovich, B. Loer, Yusuke Koshio, Franco, D., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Avanzini, M. Buizza, Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Cavalcante, P., Chavarria, A., D'Angelo, D., Davini, S., Derbin, A., Etenko, A., Fomenko, K., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-neff, M., Goretti, A., Grandi, L., Guardincerri, E., Hardy, S., Ianni, Aldo, Ianni, Andrea, Kayunov, A., Kobychev, V., Korablev, D., Korga, G., Koshio, Y., Kryn, D., Laubenstein, M., Lewke, T., Litvinovich, E., Ludhova, L., Loer, B., Lombardi, F., Lombardi, P., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Meindl, Q., Meroni, E., Miramonti, L., Misiaszek, M., Montanari, D., Mosteiro, P., Muratova, V., Oberauer, L., Obolenksy, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Perasso, L., Perasso, S., Pocar, A., Raghavan, R. S., Ranucci, G., Razeto, A., Re, A., Romani, P. A., Sabelnikov, A., Saldanha, R., Salvo, C., Schoenert, S., Simgen, K., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., Von Feilitzsch, F., Winter, J., Wojcik, M., Wright, A., Wurm, M., Xu, J., Zaimidoroga, O., Zavatarelli, S., and Zuzel, G.
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Solar neutrino, High Energy Physics::Phenomenology, Solar neutrinos, scintillators, Solar neutrino problem, Atomic and Molecular Physics, and Optics, Nuclear physics, scintillator, Neutrino detector, low background, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Neutrino astronomy, Neutrino oscillation, Borexino
Abstract: Borexino is a large-volume liquid scintillator experiment for low energy neutrino detection, operating since May 2007, and installed at the National Laboratory of Gran Sasso. Borexino is the first experiment able to observe in real-time Solar neutrino interactions also in the sub-MeV range. We report with this work the main results achieved in the Solar neutrino sector by Borexino. In particular, we report the results on the measured interaction rates of 7 Be, 8 B, and pep neutrinos, and their impacts on the physics of neutrino oscillations.
Published: 2013

34. Recent results and future development of Borexino

Author: S. V. Sukhotin, A. Wright, O. Zaimidoroga, I. N. Machulin, V. V. Kobychev, G. Bellini, D. Vignaud, D. D'Angelo, R. B. Vogelaar, G. Bonfini, M. Buizza Avanzini, Frank Calaprice, Hardy Simgen, Jingke Xu, Cristiano Galbiati, D. Montanari, Paolo Lombardi, F. von Feilitzsch, A. Pocar, C. Ghiano, A. Sabelnikov, R. Tartaglia, W. Maneschg, Alessandra Re, C. Carraro, S. Davini, Livia Ludhova, A. M. Goretti, O. Smirnov, K. Otis, M. D. Skorokhvatov, Michael Wurm, L. Grandi, R. S. Raghavan, Lino Miramonti, R. Saldanha, Q. Meindl, D. Kryn, Aldo Ianni, V. N. Muratova, G. Korga, A. V. Derbin, Matthias Laubenstein, S. Schönert, Marco Giammarchi, M. Obolensky, K. Fomenko, D. Franco, S. Hardy, Aldo Romani, Andrea Ianni, D. Bick, Sandra Zavatarelli, Laura Cadonati, L. Papp, E. Guardincerri, S. Manecki, G. Testera, M. M. Wojcik, Fausto Ortica, Gioacchino Ranucci, Denis Korablev, S. Gazzana, G. Manuzio, P. J. Mosteiro, J. Winter, Lothar Oberauer, S. Perasso, Jay Burton Benziger, P. Cavalcante, M. Misiaszek, B. Caccianiga, Y. Suvorov, T. Lewke, A.V. Etenko, D. Bravo, E. Litvinovich, N. Rossi, A. E. Chavarria, L. Perasso, A. Sotnikov, C. Salvo, E. Meroni, F. Lombardi, A. Razeto, G. Zuzel, B. Loer, Yusuke Koshio, Marco Pallavicini, M. Göger-Neff, Pallavicini, M., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Avanzini, M. Buizza, Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Cavalcante, P., Chavarria, A., D'Angelo, D., Davini, S., Derbini, A., Etenko, A., Fomenko, K., Franco, D., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Grandi, L., Guardincerri, E., Hardy, S., Ianni, Aldo, Ianni, Andrea, Kobychev, V., Korablev, D., Korga, G., Koshio, Y., Kryn, D., Laubenstein, M., Lewke, T., Litvinovich, E., Loer, B., Lombardi, P., Lombardi, E., Ludhova, L., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Meindl, Q., Meroni, E., Miramonti, L., Misiaszek, M., Montanan, D., Mosteiro, P., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Papp, L., Perasso, L., Perasso, S., Pocar, A., Raghavan, R. S., Ranucci, G., Razeto, A., Re, A., Romani, A., Rossi, N., Sabelnikov, A., Saldanha, R., Salvo, C., Schoenert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., von Feilitzsch, F., Winter, J., Wojcik, M., Wright, A., Wurm, M., Xu, J., Zaimidoroga, O., Zavatarelli, S., and Zuzel, G.
Subjects: Physics, ICARUS, Solar Neutrino, Nuclear and High Energy Physics, Liquid Scintillator Neutrino Detector, Particle physics, neutrino oscillations, Neutrino oscillation, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, High Energy Physics::Phenomenology, Solar neutrino problem, Atomic and Molecular Physics, and Optics, Nuclear physics, Neutrino detector, solar neutrinos, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino speed, Neutrino astronomy, neutrino speed, Borexino, MSW effect
Abstract: This paper summarizes the main recent results of the Borexino experiment, a liquid scintillator neutrino detector of unprecedented radiopurity currently running at the Laboratori Nazionali del Gran Sasso in Italy. Particularly, the paper is focused on the precision measurement of the 7Be solar neutrino flux, on the search of its day–night modulation, and on the first detection of pep neutrinos. The paper also covers a recent measurement of the CNGS neutrinos speed made in May 2012. A short discussion about the forthcoming scientific program on solar neutrinos, geoneutrinos, and sterile neutrino searches is included at the end.
Published: 2013

35. Lifetime measurements of 214Po and 212Po with the CTF liquid scintillator detector at LNGS

Author: R. B. Vogelaar, Alessandra Re, Matthias Laubenstein, C. Carraro, P. Cavalcante, W. Maneschg, A. Razeto, G. Manuzio, J. Benziger, Michael Wurm, L. Grandi, A. Pocar, V. Chubakov, M. Skorokhvatov, F. Lombardi, D. Korablev, D. Bick, Sandra Zavatarelli, F. von Feilitzsch, Fabio Mantovani, S. Perasso, S. Davini, S. Nisi, G. Zuzel, L. Oberauer, R. Saldanha, S. Manecki, M. Buizza Avanzini, V. N. Muratova, A. E. Chavarria, G. Testera, Hardy Simgen, L. Perasso, A. Sotnikov, Aldo Ianni, Marco Giammarchi, Y. Suvorov, Q. Meindl, A.V. Etenko, Gioacchino Ranucci, D. Kryn, D. Franco, D. Bravo, Aldo Romani, L. Papp, Laura Cadonati, E. Meroni, N. Rossi, Fausto Ortica, I. Machulin, Marco Pallavicini, D. D'Angelo, C. Salvo, O. Zaimidoroga, B. Loer, Yusuke Koshio, Andrea Ianni, M. Obolensky, A. V. Derbin, M. M. Wojcik, Cristiano Galbiati, Oleg Smirnov, G. Bellini, Paolo Lombardi, M. Göger-Neff, E. Guardincerri, S. V. Sukhotin, A. Wright, D. Montanari, V. V. Kobychev, Stefan Schönert, Livia Ludhova, A. A. Sabelnikov, A. M. Goretti, A. S. Chepurnov, S. Hardy, Marcello Lissia, C. Ghiano, Jilei Xu, K. Otis, P. J. Mosteiro, G. Bonfini, Lino Miramonti, T. Lewke, R. Tartaglia, G. Korga, E. Litvinovich, K. Fomenko, S. Gazzana, B. Caccianiga, F. Calaprice, J. Winter, Gerti Xhixha, M. Misiaszek, Borexino Collaboration, Physics Department, University of Massachusetts System (UMASS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratori Nazionali del Gran Sasso (LNGS), Istituto Nazionale di Fisica Nucleare (INFN), Dept. Microelectronics and Nanoscience, Chalmers University of Technology [Göteborg], Paul Scherrer Institute (PSI), Rhodes University, Grahamstown, Laboratoire de Spectroscopie Hertzienne de l'ENS (LSH-ENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), International Iberian Nanotechnology Laboratory (INL), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL), Bellini, G., Suvorov, Y., and Et, Al.
Subjects: Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Nuclear Theory, Hadron, FOS: Physical sciences, Scintillator, 01 natural sciences, Coincidence, Nuclear Theory (nucl-th), Nuclear physics, High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, Nuclear fusion, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, Nuclear theory, ComputingMilieux_MISCELLANEOUS, Physics, [PHYS]Physics [physics], Test facility, 010308 nuclear & particles physics, Detector, Instrumentation and Detectors (physics.ins-det), High Energy Physics - Phenomenology, National laboratory, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: We have studied the alpha decays of 214Po into 210Pb and of 212Po into 208Pb tagged by the coincidence with the preceding beta decays from 214Bi and 212Bi, respectively. The employed 222Rn, 232Th, and 220Rn sources were sealed inside quartz vials and inserted in the Counting Test Facility at the underground Gran Sasso National Laboratory in Italy. We find that the mean lifetime of 214Po is (236.00 +- 0.42(stat) +- 0.15(syst)) \mu s and that of 212Po is (425.1 +- 0.9(stat) +- 1.2(syst)) ns. Our results, obtained from data with signal-to-background ratio larger than 1000, reduce the overall uncertainties and are compatible with previous measurements., Comment: RevTex, 11 pages, 5 figures, 3 tables. This second version matches the one accepted for publication in EPJA: minor stylistic changes plus a discussion of calibration of TDC time scale
Published: 2013

