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

Your search keyword '"S. Perasso"' showing total 45 results

Start Over Author "S. Perasso" Language english

45 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. 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

5. 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

6. 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

7. 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

8. 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

9. 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

10. 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

11. 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

12. 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

13. 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

14. 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

15. 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

16. 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

17. 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

18. 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

19. 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

20. 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

21. 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

22. 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

23. 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

24. 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

25. 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

26. 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

27. 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

28. 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

29. 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

30. 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

31. 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

32. 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

33. 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

34. 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

35. 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

36. 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

37. Neutrino interactions at few MeV: results from Borexino at Gran Sasso

Author: Laura Perasso, G. Bellini, S. Bonetti, M. Buizza Avanzini, B. Caccianiga, D. DʼAngelo, D. Franco, M. Giammarchi, Y. Koshio, P. Lombardi, L. Ludhova, E. Meroni, L. Miramonti, G. Ranucci, A. Re, J. Benziger, L. Cadonati, A. Pocar, F. Calaprice, A. Chavarria, F. Dalnoki-Veress, C. Galbiati, A. Goretti, Andrea Ianni, M. Leung, B. Loer, K. McCarty, R. Saldanha, A. Wright, C. Carraro, S. Davini, E. Guardincerri, G. Manuzio, M. Pallavicini, S. Perasso, P. Risso, C. Salvo, G. Testera, S. Zavatarelli, H. de Kerret, D. Kryn, M. Obolensky, D. Vignaud, A. Derbin, V. Muratova, A. Etenko, E. Litvinovich, I. Machulin, A. Sabelnikov, M. Skorokhvatov, S. Sukhotin, K. Fomenko, O. Smirnov, A. Sotnikov, O. Zaimidoroga, S. Gazzana, C. Ghiano, Aldo Ianni, G. Korga, M. Laubenstein, L. Papp, A. Razeto, R. Tartaglia, M. Goeger-Neff, T. Lewke, Q. Meindl, L. Oberauer, F. von Feilitzsch, J. Winter, M. Wurm, C. Grieb, S. Hardy, M. Joyce, S. Manecki, R.S. Raghavan, D. Rountree, R.B. Vogelaar, V.V. Kobychev, W. Maneschg, S. Schoenert, H. Simgen, G. Zuzel, F. Masetti, F. Ortica, A. Romani, G. Fiorentini, B. Ricci, M. Misiaszek, D. Montanari, Y. Suvorov, M. Wojcik, Bellini, G., Bonetti, S., Avanzini, M. Buizza, Caccianiga, B., D'Angelo, D., Franco, D., Giammarchi, M., Koshio, Y., Lombardi, P., Ludhova, L., Meroni, E., Miramonti, L., Ranucci, G., Re, A., Benziger, J., Cadonati, L., Pocar, A., Calaprice, F., Chavarria, A., Dalnoki-Veress, F., Galbiati, C., Goretti, A., Ianni, Andrea, Leung, M., Loer, B., Mccarty, K., Saldanha, R., Wright, A., Carraro, C., Davini, S., Guardincerri, E., Manuzio, G., Pallavicini, M., Perasso, S., Risso, P., Salvo, C., Testera, G., Zavatarelli, S., de Kerret, H., Kryn, D., Obolensky, M., Vignaud, D., Derbin, A., Muratova, V., Eteriko, A., Litvinovich, E., Machulin, I., Sabelnikov, A., Skorokhvatov, M., Sukhotin, S., Fomenko, K., Smirnov, O., Sotnikov, A., Zaimidoroga, O., Gazzana, S., Chian, C., Ianni, Aldo, Korga, G., Laubenstein, M., Papp, L., Razeto, A., Tartaglia, R., Goeger-Neff, M., Lewke, T., Meindl, Q., Oberauer, L., von Feilitzsch, F., Winter, J., Wurm, M., Grieb, C., Hardy, S., Joyce, M., Manecki, S., Raghavan, R. S., Rountree, D., Vogelaar, R. B., Kobychev, V. V., Maneschg, W., Schoenert, S., Simgen, H., Zuzel, G., Masetti, F., Ortica, F., Romani, A., Fiorentini, G., Ricci, B., Misiaszek, M., Montanan, D., Suvorov, Y., and Wojcik, M.
Subjects: ICARUS, Physics, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::Instrumentation and Methods for Astrophysics, Atomic and Molecular Physics, and Optics, NO, Physics::Geophysics, Massless particle, Nuclear physics, Low energy, SOLAR NEUTRINOS, Underground laboratory, High Energy Physics::Experiment, Neutrino, Nuclear Experiment, DETECTOR, Borexino, Lepton
Abstract: Borexino, at the I.N.F.N. Gran Sasso Underground Laboratory in Italy, is an experiment designed to detect, in real-time, low energy solar neutrinos. After a brief presentation of the Borexino physics and detector, we illustrate some recent results and their physics implications. Borexino perspectives are also discussed.
Published: 2011