36. SOX : short distance neutrino Oscillations with BoreXino

Author: E. Litvinovich, M. D. Skorokhvatov, Michael Wurm, N. Rossi, G. Lukyanchenko, R. Saldanha, Gioacchino Ranucci, M. Göger-Neff, D. A. Semenov, Lino Miramonti, A. Pocar, D. Korablev, Livia Ludhova, R. Tartaglia, Y. Suvorov, A. M. Goretti, A. S. Chepurnov, G. Bonfini, O. Smirnov, E. Pantic, K. Otis, C. Ghiano, P. J. Mosteiro, Frank Calaprice, Caren Hagner, D. Kryn, Jonathan M. Link, D. Krasnicky, E. V. Unzhakov, F. Lombardi, K. Fomenko, W. Maneschg, Hardy Simgen, L. Papp, P. Cavalcante, Andrea Ianni, D. Bick, Sandra Zavatarelli, Lothar Oberauer, Matthias Laubenstein, I. N. Machulin, M. Misiaszek, Fausto Ortica, S. Manecki, Marco Pallavicini, D. D'Angelo, E. Meroni, E. V. Hungerford, Marcin Wójcik, G. Fernandes, A. Sotnikov, G. Bellini, G. Korga, B. Caccianiga, S. Schönert, A. Razeto, G. Zuzel, R. B. Vogelaar, Alessandra Re, A. Caminata, Aldo Ianni, D. Franco, V. N. Muratova, A. E. Chavarria, C. Salvo, A.V. Etenko, D. Bravo, Aldo Romani, Michael Meyer, S. Davini, S. Perasso, G. Testera, Cristiano Galbiati, A. V. Derbin, Paolo Lombardi, M. Obolensky, S. V. Sukhotin, O. Zaimidoroga, H. Wang, V. V. Kobychev, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratori Nazionali del Gran Sasso (LNGS), Istituto Nazionale di Fisica Nucleare (INFN), Dept. Microelectronics and Nanoscience, Chalmers University of Technology [Göteborg], Paul Scherrer Institute (PSI), Physik-Department E15, Technische Universität Munchen - Université Technique de Munich [Munich, Allemagne] (TUM), Dip. di Fisica dell'Università di Genova - Italy, Università degli studi di Torino (UNITO), Departamento de Engenharia Elétrica [Minas Gerais] (DEE - UFMG), Universidade Federal de Minas Gerais, Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Department of Physics-Electronics, Rhodes University, Grahamstown, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), EAST CHINA UNIVERSITY, KEY LAB, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Università degli studi di Genova = University of Genoa (UniGe), and Università degli studi di Torino = University of Turin (UNITO)
Subjects: Nuclear and High Energy Physics, Sterile neutrino, Particle physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, ddc:530, 010306 general physics, Neutrino oscillation, ComputingMilieux_MISCELLANEOUS, Borexino, [PHYS]Physics [physics], Physics, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, exotics, neutrino detectors and telescopes, Instrumentation and Detectors (physics.ins-det), Solar neutrino problem, oscillation, Neutrino detector, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: The very low radioactive background of the Borexino detector, its large size, and the well proved capability to detect both low energy neutrino and anti-neutrino make an ideal case for the study of short distance neutrino oscillations with artificial sources at Gran Sasso. This paper describes the possible layouts of 51Cr neutrino and 144Ce-144Pr anti-neutrino source experiments in Borexino and shows the expected sensitivity for three possible different phases of the experiment., Comment: 11 pages, 5 figures
Published: 2013

37. First test of Lorentz violation with a reactor-based antineutrino experiment

Author: V. Fischer, P. Novella, T. Sumiyoshi, J. L. Sida, Achim Stahl, Michael H. Shaevitz, G. Keefer, I. Ostrovskiy, A. Bernstein, H. Furuta, T.J.C. Bezerra, E. Damon, A. Onillon, G. Mention, Matthew L Strait, Michael Wurm, H. Watanabe, D. Greiner, D. Lhuillier, K. Nakajima, V. Zimmer, M. Cerrada, A. J. Franke, Z. Djurcic, P. Pfahler, J. Maeda, M. Göger-Neff, Takeo Kawasaki, Iuri Muniz Pepe, R. Gama, M. Bergevin, V. Sinev, M. Skorokhvatov, Bayarto Lubsandorzhiev, M. Röhling, Thierry Lasserre, Th. A. Mueller, G. Pronost, Stefan Roth, J. Reichenbacher, J.V. Dawson, Caren Hagner, J. M. López-Castaño, Muriel Fallot, T. Classen, J. Martino, Anatael Cabrera, Teppei Katori, Florian Kaether, Yu. Efremenko, Y. Kamyshkov, J. Felde, D. Franco, L. Camilleri, C. Palomares, Kazuhiro Terao, A. Stüken, F. Sato, M. Toups, Christopher Wiebusch, E. Conover, G. A. Valdiviesso, Yasushi Nagasaka, J. C. dos Anjos, J. Maricic, H. Miyata, Christian Buck, B. Rybolt, E. Caden, V. Durand, Yoshio Abe, D. McKee, Frank Hartmann, Anna Erickson, C. N. Maesano, F. Suekane, L.F.F. Stokes, C. Mariani, J. Haser, Josef Jochum, D. Dietrich, L. Bezrukhov, F. von Feilitzsch, Lindley Winslow, L. Oberauer, Lydie Giot, S. Dazeley, H. P. Lima, D. Shrestha, M. Elnimr, J. Spitz, C. Aberle, Ernesto Kemp, Stefan Schoppmann, J. Busenitz, Masahiro Kuze, Cécile Jollet, P. Chimenti, T. Matsubara, A. Remoto, A. Hatzikoutelis, H. H. Trinh Thi, R. Milincic, M. Franke, C. E. Lane, M. Ishitsuka, I. Stancu, M. Fechner, M. Worcester, T. Miletic, S. Habib, F. Yermia, M. Dracos, I. Gil-Botella, S. Perasso, C. Veyssiere, P. Perrin, A. Osborn, R. Roncin, Tobias Lachenmaier, Ying Sun, Tomoyuki Konno, Daniel M. Kaplan, A. Tonazzo, Stefan Schönert, John M. LoSecco, M. V. d'Agostino, S. V. Sukhotin, E. Smith, N. Haag, B. Reinhold, S. Lucht, M. Obolensky, G. A. Horton-Smith, L. N. Kalousis, C. L. Jones, Michael Hofmann, T. Schwetz, Luis González, Nathaniel Bowden, A. S. Cucoanes, Janet Conrad, W. Potzel, Manuel Meyer, B. R. White, J. Ebert, Sebastian Wagner, Manfred Lindner, Antoine Collin, E. Blucher, Maury Goodman, P.-J. Chang, K. Crum, E. Yanovitch, R. Carr, Alain Letourneau, D. Kryn, Anselmo Meregaglia, Amanda Porta, J. I. Crespo-Anadón, H. de Kerret, T. Hayakawa, T. Hara, R. Santorelli, J. Tm. Goon, Y. Sakamoto, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Double-CHOOZ, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Double Chooz Collaboration, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Muon, 010308 nuclear & particles physics, Lorentz transformation, FOS: Physical sciences, Electron, Lorentz covariance, CHOOZ, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, symbols.namesake, High Energy Physics - Experiment (hep-ex), Sidereal time, 0103 physical sciences, symbols, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], High Energy Physics::Experiment, 010306 general physics, Neutrino oscillation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Electron neutrino
Abstract: We present a search for Lorentz violation with 8249 candidate electron antineutrino events taken by the Double Chooz experiment in 227.9 live days of running. This analysis, featuring a search for a sidereal time dependence of the events, is the first test of Lorentz invariance using a reactor-based antineutrino source. No sidereal variation is present in the data and the disappearance results are consistent with sidereal time independent oscillations. Under the Standard-Model Extension (SME), we set the first limits on fourteen Lorentz violating coefficients associated with transitions between electron and tau flavor, and set two competitive limits associated with transitions between electron and muon flavor., Comment: 6 pages, 2 figures; (new version after referee's comments)
Published: 2012

38. The DarkSide-50 outer detectors

Author: J. Maricic, S. Perasso, S. Walker, I. N. Machulin, N. Canci, Marco Pallavicini, D. D'Angelo, L. Grandi, Nicomede Pelliccia, K. Arisaka, C. Stanford, G. Fiorillo, A. M. Goretti, S. De Cecco, B. Reinhold, Anton Empl, M. M. Wojcik, Gioacchino Ranucci, S. Luitz, M. Cariello, Thomas Alexander, A. Brigatti, C. Giganti, Laura Cadonati, M. D'Incecco, Anselmo Meregaglia, Jingke Xu, W. Sands, H. Qian, C. J. Martoff, G. Bonfini, C. Savarese, K. J. Keeter, G. Zuzel, M. Orsini, Han Wang, L. Marini, Frank Calaprice, E. V. Hungerford, X. Xiang, E. Pantic, Sandra Zavatarelli, G. Testera, M. Bossa, F. Granato, B. Rossi, D. Franco, A. S. Kubankin, R. Tartaglia, A. Sotnikov, W. Zhong, K. Pelczar, Caoxiang Zhu, M. Cadeddu, Y. Suvorov, Cristiano Galbiati, S. Westerdale, P. J. Mosteiro, Michele Montuschi, E. Shields, Alan Watson, A. Mandarano, A. Monte, Cécile Jollet, Min-Xin Guan, S. Bussino, S. Catalanotti, Fausto Ortica, B. Bottino, S. M. Mari, A. Razeto, A. S. Chepurnov, Mariano Cadoni, Griffin Foster, P. Cavalcante, A. G. Cocco, B. Vogelaar, M. Lissia, C. L. Kendziora, Irina James, Henning O. Back, J. Tatarowicz, N. Rossi, M DSkorokhvatov, Xiujiang Li, H. Cao, T. Miletic, B. Baldin, V. N. Muratova, K. Biery, Yanchu Wang, Samuele Sangiorgio, L. Agostino, E. Edkins, Ianni Aldo, K. Herner, P. D. Meyers, R. Saldanha, J. Wilhelmi, M. Wada, S. Davini, F. Di Eusanio, Y. Guardincerri, M. De Vincenzi, Yanhui Ma, M. De Deo, A. L. Renshaw, Ivone F. M. Albuquerque, Aldo Romani, M. Gromov, P. Agnes, Ianni Andrea, J. Yoo, R. Milincic, Denis Korablev, F. Gabriele, E. Segreto, J. Brodsky, Jim Napolitano, P. Saggese, A. Tonazzo, M. Carlini, Paolo Musico, P. N. Singh, A. Fan, D. A. Pugachev, G. Di Pietro, Giovanni Covone, V. V. Kobychev, G. Koh, K. Fomenko, F. Budano, A. Devoto, S. D. Rountree, Paolo Lombardi, B. R. Hackett, A. Zec, S. Pordes, D. Sablone, A. Candela, L. Pagani, D. Montanari, P Trinchese, Chung-Yao Yang, A. V. Derbin, A. K. Alton, B. J. Mount, M. E. Monzani, A. Pocar, O. Smirnov, S. Parmeggiano, E. V. Unzhakov, G. Korga, K. Randle, A. Vishneva, D. A. Semenov, Darkside Collaboration, The, Westerdale, S., Agnes, P., Agostino, L., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, Federico, Bussino, Severino Angelo Maria, Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., D'Angelo, D., D'Incecco, M., Davini, S., De Cecco, S., De Deo, M., DE VINCENZI, Mario, Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Foster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K. R., Hungerford, E. V., Aldo, Ianni, Andrea, Ianni, James, Irina, Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, Stefano Maria, Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Dskorokhvatov, M., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., Westerdale, S, Agnes, P, Agostino, L, Albuquerque, I. F. M, Alexander, T, Alton, A. K, Arisaka, K, Back, H. O, Baldin, B, Biery, K, Bonfini, G, Bossa, M, Bottino, B, Brigatti, A, Brodsky, J, Budano, F, Bussino, S, Cadeddu, M, Cadonati, L, Cadoni, M, Calaprice, F, Canci, N, Candela, A, Cao, H, Cariello, M, Carlini, M, Catalanotti, Sergio, Cavalcante, P, Chepurnov, A, Cocco, ALFREDO GIUSEPPE, Covone, Giovanni, D’Angelo, D, D’Incecco, M, Davini, S, De Cecco, S, De Deo, M, De Vincenzi, M, Derbin, A, Devoto, A, Di Eusanio, F, Di Pietro, G, Edkins, E, Empl, A, Fan, A, Fiorillo, Giuliana, Fomenko, K, Foster, G, Franco, D, Gabriele, F, Galbiati, C, Giganti, C, Goretti, A. M, Granato, F, Grandi, L, Gromov, M, Guan, M, Guardincerri, Y, Hackett, B. R, Herner, K. R, Hungerford, E. V, James, I, Jollet, C, Keeter, K, Kendziora, C. L, Kobychev, V, Koh, G, Korablev, D, Korga, G, Kubankin, A, Li, X, Lissia, M, Lombardi, P, Luitz, S, Ma, Y, Machulin, I. N, Mandarano, A, Mari, S. M, Maricic, J, Marini, L, Martoff, C. J, Meregaglia, A, Meyers, P. D, Miletic, T, Milincic, R, Montanari, D, Monte, A, Montuschi, M, Monzani, M. E, Mosteiro, P, Mount, B. J, Muratova, V. N, Musico, P, Napolitano, J, Orsini, M, Ortica, F, Pagani, L, Pallavicini, M, Pantic, E, Parmeggiano, S, Pelczar, K, Pelliccia, N, Perasso, S, Pocar, A, Pordes, S, Pugachev, D. A, Qian, H, Randle, K, Ranucci, G, Razeto, A, Reinhold, B, Renshaw, A. L, Romani, A, Rossi, B, Rossi, N, Rountree, S. D, Sablone, D, Saggese, P, Saldanha, R, Sands, W, Sangiorgio, S, Savarese, C, Segreto, E, Semenov, D. A, Shields, E, Singh, P. N, Dskorokhvatov, M, Smirnov, O, Sotnikov, A, Stanford, C, Suvorov, Y, Tartaglia, R, Tatarowicz, J, Testera, G, Tonazzo, A, Trinchese, P, Unzhakov, E. V, Vishneva, A, Vogelaar, B, Wada, M, Walker, Susan Elizabeth, Wang, H, Wang, Y, Watson, A. W, Wilhelmi, J, Wojcik, M. M, Xiang, X, Xu, J, Yang, C, Yoo, J, Zavatarelli, S, Zec, A, Zhong, W, and Zhu, C
Subjects: Physics, Physics and Astronomy (all), History, Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment, DarkSide, Computer Science Applications, Education
Abstract: DarkSide-50 is a dark matter detection experiment searching for Weakly Interacting Massive Particles (WIMPs), in Gran Sasso National Laboratory. For experiments like DarkSide-50, neutrons are one of the primary backgrounds that can mimic WIMP signals. The experiment consists of three nested detectors: a liquid argon time projection chamber surrounded by two outer detectors. The outermost detector is a 10 m by 11 m cylindrical water Cherenkov detector with 80 PMTs, designed to provide shielding and muon vetoing. Inside the water Cherenkov detector is the 4 m diameter spherical boron-loaded liquid scintillator veto, with a cocktail of pseudocumene, trimethyl borate, and PPO wavelength shifter, designed to provide shielding, neutron vetoing, and in situ measurements of the TPC backgrounds. We present design and performance details of the DarkSide-50 outer detectors.
Published: 2016

39. Borexino calibrations: Hardware, Methods, and Results

Author: Cristiano Galbiati, A. Razeto, E. Litvinovich, R. Saldanha, F. von Feilitzsch, B. Caccianiga, S. Gazzana, F. Calaprice, Marco Giammarchi, D. Vignaud, Laura Cadonati, Livia Ludhova, A. Kayunov, Jilei Xu, T. Lewke, Fausto Ortica, Y. Suvorov, I. Machulin, G. Zuzel, L. Oberauer, P. Cavalcante, R. Tartaglia, K. Otis, S. Kidner, M. Obolensky, A. E. Chavarria, W. Maneschg, M. Goeger-Neff, M. Skorokhvatov, A. Sotnikov, Aldo Ianni, L. Perasso, R. B. Vogelaar, Matthias Laubenstein, V. Muratova, P. J. Mosteiro, A.V. Etenko, Michael Wurm, L. Grandi, Lino Miramonti, Alessandra Re, D. Franco, S. V. Sukhotin, G. Korga, Andrea Ianni, D. Bravo, D. Bick, Sandra Zavatarelli, A. Wright, V. V. Kobychev, A. Pocar, Stefan Schönert, D. Rountree, A. Derbin, R. S. Raghavan, A. Goretti, D. Korablev, D. Kryn, G. Bonfini, C. Ghiano, N. Rossi, E. Meroni, Paolo Lombardi, G. Bellini, Marco Pallavicini, D. D'Angelo, C. Salvo, Marcin Wójcik, S. Manecki, M. Buizza Avanzini, S. Hardy, O. Zaimidoroga, K. Fomenko, Hardy Simgen, S. Davini, J. Benziger, F. Lombardi, Gioacchino Ranucci, C. Carraro, D. Montanari, G. Fernandes, S. Perasso, Q. Meindl, Aldo Romani, L. Papp, E. Guardincerri, G. Manuzio, G. Testera, A. A. Sabelnikov, J. Winter, M. Misiaszek, O. Smirnov, H. O. Back, B. Loer, Yusuke Koshio, Borexino collaboration, H, Back, G, Bellini, Suvorov, Yury, and Et, Al.
Subjects: Calorimeter, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Solar neutrino, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Scintillator, Large detector systems for particle and astroparticle physic, Calibration, Environmental science, Neutrino, Instrumentation, Borexino, Mathematical Physics, Remote sensing
Abstract: Borexino was the first experiment to detect solar neutrinos in real-time in the sub-MeV region. In order to achieve high precision in the determination of neutrino rates, the detector design includes an internal and an external calibration system. This paper describes both calibration systems and the calibration campaigns that were carried out in the period between 2008 and 2011. We discuss some of the results and show that the calibration procedures preserved the radiopurity of the scintillator. The calibrations provided a detailed understanding of the detector response and led to a significant reduction of the systematic uncertainties in the Borexino measurements.
Published: 2012