38. Production and suppression of C-11 in the solar neutrino experiment Borexino

Author: Matthias Laubenstein, E. Litvinovich, Laura Cadonati, D. Rountree, C. Salvo, S. Hardy, L. Papp, W. Maneschg, R. S. Raghavan, C. Galbiati, Livia Ludhova, R. B. Vogelaar, A. S. Chepurnov, A.V. Etenko, M. Goeger-Neff, A. M. Goretti, G. Manuzio, E. Meroni, M. D. Skorokhvatov, Michael Wurm, S. Gazzana, A. Pocar, D. Vignaud, Fausto Ortica, S. Bonetti, Gioacchino Ranucci, D. Kryn, M. M. Wojcik, S. Schönert, D. Franco, Aldo Ianni, Lothar Oberauer, Q. Meindl, Aldo Romani, Quirin Meindl, Michael K.H. Leung, T. Lewke, A. E. Chavarria, Marco Pallavicini, L. Perasso, F. Dalnoki-Veress, Jingke Xu, S. Davini, Ben Loer, Jay Burton Benziger, A. Sotnikov, V. N. Muratova, O. Smirnov, B. Caccianiga, J. Winter, D. Montanari, A. Razeto, G. Testera, Alessandra Re, Andrea Ianni, G. Zuzel, Sandra Zavatarelli, P. Risso, A. A. Sabelnikov, Y. Suvorov, I. N. Machulin, D. D'Angelo, G. Bellini, S. Perasso, G. Korga, K. Fomenko, S. Manecki, Frank Calaprice, Hardy Simgen, C. Carraro, F. von Feilitzsch, Malcolm J. Joyce, C. Ghiano, M. Misiaszek, R. Saldanha, Marco Giammarchi, Lino Miramonti, M. Buizza Avanzini, A. V. Derbin, E. Guardincerri, Paolo Lombardi, M. Obolensky, H. de Kerret, S. V. Sukhotin, A. Wright, O. Zaimidoroga, V. V. Kobychev, R. Tartaglia, Meindl, Quinn, Bellini, G., Benziger, J., Bonetti, S., Avanzini, M. Buizza, Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Chavarria, A., Chepurnov, A., Dalnoki-Veress, F., D'Angelo, D., Davini, S., de Kerret, H., Derbin, A., Etenko, A., von Feilitzsch, F., Fomenko, K., Franco, D., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Guardincerri, E., Hardy, S., Ianni, Aldo, Ianni, Andrea, Joyce, M., Kobychev, V., Korga, G., Kryn, D., Laubenstein, M., Leung, M., Lewke, T., Litvinovich, E., Loer, B., Lombardi, P., Ludhova, L., Machulin, I., Manecki, S., Maneschg, W., Manuzio, G., Meindl, Q., Meroni, E., Miramonti, L., Misiaszek, M., Montanari, D., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Pallavicini, M., Papp, L., Perasso, L., Perasso, S., Pocar, A., Raghavan, R. S., Ranucci, G., Razeto, A., Re, A., Risso, P., Romani, A., Rountree, D., 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., Winter, J., Wojcik, M., Wright, A., Wurm, M., Xu, J., Zaimidoroga, O., Zavatarelli, S., and Zuzel, G.
Subjects: Physics, Particle physics, Muon, Solar energetic particles, Physics::Instrumentation and Detectors, Solar neutrino, Cosmic ray, Nuclear physics, Astrophysics::Solar and Stellar Astrophysics, High Energy Physics::Experiment, Neutron, Neutrino, Borexino, Lepton
Abstract: Cosmogenic C-11 is produced in-situ by atmospheric mons and forms the main background for the measurement of solar pep- and CNO-neutrinos. However, FLUKA simulations show that the majority of C-11 is accompanied by a free neutron in the final state, thus allowing for an efficient tagging method, the so-called Three-Fold Coincidence technique. The technique and its first applications on Borexino data are presented.
Published: 2011