40. Direct Measurement of Backgrounds using Reactor-Off Data in Double Chooz

Author: J. Maricic, A. Hourlier, Lydie Giot, Matthew L Strait, M. Röhling, A.V. Etenko, J. Ebert, Audrey Letourneau, R. Santorelli, Janet Conrad, I. Stancu, Sebastian Wagner, Manfred Lindner, H. Furuta, Antoine Collin, Daniel M. Kaplan, R. Roncin, E. Blucher, S. Schönert, M. Franke, Ying Sun, T. Hayakawa, S. Dazeley, M. D. Skorokhvatov, Michael Wurm, H. Watanabe, T. Sumiyoshi, T. Konno, D. Kryn, F. Suekane, L.F.F. Stokes, S. Roth, C. Veyssiere, T. Hara, M. Elnimr, B. K. Lubsandorzhiev, A. Bernstein, I. Ostrovskiy, W. Potzel, Th. A. Mueller, T. Miletic, S. Habib, S. M. Fernandes, D. Shrestha, Amanda Porta, R. Gama, Z. Djurcic, E. Damon, S. Perasso, H. Miyata, G. Mention, A. Onillon, A. Cucoanes, K. Nakajima, M. Worcester, Yuri Kamyshkov, D. McKee, Stefan Schoppmann, Christian Buck, Thierry Lasserre, F. Yermia, L. Camilleri, B. Rybolt, A. Remoto, Michael Hofmann, B. White, J. Spitz, P. Novella, J. C. Barriere, C. N. Maesano, D. Dietrich, C. Mariani, T. Kawasaki, Josef Jochum, V. V. Sinev, M. Göger-Neff, P.-J. Chang, V. Durand, A. Hatzikoutelis, P. Perrin, L. Bezrukhov, F. von Feilitzsch, Marcos Cerrada, E. Caden, H. P. Lima, V. Zimmer, David Lhuillier, Lothar Oberauer, J. Reichenbacher, Yasushi Nagasaka, Anatael Cabrera, M. Toups, J. T. M. Goon, A. J. Franke, J. L. Sida, C. Aberle, J. Busenitz, Masahiro Kuze, Anna Erickson, J. M. López-Castaño, J. Haser, S. Shimojima, Muriel Fallot, T. Classen, Michael Fechner, G. A. Horton-Smith, J.V. Dawson, I. M. Pepe, P. Chimenti, C. Palomares, J. M. LoSecco, G. Keefer, T. Matsubara, C. Langbrandtner, E. Kemp, Anselmo Meregaglia, Cécile Jollet, B. Reinhold, Florian Kaether, Y. Kibe, M. Ishitsuka, E. Conover, J. Felde, D. Franco, C. L. Jones, Lindley Winslow, H. H. Trinh Thi, J. Maeda, F. Hartmann, A. Stüken, F. Sato, R. Carr, D. Greiner, I. Gil-Botella, Tobias Lachenmaier, Kazuhiro Terao, L. Goodenough, R. Milincic, Robert Svoboda, Christopher Wiebusch, G. A. Valdiviesso, A. Tonazzo, M. C. Goodman, J. C. dos Anjos, Luis González, Nathaniel Bowden, Thomas Schwetz, Achim Stahl, Yoshio Abe, M. Obolensky, G. Pronost, H. de Kerret, L. N. Kalousis, T.J.C. Bezerra, P. Pfahler, C. E. Lane, A. Osborn, M. V. d'Agostino, S. V. Sukhotin, E. Smith, N. Haag, Manuel Meyer, Marcos Dracos, S. Lucht, V. Fischer, J. Martino, M. Bergevin, K. Crum, J. I. Crespo-Anadón, Y. Sakamoto, M. H. Shaevitz, Yu. Efremenko, Caren Hagner, APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucl'eaire, Atomique et de Spectroscopie, Université de Liège, Double-CHOOZ, Massachusetts Institute of Technology. Department of Physics, Massachusetts Institute of Technology. Plasma Science and Fusion Center, Conrad, Janet, Jones, Christopher LaDon, Spitz, Joshua B., Terao, Yasuaki, Winslow, L., Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Nuclear and High Energy Physics, Particle physics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Daya bay, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, CHOOZ, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), 010306 general physics, Neutrino oscillation, Nuclear Experiment, Physics, Muon, 010308 nuclear & particles physics, Oscillation, Neutron temperature, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], 13. Climate action, High Energy Physics::Experiment, Neutrino
Abstract: Double Chooz is unique among modern reactor-based neutrino experiments studying ν¯e disappearance in that data can be collected with all reactors off. In this paper, we present data from 7.53 days of reactor-off running. Applying the same selection criteria as used in the Double Chooz reactor-on oscillation analysis, a measured background rate of 1.0±0.4 events/day is obtained. The background model for accidentals, cosmogenic β-n-emitting isotopes, fast neutrons from cosmic muons, and stopped-μ decays used in the oscillation analysis is demonstrated to be correct within the uncertainties. Kinematic distributions of the events, which are dominantly cosmic-ray-produced correlated-background events, are provided. The background rates are scaled to the shielding depths of two other reactor-based oscillation experiments, Daya Bay and RENO., United States. Dept. of Energy, National Science Foundation (U.S.)
Published: 2012

41. Reactor ν ̄e disappearance in the Double Chooz experiment

Author: G. Mention, M. Ishitsuka, Matthew L Strait, Tobias Lachenmaier, I. M. Pepe, Daniel M. Kaplan, S. V. Sukhotin, E. Smith, M. V. d'Agostino, H. Miyata, M. Kuze, E. Caden, N. Haag, Christian Buck, A. Hatzikoutelis, S. Dazeley, T. Kawasaki, E. Damon, A.V. Etenko, T. Konno, H. P. Lima, F. Suekane, L.F.F. Stokes, I. Stancu, H. Furuta, L.N. Kalousis, Yuri Kamyshkov, C. N. Maesano, Y. Sakamoto, M. Toups, T. Miletic, P. Novella, D. McKee, D. Dietrich, S. Perasso, J. Busenitz, P.-J. Chang, J. Haser, S. Shimojima, Lindley Winslow, F. Yermia, S. Lucht, G. A. Horton-Smith, Michael Hofmann, A. Bernstein, Anatael Cabrera, P. Perrin, Michael Fechner, David Lhuillier, A. Cucoanes, E. Conover, H. H. Trinh Thi, E. Kemp, Luis González, Nathaniel Bowden, Thomas Schwetz, B. White, T.J.C. Bezerra, A. Remoto, C. L. Jones, A. Onillon, C. Mariani, P. Chimenti, Kazuhiro Terao, Janet Conrad, Marcos Dracos, Josef Jochum, T. Matsubara, T. Hayakawa, I. Gil-Botella, J. Martino, L. Bezrukhov, M. Bergevin, V. V. Sinev, F. von Feilitzsch, M. Obolensky, A. Osborn, H. de Kerret, Christopher Wiebusch, M. D. Skorokhvatov, J. Ebert, Michael Wurm, H. Watanabe, Robert Svoboda, Sebastian Wagner, G. A. Valdiviesso, M. Röhling, D. Kryn, M. C. Goodman, K. Crum, Alain Letourneau, Yu. Efremenko, Manfred Lindner, Antoine Collin, E. Blucher, Zelimir Djurcic, A. Hourlier, Lydie Giot, Stefan Schoppmann, W. Potzel, Caren Hagner, J. I. Crespo-Anadón, R. Gama, Anselmo Meregaglia, M. H. Shaevitz, J. C. dos Anjos, J. M. López-Castaño, Yoshio Abe, Bayarto Lubsandorzhiev, S. Schönert, Lothar Oberauer, C. Palomares, Thierry Lasserre, G. Keefer, V. Zimmer, Muriel Fallot, T. Classen, J. C. Barriere, A. J. Franke, R. Carr, D. Greiner, P. Pfahler, C. E. Lane, L. Camilleri, Florian Kaether, Y. Kibe, F. Hartmann, J. Felde, D. Franco, J.V. Dawson, T. Sumiyoshi, A. Stahl, J. L. Sida, M. Cerrada, Amanda Porta, J. Maricic, A. Stüken, F. Sato, J. Reichenbacher, C. Veyssiere, R. Santorelli, J. Tm. Goon, D. Shrestha, J. Spitz, V. Durand, R. Roncin, Ying Sun, T. Hara, John M. LoSecco, M. Elnimr, R. Milincic, S. Roth, I. Ostrovskiy, M. Franke, Th. A. Mueller, K. Nakajima, C. Aberle, M. Worcester, Cécile Jollet, B. Reinhold, C. Langbrandtner, J. Maeda, A. Tonazzo, M. Göger-Neff, and Yasushi Nagasaka
Subjects: Physics, NOνA, Nuclear and High Energy Physics, Particle physics, 010308 nuclear & particles physics, Detector, CHOOZ, 01 natural sciences, Spectral line, Nuclear physics, 0103 physical sciences, 010306 general physics, Neutrino oscillation, Electron neutrino
Abstract: The Double Chooz experiment has observed 8,249 candidate electron antineutrino events in 227.93 live days with 33.71 GW-ton-years (reactor power x detector mass x livetime) exposure using a 10.3 cubic meter fiducial volume detector located at 1050 m from the reactor cores of the Chooz nuclear power plant in France. The expectation in case of theta13 = 0 is 8,937 events. The deficit is interpreted as evidence of electron antineutrino disappearance. From a rate plus spectral shape analysis we find sin^2 2{\theta}13 = 0.109 \pm 0.030(stat) \pm 0.025(syst). The data exclude the no-oscillation hypothesis at 99.9% CL (3.1{\sigma}).
Published: 2012