39. Observation of Geo-Neutrinos

Author: W. Maneschg, F. Dalnoki-Veress, G. Zuzel, P. Risso, R. Tartaglia, Matthias Laubenstein, A. A. Sabelnikov, A. Razeto, M. Skorokhvatov, G. Bellini, R. Saldanha, Michael Wurm, C. Salvo, Jilei Xu, Aldo Romani, L. Papp, A. Goretti, M. Goeger-Neff, Marco Giammarchi, S. Davini, Malcolm J. Joyce, S. Gazzana, S. Perasso, J. Winter, D. Franco, C. Ghiano, R. B. Vogelaar, Q. Meindl, Barbara Ricci, E. Litvinovich, M. Misiaszek, G. Manuzio, Gioacchino Ranucci, A. Sotnikov, O. Zaimidoroga, Alessandra Re, B. Caccianiga, F. Calaprice, E. Guardincerri, T. Lewke, D. Kryn, Cristiano Galbiati, G. Testera, O. Smirnov, Livia Ludhova, A.V. Etenko, D. Vignaud, Giovanni Fiorentini, D. Montanari, D. Rountree, Stefano Bonetti, A. Pocar, B. Loer, Yusuke Koshio, R. S. Raghavan, Aldo Ianni, Marcin Wójcik, Y. Suvorov, L. Oberauer, A. E. Chavarria, L. Perasso, S. Schönert, S. Hardy, Lino Miramonti, Andrea Ianni, Sandra Zavatarelli, S. Manecki, Michael K.H. Leung, V. Muratova, K. Fomenko, Marco Pallavicini, D. D'Angelo, A. Derbin, E. Meroni, J. Benziger, Laura Cadonati, G. Korga, Fausto Ortica, I. Machulin, F. von Feilitzsch, M. Buizza Avanzini, Hardy Simgen, C. Carraro, S. V. Sukhotin, A. Wright, V. V. Kobychev, Paolo Lombardi, M. Obolensky, H. de Kerret, 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), Borexino, 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), 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), Bellini, G., Suvorov, Y., and Et, Al.
Subjects: Nuclear and High Energy Physics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Anti-neutrinos from reactors, Geoneutrino, Physics::Instrumentation and Detectors, Solar neutrino, FOS: Physical sciences, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Anti-neutrinos from reactors, Geo-neutrino, Neutrino detector, 01 natural sciences, 7. Clean energy, NO, Physics::Geophysics, High Energy Physics - Experiment, Neutrino detector, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, 010306 general physics, Nuclear Experiment, Borexino, Physics, Anti-neutrinos from reactor, 010308 nuclear & particles physics, Astronomy, Solar neutrino problem, humanities, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Cosmic neutrino background, Geo-neutrino, 13. Climate action, Measurements of neutrino speed, High Energy Physics::Experiment, Astrophysics::Earth and Planetary Astrophysics, Neutrino, Neutrino astronomy
Abstract: Geo-neutrinos, electron anti-neutrinos produced in beta decays of naturally occurring radioactive isotopes in the Earth, are a unique direct probe of our planet's interior. We report the first observation at more than 3$\sigma$ C.L. of geo-neutrinos, performed with the Borexino detector at Laboratori Nazionali del Gran Sasso. Anti-neutrinos are detected through the neutron inverse beta decay reaction. With a 252.6 ton-yr fiducial exposure after all selection cuts, we detected 9.9^{+4.1}_{-3.4}(^{+14.6}_{-8.2}) geo-neutrino events, with errors corresponding to a 68.3%(99.73%) C.L. From the $\ln{\cal{L}}$ profile, the statistical significance of the Borexino geo-neutrino observation corresponds to a 99.997% C.L. Our measurement of the geo-neutrinos rate is 3.9^{+1.6}_{-1.3}(^{+5.8}_{-3.2}) events/(100ton-yr). This measurement rejects the hypothesis of an active geo-reactor in the Earth's core with a power above 3 TW at 95% C.L. The observed prompt positron spectrum above 2.6 MeV is compatible with that expected from european nuclear reactors (mean base line of approximately 1000 km). Our measurement of reactor anti-neutrinos excludes the non-oscillation hypothesis at 99.60% C.L., Comment: 8 pages, 4 figures, 3 tables
Published: 2010