42. Measurement of CNGS muon neutrino speed with Borexino

Author: Y. Suvorov, R. Saldanha, S. V. Sukhotin, T. Lewke, S. Hardy, D. Kryn, Matthias Laubenstein, A. Wright, D. Missiaen, O. Zaimidoroga, G. Korga, M. M. Wojcik, Aldo Romani, Marco Giammarchi, V. V. Kobychev, S. Schoenert, Matthew Jones, B. Caccianiga, G. Cerretto, E. Meroni, C. Ghiano, S. Gazzana, E. Litvinovich, N. Rossi, I. N. Machulin, P. Spinnato, C. I. De Gaetani, Marco Pallavicini, D. D'Angelo, P. Cavalcante, V. Pettiti, Alessandra Re, B. Loer, M. Goeger-Neff, M. Misiaszek, P. J. Mosteiro, Paolo Lombardi, Aldo Ianni, M. Obolensky, Yusuke Koshio, S. Manecki, Lothar Oberauer, G. Zuzel, D. Franco, R. S. Raghavan, G. Manuzio, R. B. Vogelaar, M. G. Visconti, B. Betti, Jay Burton Benziger, M. Buizza Avanzini, A. Sotnikov, F. Lombardi, Riccardo Barzaghi, A. Razeto, O. Smirnov, D. Passoni, K. Otis, C. Plantard, K. Fomenko, F. von Feilitzsch, Laura Cadonati, L. Papp, Fausto Ortica, A. Pocar, S. Perasso, S. Davini, C. Carraro, Andrea Ianni, D. Bick, Sandra Zavatarelli, G. Testera, M. D. Skorokhvatov, Michael Wurm, L. Grandi, Q. Meindl, Denis Korablev, G. Bonfini, Hardy Simgen, P. Alvarez Sanchez, R. Tartaglia, Lino Miramonti, W. Maneschg, J. Serrano, A. Kayunov, E. Guardincerri, A. V. Derbin, Ludovico Biagi, Livia Ludhova, D. Vignaud, H. Esteban, A. M. Goretti, Jingke Xu, Cristiano Galbiati, A. A. Sabelnikov, D. Montanari, G. Bellini, A.V. Etenko, J. Winter, D. Bravo, Gioacchino Ranucci, Livio Pinto, V. N. Muratova, A. E. Chavarria, L. Perasso, C. Salvo, AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Borexino, Alvarez Sanchez, P., Suvorov, Y., Et, Al., Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Particle physics, Special relativity, Nuclear and High Energy Physics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, FOS: Physical sciences, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Neutrino beam, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Muon neutrino, Nuclear Experiment, 010306 general physics, Neutrino oscillation, neutrino speed, Borexino, Physics, Muon, GPS time-link, special relativity, 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Neutrino detector, neutrino beams, Measurements of neutrino speed, Physics::Accelerator Physics, Neutrino speed, High Energy Physics::Experiment, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Particle Physics - Experiment
Abstract: We have measured the speed of muon neutrinos with the Borexino detector using short-bunch CNGS beams. The final result for the difference in time-of-flight between a =17 GeV muon neutrino and a particle moving at the speed of light in vacuum is {\delta}t = 0.8 \pm 0.7stat \pm 2.9sys ns, well consistent with zero., Comment: 6 pages, 5 figures
Published: 2012

43. Search for solar axions produced in thep(d,He3)Areaction with Borexino detector

Author: D. Vignaud, M. D. Skorokhvatov, Michael Wurm, L. Grandi, Y. Suvorov, Livia Ludhova, A. M. Goretti, R. B. Vogelaar, Q. Meindl, Matthias Laubenstein, O. Smirnov, A. Kobychev, Denis Korablev, I. N. Machulin, Aldo Ianni, Alessandra Re, K. Otis, L. Lewke, G. Bonfini, G. Korga, K. Fomenko, M. Buizza Avanzini, Marco Pallavicini, D. D'Angelo, Frank Calaprice, R. Tartaglia, G. Bellini, Jingke Xu, Hardy Simgen, P. A. Romani, S. Hardy, E. Meroni, Cristiano Galbiati, S. Manecki, C. Carraro, W. Maneschg, M. Obolensky, J. Winter, S. Davini, G. Testera, D. Kryn, Lino Miramonti, S. Gazzana, A. Pocar, F. von Feilitzsch, R. S. Raghavan, G. Manuzio, Lothar Oberauer, B. Caccianiga, M. Goeger-Neff, M. M. Wojcik, C. Ghiano, E. Litvinovich, A. A. Sabelnikov, Laura Cadonati, L. Papp, Jay Burton Benziger, A. V. Derbin, P. Cavalcante, D. Franco, Fausto Ortica, M. Misiaszek, A. Kayunov, E. Guardincerri, S. Perasso, B. Loer, Paolo Lombardi, S. V. Sukhotin, G. Zuzel, Yusuke Koshio, A. Wright, O. Zaimidoroga, Gioacchino Ranucci, A. Sotnikov, F. Lombardi, A. Razeto, V. N. Muratova, C. Salvo, D. Montanari, A.V. Etenko, D. Bravo, P. J. Mosteiro, A. E. Chavarria, L. Perasso, R. Saldanha, S. Schönert, Marco Giammarchi, Andrea Ianni, D. Bick, and Sandra Zavatarelli
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Isovector, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Inverse, 7. Clean energy, 01 natural sciences, 0103 physical sciences, Nuclear Experiment, 010306 general physics, Axion, Borexino
Abstract: A search for 5.5 MeV solar axions produced in the $p+d\ensuremath{\rightarrow}^{3}\mathrm{He}+\mathrm{A}$ (5.5 MeV) reaction was performed using the Borexino detector. The Compton conversion of axions to photons, $\mathrm{A}+e\ensuremath{\rightarrow}e+\ensuremath{\gamma}$; the axioelectric effect, $\mathrm{A}+e+Z\ensuremath{\rightarrow}e+Z$; the decay of axions into two photons, $\mathrm{A}\ensuremath{\rightarrow}2\ensuremath{\gamma}$; and inverse Primakoff conversion on nuclei, $\mathrm{A}+Z\ensuremath{\rightarrow}\ensuremath{\gamma}+Z$, are considered. Model-independent limits on axion-electron (${g}_{Ae}$), axion-photon (${g}_{A\ensuremath{\gamma}}$), and isovector axion-nucleon (${g}_{3AN}$) couplings are obtained: $|{g}_{Ae}\ifmmode\times\else\texttimes\fi{}{g}_{3AN}|\ensuremath{\le}5.5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}13}$ and $|{g}_{A\ensuremath{\gamma}}\ifmmode\times\else\texttimes\fi{}{g}_{3AN}|\ensuremath{\le}4.6\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}11}\text{ }\text{ }{\mathrm{GeV}}^{\ensuremath{-}1}$ at ${m}_{A}l1\text{ }\text{ }\mathrm{MeV}$ (90% confidence level). These limits are 2--4 orders of magnitude stronger than those obtained in previous laboratory-based experiments using nuclear reactors and accelerators.
Published: 2012

44. Cosmic-muon flux and annual modulation in Borexino at 3800 m water-equivalent depth

Author: Jilei Xu, R. Tartaglia, K. Otis, D. Vignaud, G. Testera, C. Carraro, A. Sotnikov, Aldo Ianni, Caren Hagner, G. Zuzel, P. J. Mosteiro, T. Lewke, L. Oberauer, J. Benziger, V. N. Muratova, P. Cavalcante, A. Razeto, A. E. Chavarria, G. Manuzio, S. Manecki, W. Maneschg, L. Perasso, Gioacchino Ranucci, C. Ghiano, F. Lombardi, S. Davini, M. Misiaszek, Cristiano Galbiati, Y. Suvorov, A. Pocar, Michael Wurm, L. Grandi, B. Loer, M. Skorokhvatov, Yusuke Koshio, H. Simgen, Oleg Smirnov, D. Korablev, D. Kryn, C. Salvo, Matthias Laubenstein, G. Bonfini, M. Buizza Avanzini, E. Litvinovich, K. Fomenko, E. Guardincerri, F. von Feilitzsch, J. Winter, R. Saldanha, D. Montanari, R. S. Raghavan, Paolo Lombardi, B. Caccianiga, S. Gazzana, O. Zaimidoroga, A.V. Etenko, S. Hardy, S. V. Sukhotin, F. Calaprice, Laura Cadonati, Marco Giammarchi, D. Bravo, R. B. Vogelaar, Lino Miramonti, A. Wright, M. Goeger-Neff, E. Meroni, Alessandra Re, Fausto Ortica, I. Machulin, Stefan Schönert, D. Franco, G. Bellini, M. Obolensky, Livia Ludhova, A. A. Sabelnikov, A. M. Goretti, A. S. Chepurnov, Andrea Ianni, D. Bick, A. V. Derbin, Sandra Zavatarelli, M. M. Wojcik, S. Perasso, Q. Meindl, Aldo Romani, L. Papp, Marco Pallavicini, D. D'Angelo, G. Korga, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Borexino, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Bellini, G., Suvorov, Y., and Et, Al.
Subjects: Particle physics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], FOS: Physical sciences, Water equivalent, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Relative amplitude, Borexino, Physics, [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph], COSMIC cancer database, Muon, 010308 nuclear & particles physics, Astronomy and Astrophysics, Atmospheric temperature, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Physics - Atmospheric and Oceanic Physics, neutrino detector, 13. Climate action, Modulation, Atmospheric and Oceanic Physics (physics.ao-ph), Muon flux, neutrino experiment, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We have measured the muon flux at the underground Gran Sasso National Laboratory (3800 m w.e.) to be (3.41 \pm 0.01) \times 10-4m-2s-1 using four years of Borexino data. A modulation of this signal is observed with a period of (366\pm3) days and a relative amplitude of (1.29 \pm 0.07)%. The measured phase is (179 \pm 6) days, corresponding to a maximum on the 28th of June. Using the most complete atmospheric data models available, muon rate fluctuations are shown to be positively correlated with atmospheric temperature, with an effective coefficient {\alpha}T = 0.93 \pm 0.04. This result represents the most precise study of the muon flux modulation for this site and is in good agreement with expectations., Comment: 14 pages, 8 figures, published on JCAP as JCAP05(2012)015 on May 15th 2012
Published: 2012

45. Indication of Reactorν¯eDisappearance in the Double Chooz Experiment

Author: A. Cucoanes, F. Ardellier, M. Obolensky, M. Dracos, H. de Kerret, D. Shrestha, R. Svoboda, C. L. Jones, J. Maeda, I. Ostrovskiy, R. Santorelli, A. Tonazzo, C. Jollet, M. Franke, A. F. Barbosa, T. Hayakawa, J. Tm. Goon, I. Gil-Botella, Daniel M. Kaplan, G. Keefer, J.V. Dawson, R. Milincic, Tobias Lachenmaier, C. E. Lane, B. Guillon, J. Reichenbacher, J. Spitz, M. Worcester, N. Tamura, M. Dierckxsens, M. Cribier, J. Haser, G. Mention, H. Miyata, M. Kuze, K. Nakajima, C. Langbrandtner, J. Hartnell, Z. Sun, Christian Buck, H. P. Lima, M. Cerrada, C. Aberle, Yasushi Nagasaka, S. Cormon, Muriel Fallot, T. Classen, E. Kemp, J. Busenitz, Janet Conrad, E. Damon, S. Perasso, S. Roth, C. N. Maesano, C. Mariani, Th. A. Mueller, E. Caden, A. Onillon, W. Potzel, T. Kawasaki, D. Dietrich, Matthew L Strait, A. Hatzikoutelis, M. D. Skorokhvatov, Michael Wurm, H. Watanabe, A. Bernstein, Florian Kaether, Y. Kibe, J. Felde, Z. Djurcic, A. Osborn, A. Milzstajn, D. Franco, C. Palomares, K. Zbiri, D. E. Reyna, S. M. Fernandes, Yu. Efremenko, M. Bongrand, Ying Sun, Alain Letourneau, L. Bezrukhov, T.J.C. Bezerra, U. Schwan, Kazuhiro Terao, Yuri Kamyshkov, F. von Feilitzsch, Caren Hagner, R. Gama, Amanda Porta, H. H. Trinh Thi, T. Miletic, P. Perrin, A. Meregaglia, D. Kryn, J. Maricic, Christopher Wiebusch, J. M. LoSecco, David Lhuillier, Lothar Oberauer, Bayarto Lubsandorzhiev, B. White, P.-J. Chang, Masaki Ishitsuka, E. Falk, M. Elnimr, Thierry Lasserre, V. V. Sinev, M. Göger-Neff, H. Furuta, G. A. Horton-Smith, M. C. Goodman, F. Yermia, V. Durand, Lindley Winslow, Anatael Cabrera, F. X. Hartmann, E. Yanovitch, Y. Sakamoto, H. A. Rubin, Michael Hofmann, B. Reinhold, F. Sato, M. H. Shaevitz, Luis González, Nathaniel Bowden, Thomas Schwetz, E. Conover, H. Tabata, J. C. dos Anjos, V. Zimmer, L.N. Kalousis, M. Toups, I. M. Pepe, A. Baxter, A. Stüken, Steven Dazeley, R. Carr, D. Greiner, Yoshio Abe, L. Camilleri, Lydie Giot, M. V. d'Agostino, J. Martino, Sebastian Wagner, Manfred Lindner, Antoine Collin, E. Blucher, M. Röhling, S. Schönert, Y. Endo, P. Pfahler, M. Fechner, P. Chimenti, A.V. Etenko, T. Matsubara, J. M. López-Castanõ, I. Stancu, S. J. M. Peeters, T. Akiri, Stefan Schoppmann, D. Mckee, T. Haruna, Yehan Liu, T. Konno, A. Remoto, F. Suekane, P. Novella, T. Sumiyoshi, D. Motta, T. Hara, A. Stahl, J. L. Sida, R. Queval, M. Bergevin, J. Jochum, K. Crum, A. J. Franke, S. V. Sukhotin, J. I. Crespo-Anadón, E. Smith, N. Haag, S. Lucht, and C. Veyssiere
Subjects: NOνA, Physics, Particle physics, Muon, 010308 nuclear & particles physics, General Physics and Astronomy, Flux, Daya Bay Reactor Neutrino Experiment, CHOOZ, 7. Clean energy, 01 natural sciences, Nuclear physics, 0103 physical sciences, High Energy Physics::Experiment, Neutrino, Nuclear Experiment, 010306 general physics, Neutrino oscillation, Electron neutrino
Abstract: The Double Chooz experiment presents an indication of reactor electron antineutrino disappearance consistent with neutrino oscillations. An observed-to-predicted ratio of events of 0.944±0.016(stat)±0.040(syst) was obtained in 101 days of running at the Chooz nuclear power plant in France, with two 4.25GWth reactors. The results were obtained from a single 10m3 fiducial volume detector located 1050 m from the two reactor cores. The reactor antineutrino flux prediction used the Bugey4 flux measurement after correction for differences in core composition. The deficit can be interpreted as an indication of a nonzero value of the still unmeasured neutrino mixing parameter sin⁡22θ13. Analyzing both the rate of the prompt positrons and their energy spectrum, we find sin⁡22θ13=0.086±0.041(stat)±0.030(syst), or, at 90% C.L., 0.017
Published: 2012