40. The liquid handling systems for the Borexino solar neutrino detector

Author: A. de Bellefon, R. von Hentig, S. Kidner, S. Parmeggiano, J. Maneira, A. Nelson, Danilo Giugni, W. Hampel, R. Eisenstein, G. Cecchet, A. Bevilacqua, Gunther Korschinek, T. A. Shutt, R. Fernholz, Mikael Hult, Elisa Resconi, An. Ianni, S. Gazzana, C. Arpesella, S. Hardy, R. Tartaglia, M. Parodi, Cristiano Galbiati, F. Soricelli, P. Risso, S. Vitale, A. E. Chavarria, K. McCarty, Nicomede Pelliccia, R. Cereseto, L. Perasso, E. Harding, C. Sule, Y. Suvorov, K. Jaenner, P. Saggese, Aldo Ianni, T. Lewke, A. Sotnikov, D. Kryn, Bryant Williams, C. Salvo, W. Maneschg, T. Goldbrunner, K. H. Schubeck, V. Vyrodov, Stefano Nisi, M. Goeger-Neff, M. Balata, G. Testera, Paolo Lombardi, F. Loeser, Margherita Buizza Avanzini, Laura Cadonati, L. Papp, M. Obolensky, Jay Burton Benziger, H. de Kerret, Y. Kozlov, A. M. Goretti, A.V. Etenko, C. Grieb, G. Heusser, M. Marchelli, G. Di Pietro, Lino Miramonti, Stefano Bonetti, D. Franco, M. D. Skorokhvatov, D. Bartolomei, A. Razeto, D. Manuzio, I. N. Machulin, D. Bondi, E. de Haas, A. Golubchikov, Fausto Ortica, Michael Wurm, R. Wordel, E. Litvinovich, M. Chen, V. G. Tarasenkov, R. Saldanha, Fausto Masetti, F. Siccardi, F. Dalnoki-Veress, Gioacchino Ranucci, Lothar Oberauer, R. Parsells, S. V. Sukhotin, Matthias Laubenstein, Marco Pallavicini, D. D'Angelo, O. Zaimidoroga, R. J. Ford, Frank Calaprice, T. Hagner, Marco Giammarchi, Martin Deutsch, S. Davini, F. Hartmann, Hardy Simgen, V. M. Gehman, V. V. Kobychev, Livia Ludhova, F. von Feilitzsch, Malcolm J. Joyce, Till Kirsten, A. S. Chepurnov, H.O. Back, C. Carraro, G. Bellini, Sandra Malvezzi, T. Hertrich, M. Orsini, E. Meroni, B. Loer, C. Hagner, D. Rountree, W. Czech, Gianluca Alimonti, Flavio Gatti, N. Gaertner, Ugo Mazzucato, L. Ioannucci, A. V. Derbin, Daniel McKinsey, A. Manco, A. Marternianov, Augusto Brigatti, R. B. Vogelaar, H. Neder, S. Schönert, W. Rau, Q. Meindl, L. Niedermeier, I. Manno, D. Vignaud, C. Lendvai, E. Guardincerri, G. Zuzel, Sandra Zavatarelli, G. Korga, K. Fomenko, Michael K.H. Leung, B. Freudiger, A. Di Credico, M. Misiaszek, P.H. La Marche, R. Scardaoni, B. Caccianiga, D. Schimizzi, D. Montanari, A. de Bari, A. A. Sabelnikov, V. N. Muratova, Fausto Elisei, S. Perasso, V. Lagomarsino, Aldo Romani, Paolo Musico, Marcin Wójcik, A. Cubaiu, J. Kiko, M. E. Monzani, A. Pocar, O. Smirnov, Andrew Sonnenschein, A. Di Ludovico, R. S. Raghavan, G. Manuzio, 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, 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), 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), 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 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, Alimonti, G., Suvorov, Y., and Et, Al.
Subjects: Nuclear and High Energy Physics, Low background detector, Liquid scintillator, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Physics::Instrumentation and Detectors, Solar neutrino, Nuclear engineering, Radiopurity, Scintillator, 01 natural sciences, Nuclear physics, Physics::Fluid Dynamics, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, Borexino, Nuclear and High Energy Physic, Physics, 010308 nuclear & particles physics, Modular system, Detector, Volumetric flow rate, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Flow control (fluid), Neutrino detector, High Energy Physics::Experiment
Abstract: The successful deployment of the Borexino solar neutrino detector required assorted physical and chemical operations to produce exceptional pure fluids and fill multiple detector zones. The composition and flow rates of high purity gases and liquids had to be precisely controlled to maintain liquid levels and pressures. The system was required to meet exceptional requirements for cleanliness and leak-tightness. A large scale modular system connecting fluid receiving, purification and fluid delivery processes was developed for Borexino. At the core is a flow control system that delivers scintillator components to plants for purification, and then fills the Borexino detector volumes with ultrahigh purity buffer or ultrahigh purity scintillator. The liquid handling system maintains precise control over the liquid levels and differential pressures between the different volumes of the detectors that are separated by flexible nylon vessels. The preparation, commissioning and operation of the system for filling the Borexino detector with scintillator is described.
Published: 2009