46. Indication of reactor ν(e) disappearance in the Double Chooz experiment

Author: Y, Abe, C, Aberle, T, Akiri, J C, dos Anjos, F, Ardellier, A F, Barbosa, A, Baxter, M, Bergevin, A, Bernstein, T J C, Bezerra, L, Bezrukhov, E, Blucher, M, Bongrand, N S, Bowden, C, Buck, J, Busenitz, A, Cabrera, E, Caden, L, Camilleri, R, Carr, M, Cerrada, P-J, Chang, P, Chimenti, T, Classen, A P, Collin, E, Conover, J M, Conrad, S, Cormon, J I, Crespo-Anadón, M, Cribier, K, Crum, A, Cucoanes, M V, D'Agostino, E, Damon, J V, Dawson, S, Dazeley, M, Dierckxsens, D, Dietrich, Z, Djurcic, M, Dracos, V, Durand, Y, Efremenko, M, Elnimr, Y, Endo, A, Etenko, E, Falk, M, Fallot, M, Fechner, F, von Feilitzsch, J, Felde, S M, Fernandes, D, Franco, A J, Franke, M, Franke, H, Furuta, R, Gama, I, Gil-Botella, L, Giot, M, Göger-Neff, L F G, Gonzalez, M C, Goodman, J T M, Goon, D, Greiner, B, Guillon, N, Haag, C, Hagner, T, Hara, F X, Hartmann, J, Hartnell, T, Haruna, J, Haser, A, Hatzikoutelis, T, Hayakawa, M, Hofmann, G A, Horton-Smith, M, Ishitsuka, J, Jochum, C, Jollet, C L, Jones, F, Kaether, L, Kalousis, Y, Kamyshkov, D M, Kaplan, T, Kawasaki, G, Keefer, E, Kemp, H, de Kerret, Y, Kibe, T, Konno, D, Kryn, M, Kuze, T, Lachenmaier, C E, Lane, C, Langbrandtner, T, Lasserre, A, Letourneau, D, Lhuillier, H P, Lima, M, Lindner, Y, Liu, J M, López-Castanõ, J M, LoSecco, B K, Lubsandorzhiev, S, Lucht, D, McKee, J, Maeda, C N, Maesano, C, Mariani, J, Maricic, J, Martino, T, Matsubara, G, Mention, A, Meregaglia, T, Miletic, R, Milincic, A, Milzstajn, H, Miyata, D, Motta, Th A, Mueller, Y, Nagasaka, K, Nakajima, P, Novella, M, Obolensky, L, Oberauer, A, Onillon, A, Osborn, I, Ostrovskiy, C, Palomares, S J M, Peeters, I M, Pepe, S, Perasso, P, Perrin, P, Pfahler, A, Porta, W, Potzel, R, Queval, J, Reichenbacher, B, Reinhold, A, Remoto, D, Reyna, M, Röhling, S, Roth, H A, Rubin, Y, Sakamoto, R, Santorelli, F, Sato, S, Schönert, S, Schoppmann, U, Schwan, T, Schwetz, M H, Shaevitz, D, Shrestha, J-L, Sida, V, Sinev, M, Skorokhvatov, E, Smith, J, Spitz, A, Stahl, I, Stancu, M, Strait, A, Stüken, F, Suekane, S, Sukhotin, T, Sumiyoshi, Y, Sun, Z, Sun, R, Svoboda, H, Tabata, N, Tamura, K, Terao, A, Tonazzo, M, Toups, H H, Trinh Thi, C, Veyssiere, S, Wagner, H, Watanabe, B, White, C, Wiebusch, L, Winslow, M, Worcester, M, Wurm, E, Yanovitch, F, Yermia, K, Zbiri, and V, Zimmer
Abstract: The Double Chooz experiment presents an indication of reactor electron antineutrino disappearance consistent with neutrino oscillations. An observed-to-predicted ratio of events of 0.944±0.016(stat)±0.040(syst) was obtained in 101 days of running at the Chooz nuclear power plant in France, with two 4.25 GW(th) reactors. The results were obtained from a single 10 m(3) fiducial volume detector located 1050 m from the two reactor cores. The reactor antineutrino flux prediction used the Bugey4 flux measurement after correction for differences in core composition. The deficit can be interpreted as an indication of a nonzero value of the still unmeasured neutrino mixing parameter sin(2)2θ(13). Analyzing both the rate of the prompt positrons and their energy spectrum, we find sin(2)2θ(13)=0.086±0.041(stat)±0.030(syst), or, at 90% C.L., 0.017sin(2)2θ(13)0.16.
Published: 2012

47. High precision 7Be solar neutrinos measurement and day night effect obtained with Borexino

Author: Matthias Laubenstein, Cristiano Galbiati, B. Loer, Yusuke Koshio, G. Bellini, D. Montanari, M. D. Skorokhvatov, S. V. Sukhotin, O. Zaimidoroga, A. E. Chavarria, P. J. Mosteiro, F. Lombardi, L. Perasso, Michael Wurm, L. Grandi, A. Razeto, V. V. Kobychev, Michael K.H. Leung, Y. Suvorov, L. Miramonti, D. Vignaud, A.V. Etenko, T. Lewke, D. Kryn, R. Saldanha, Q. Meindl, M. Göger-Neff, M. Obolensky, S. Schönert, B. Caccianiga, R. B. Vogelaar, Jay Burton Benziger, A. V. Derbin, Marco Giammarchi, C. Carraro, S. Bonetti, D. Franco, E. Litvinovich, I. N. Machulin, R. Tartaglia, Andrea Ianni, D. Bick, Sandra Zavatarelli, C. Ghiano, Lothar Oberauer, Marco Pallavicini, D. D'Angelo, M. M. Wojcik, E. Guardincerri, Aldo Romani, C. Salvo, F. von Feilitzsch, Carlos Pena-Garay, S. Gazzana, A. Sotnikov, W. Maneschg, S. Hardy, M. Misiaszek, Laura Cadonati, S. Perasso, L. Papp, Gioacchino Ranucci, G. Bonfini, Frank Calaprice, Aldo Ianni, Livia Ludhova, Fausto Ortica, Hardy Simgen, G. Zuzel, A. M. Goretti, V. N. Muratova, E. Meroni, J. Winter, G. Korga, K. Fomenko, Denis Korablev, A. A. Sabelnikov, A. Pocar, G. Testera, O. Smirnov, R. S. Raghavan, G. Manuzio, S. Manecki, Paolo Lombardi, Testera, G., Bellini, G., Benziger, J., Bick, D., Bonetti, S., Bonfini, G., Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Chavarria, A., D'Angelo, D., Derbin, A., Etenko, A., Fomenko, K., Franco, D., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Grandi, L., Guardincerri, E., Hardy, S., Ianni, Aldo, Ianni, Andrea, Korablev, D., Kobychev, V., Korga, G., Koshio, Y., Kryn, D., Laubenstein, M., Leung, M., Lewke, T., Litvinovich, E., Loer, B., Lombardi, P., Lombardi, F., Ludhova, L., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Meindl, Q., Meroni, E., Miramonti, L., Misiaszek, M., Montanari, D., Mosteiro, P., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Pallavicini, M., Papp, L., Pena-Garay, C., Perasso, L., Perasso, S., Pocar, A., Raghavan, R. S., Ranucci, G., Razeto, A., Romani, A., Sabelnikov, A., Saldanha, R., Salvo, C., Schoenert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Vignaud, D., Vogelaar, R. B., von Feilitzsch, F., Winter, J., Wojcik, M., Wurm, M., Zaimidoroga, O., Zavatarelli, S., and Zuzel, G.
Subjects: Low background detector, Nuclear and High Energy Physics, Particle physics, Neutrino oscillation, Physics::Instrumentation and Detectors, CPT symmetry, media_common.quotation_subject, Solar neutrino, Physics beyond the Standard Model, low background detectors, liquid scintillators, Asymmetry, Nuclear physics, ENHANCEMENT, OSCILLATIONS, DETECTOR, Instrumentation, Borexino, media_common, Physics, Liquid, neutrino oscillations, scintillator, solar neutrinos, Measurements of neutrino speed, High Energy Physics::Experiment, Astrophysics::Earth and Planetary Astrophysics, Neutrino, MATTER
Abstract: We report the direct measurement of the 7 Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso and the search for a day–night asymmetry of this interaction rate. The interaction rate of the 0.862 MeV 7 Be neutrinos is 46 ± 1.6 ( stat ) − 1.6 + 1.5 ( syst ) counts/(day · 100 ton). The hypothesis of no oscillation for this solar neutrinos is inconsistent with our measurement at the 5.8 σ C.L. Our result is the first direct measurement of solar neutrinos with an accuracy better than 5%. We report the survival probability for solar ν e in the transition region between matter-enhanced and vacuum-driven oscillations. The measured day night asymmetry is A dn = 0.001 ± 0.012 (stat)±0.007 (syst), in agreement with the predicition of MSW–LMA neutrino [13] oscillations. This result discourages MSW oscillations with mixing parameters in the LOW region at more than 8.5 σ , meaning that this region is, for the first time, strongly rejected without the assumption of CPT symmetry. The result can also be used to constrain some neutrino oscillation scenarios involving new physics.
Published: 2012