41. Measurement of the solar 8B neutrino flux down to 2.8 MeV with Borexino

Author: Andrea Ianni, Sandra Zavatarelli, O. Smirnov, M. D. Skorokhvatov, Michael Wurm, Aldo Ianni, K. McCarty, Marco Pallavicini, Paolo Lombardi, Frank Calaprice, Q. Meindl, A. V. Derbin, A. Sotnikov, P. Risso, M. Obolensky, H. de Kerret, Malcolm J. Joyce, F. von Feilitzsch, R. Tartaglia, Hardy Simgen, C. Carraro, F. Dalnoki-Veress, C. Galbiati, D. Vignaud, V. N. Muratova, Livia Ludhova, C. Salvo, Y. Suvorov, S. Bonetti, W. Maneschg, M. Misiaszek, S. Gazzana, R. Saldanha, S. Perasso, S. Hardy, T. Lewke, Ben Loer, A. A. Sabelnikov, Marco Giammarchi, S. V. Sukhotin, G. Korga, C. Grieb, K. Fomenko, Lothar Oberauer, D. Rountree, Laura Cadonati, L. Papp, O. Zaimidoroga, Gioacchino Ranucci, A. M. Goretti, R. B. Vogelaar, E. Litvinovich, A.V. Etenko, Matthias Laubenstein, S. Schönert, Fausto Ortica, A. Razeto, G. Bellini, V. V. Kobychev, A. Pocar, G. Zuzel, M. M. Wojcik, Aldo Romani, E. Meroni, D. Montanari, Jay Burton Benziger, G. Testera, I. N. Machulin, D. D'Angelo, D. Kryn, Fausto Masetti, Michael K.H. Leung, A. E. Chavarria, L. Perasso, S. Manecki, B. Caccianiga, R. S. Raghavan, G. Manuzio, Lino Miramonti, M. Buizza Avanzini, M. Goeger-Neff, and D. Franco
Subjects: Physics, Elastic scattering, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Solar neutrino, Solar neutrino problem, Atomic and Molecular Physics, and Optics, Nuclear physics, Neutrino detector, High Energy Physics::Experiment, Neutrino, Nuclear Experiment, Electron neutrino, Borexino, Lepton
Abstract: We report the measurement of the 8B solar neutrinos interaction rate with the Borexino detector. The extremly high radio-purity reached in the Borexino scintillator, combined with the efficient software rejection of cosmogenic background, allows to investigate the recoiled electron spectrum, induced by 8B solar neutrinos, down to the unprecedented energy threshold of 2.8 MeV. The rate of 8B solar neutrino interaction as measured through their scattering on the target electrons is 0.26 ± 0.04 stat ± 0.02 syst c/d/100 tons. This corresponds to an equivalent electron neutrino flux of ( 2.65 ± 0.44 stat ± 0.18 syst ) × 10 6 cm − 2 s − 1 , as derived from the elastic scattering only, in good agreement with existing measurements and predictions.
Published: 2009