48. Absence of a day-night asymmetry in the7Be solar neutrino rate in Borexino

Author: A. Etenkog, W. Maneschg, Cristiano Galbiati, Lothar Oberauer, R. Saldanha, G. Testera, Marco Giammarchi, Laura Cadonati, Andrea Ianni, D. Bick, Sandra Zavatarelli, L. Papp, Matthias Laubenstein, A. Sotnikov, D. Vignaud, M. D. Skorokhvatov, A. Pocar, Michael Wurm, L. Grandi, J. Winter, S. Hardy, D. Franco, M. Göger-Neff, T. Lewke, D. Kryn, B. Caccianiga, Livia Ludhova, R. B. Vogelaar, A. M. Goretti, Fausto Ortica, S. Davinic, Q. Meindl, Y. Suvorov, C. Carraro, A. Derbinm, E. Meroni, Stefano Bonetti, Denis Korablev, Marcin Wójcik, E. Litvinovich, S. Gazzana, F. Lombardi, S. Schoenert, C. Salvo, Jilei Xu, O. Smirnov, Alessandra Re, A. Razeto, F. von Feilitzsch, G. Bellini, I. N. Machulin, Marco Pallavicini, S. Manecki, Jay Burton Benziger, Aldo Ianni, D. D'Angelo, Aldo Romani, A. E. Chavarria, L. Perasso, G. Zuzel, Carlos Pena-Garay, R. S. Raghavan, Lino Miramonti, S. Perasso, G. Manuzio, B. Loer, Yusuke Koshio, G. Korga, K. Fomenko, G. Bonfini, M. Buizza Avanzini, Frank Calaprice, Hardy Simgen, P. J. Mosteiro, C. Ghiano, P. Cavalcante, M. Misiaszek, V. N. Muratova, D. Montanari, Gioacchino Ranucci, E. Guardincerri, A. A. Sabelnikov, M. Obolensky, Paolo Lombardi, S. V. Sukhotin, A. Wright, O. Zaimidoroga, V. V. Kobychev, R. Tartaglia, Bellini, G., Suvorov, Y., and Et, Al.
Subjects: Particle physics, Nuclear and High Energy Physics, Neutrino oscillation, Physics::Instrumentation and Detectors, media_common.quotation_subject, Solar neutrino, 01 natural sciences, Asymmetry, Nuclear physics, Day-night effect, 0103 physical sciences, 010306 general physics, Nuclear Experiment, day–night effect, Borexino, media_common, Physics, neutrino oscillations, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Física, Solar neutrino problem, Neutrino detector, solar neutrinos, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, CPT violation
Abstract: We report on a search for the day-night asymmetry of the Be-7 solar neutrino rate measured by Borexino at the Laboratori Nazionali del Gran Sasso (LNGS), Italy. The measured value, Adn=0.001 +- 0.012 (stat) +- 0.007 (syst), shows the absence of a significant asymmetry. This result alone rejects the so-called LOW solution at more than 8.5 sigma. Combined with the other solar neutrino data, it isolates the Large Mixing Angle (LMA) -- MSW solution at DeltaChi2 > 190 without relying on the assumption of CPT symmetry in the neutrino sector. We also show that including the day-night asymmetry, data from Borexino alone restricts the MSW neutrino oscillations to the LMA solution at 90% confidence level.
Published: 2012

49. First evidence of pep solar neutrinos by direct detection in Borexino

Author: A.V. Etenko, A. Pocar, D. Bravo, R. Tartaglia, Livia Ludhova, Denis Korablev, A. S. Chepurnov, A. Razeto, S. Davini, S. Schönert, Marcin Wójcik, G. Manuzio, B. Loer, R. S. Raghavan, C. Ghiano, G. Zuzel, R. B. Vogelaar, M. Obolensky, R. Saldanha, Yusuke Koshio, M. Goeger-Neff, K. Otis, Y. Suvorov, D. Montanari, Alessandra Re, L. Oberauer, A. A. Sabelnikov, P. Cavalcante, A. Derbin, M. Misiaszek, A. E. Chavarria, L. Perasso, Aldo Ianni, Marco Giammarchi, A. Sotnikov, E. Litvinovich, E. Meroni, F. Lombardi, V. Muratova, B. Caccianiga, P. J. Mosteiro, J. Benziger, Andrea Ianni, F. Calaprice, D. Bick, Sandra Zavatarelli, C. Salvo, O. Zaimidoroga, A. Goretti, E. Guardincerri, O. Smirnov, G. Testera, S. Manecki, Aldo Romani, L. Papp, Paolo Lombardi, J. Winter, S. Perasso, S. V. Sukhotin, Gioacchino Ranucci, A. Wright, Jingke Xu, Cristiano Galbiati, G. Bellini, S. Hardy, M. Skorokhvatov, Matthias Laubenstein, J. Quirk, T. Lewke, D. Kryn, Marco Pallavicini, D. D'Angelo, Stefano Bonetti, K. Fomenko, S. Gazzana, Michael Wurm, L. Grandi, Q. Meindl, F. von Feilitzsch, W. Maneschg, Laura Cadonati, Fausto Ortica, I. Machulin, Lino Miramonti, D. Vignaud, G. Korga, D. Franco, G. Bonfini, M. Buizza Avanzini, Hardy Simgen, C. Carraro, Bellini, G., Suvorov, Y., Et, Al., APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), AstroParticule et Cosmologie (APC (UMR_7164)), Borexino, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: History, Metallicity, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrinos, General Physics and Astronomy, FOS: Physical sciences, Astrophysics, 01 natural sciences, Main-sequence: late-type stars, Education, High Energy Physics - Experiment, 26.65.+t, 14.60.Lm, 95.55.Vj, 97.20.Jg, Nuclear physics, Physics and Astronomy (all), High Energy Physics - Experiment (hep-ex), Ordinary neutrinos (nuW bosons, muon, 0103 physical sciences, Neutrino, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Astrophysics::Solar and Stellar Astrophysics, 010306 general physics, Neutrino oscillation, Borexino, Solar and Stellar Astrophysics (astro-ph.SR), Physics, Range (particle radiation), Standard solar model, Muon, 010308 nuclear & particles physics, [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], High Energy Physics::Phenomenology, pion, cosmic ray detectors, [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], and other elementary particle detectors, Computer Science Applications, 3. Good health, Astrophysics - Solar and Stellar Astrophysics, 13. Climate action, Physics::Space Physics, High Energy Physics::Experiment
Abstract: We observed, for the first time, solar neutrinos in the 1.0-1.5 MeV energy range. We measured the rate of pep solar neutrino interactions in Borexino to be [3.1+-0.6(stat)+-0.3(syst)] counts/(day x 100 ton) and provided a constraint on the CNO solar neutrino interaction rate of, Submitted to Physical Review Letters (2011)
Published: 2011
Full Text: View/download PDF

50. Borexino: recent results, detector calibration and future perspectives

Author: Marco Pallavicini, G. Bellini, J. Benziger, S. Bonetti, M. Buizza Avanzini, B. Caccianiga, L. Cadonati, F. Calaprice, C. Carraro, A. Chavarria, F. Dalnoki-Veress, D. DʼAngelo, S. Davini, H. de Kerret, A. Derbin, A. Etenko, F. von Feilitzsch, K. Fomenko, D. Franco, C. Galbiati, S. Gazzana, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, E. Guardincerri, S. Hardy, Aldo Ianni, Andrea Ianni, M. Joyce, V. Kobychev, Y. Koshio, G. Korga, D. Kryn, M. Laubenstein, M. Leung, T. Lewke, E. Litvinovich, B. Loer, F. Lombardi, P. Lombardi, L. Ludhova, I. Machulin, S. Manecki, W. Maneschg, G. Manuzio, Q. Meindl, E. Meroni, L. Miramonti, M. Misiaszek, D. Montanari, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, M. Pallavicini, L. Papp, L. Perasso, S. Perasso, A. Pocar, R.S. Raghavan, G. Ranucci, A. Razeto, A. Re, P. Risso, A. Romani, D. Rountree, A. Sabelnikov, R. Saldanha, C. Salvo, S. Schönert, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, R.B. Vogelaar, J. Winter, M. Wojcik, M. Wurm, A. Wright, J. Xu, O. Zaimidoroga, S. Zavatarelli, and G. Zuzel
Subjects: Physics, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, Detector, Scintillator, Solar neutrino problem, Atomic and Molecular Physics, and Optics, Physics::Geophysics, Nuclear physics, Neutrino detector, Calibration, High Energy Physics::Experiment, Neutrino, Nuclear Experiment, Borexino
Abstract: The Borexino experiment has been running since May 2007 at the Gran Sasso underground laboratory, in Italy. Solar neutrinos are detected with a large unsegmented liquid scintillator detector with unprecedented radioactive purity. The main results obtained include the measurement of the 7Be solar neutrino flux, the measurement of the 8B neutrino flux with electron recoil energy threshold of 3.0 MeV and the first clear detection of geo-neutrinos (see Aldo Ianniʼs talk in these proceedings for further details). Borexino has recently completed a large calibration campaign, and better results on 7Be solar neutrino measurement are expected soon. Short and medium term perspectives are summarized in the conclusions.
Published: 2011

Catalog

Books, media, physical & digital resources

See catalog results

Searchworks

Select search scope, currently: Articles Catalog books, media & more in Jio Institute collections Articles journal articles & other e-resources

Search

Search Constraints

Refine your results

Search Limiters

Topic

Publication Year Range

Language

Publication Type

Journal

Database

Publisher

64 results on '"S. Perasso"'

Search Results

Catalog

Select search scope, currently: Articles

Catalog

books, media & more in Jio Institute collections

Articles

journal articles & other e-resources