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

Author: Miramonti L, Bellini G, Benziger J, Bick D, Bonfini G, Bravo D, Buizza Avanzini M, Caccianiga B, Cadonati L, Calaprice F, Carraro C, Cavalcante P, Chavarria A, Chubakov V, D'Angelo D, Davini S, Derbin A, Etenko A, Fomenko K, Franco D, Galbiati C, Gazzana S, Ghiano C, Giammarchi M, Göger-Neff M, Goretti A, Grandi L, Guardincerri E, Hardy S, Ianni A, Ianni A, Kobychev V, Korablev D, Korga G, Koshio Y, Kryn D, Laubenstein M, Lewke T, Lissia M, Litvinovich E, Loer B, Lombardi F, Lombardi P, Ludhova L, Machulin I, Manecki S, Maneschg W, Mantovani F, Manuzio G, Meindl Q, Meroni E, Misiaszek M, Montanari D, Mosteiro P, Muratova V, Nisi S, Oberauer L, Obolensky M, Ortica F, Otis K, Pallavicini M, Papp L, Perasso L, Perasso S, Pocar A, Ranucci G, Razeto A, Re A, Romani A, Rossi N, Sabelnikov A, Saldanha R, Salvo C, Schönert S, Simgen H, Skorokhvatov M, Smirnov O, Sotnikov A, Sukhotin S, Suvorov Y, Tartaglia R, Testera G, Vignaud D, Vogelaar RB, von Feilitzsch F, Winter J, Wojcik M, Wright A, Wurm M, Xhixha G, Xu J, Zaimidoroga O, Zavatarelli S, and Zuzel G
Subjects: Alpha Particles, Half-Life, Laboratories, Radiation Monitoring, Lead Radioisotopes analysis, Polonium analysis, Radioactive Pollutants analysis
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., (Copyright © 2014 Elsevier Ltd. All rights reserved.)
Published: 2014
Full Text: View/download PDF

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

Author: Abe Y, Aberle C, Akiri T, dos Anjos JC, Ardellier F, Barbosa AF, Baxter A, Bergevin M, Bernstein A, Bezerra TJ, Bezrukhov L, Blucher E, Bongrand M, Bowden NS, Buck C, Busenitz J, Cabrera A, Caden E, Camilleri L, Carr R, Cerrada M, Chang PJ, Chimenti P, Classen T, Collin AP, Conover E, Conrad JM, Cormon S, Crespo-Anadón JI, Cribier M, Crum K, Cucoanes A, D'Agostino MV, Damon E, Dawson JV, Dazeley S, Dierckxsens M, Dietrich D, Djurcic Z, Dracos M, Durand V, Efremenko Y, Elnimr M, Endo Y, Etenko A, Falk E, Fallot M, Fechner M, von Feilitzsch F, Felde J, Fernandes SM, Franco D, Franke AJ, Franke M, Furuta H, Gama R, Gil-Botella I, Giot L, Göger-Neff M, Gonzalez LF, Goodman MC, Goon JT, Greiner D, Guillon B, Haag N, Hagner C, Hara T, Hartmann FX, Hartnell J, Haruna T, Haser J, Hatzikoutelis A, Hayakawa T, Hofmann M, Horton-Smith GA, Ishitsuka M, Jochum J, Jollet C, Jones CL, Kaether F, Kalousis L, Kamyshkov Y, Kaplan DM, Kawasaki T, Keefer G, Kemp E, de Kerret H, Kibe Y, Konno T, Kryn D, Kuze M, Lachenmaier T, Lane CE, Langbrandtner C, Lasserre T, Letourneau A, Lhuillier D, Lima HP Jr, Lindner M, Liu Y, López-Castanõ JM, LoSecco JM, Lubsandorzhiev BK, Lucht S, McKee D, Maeda J, Maesano CN, Mariani C, Maricic J, Martino J, Matsubara T, Mention G, Meregaglia A, Miletic T, Milincic R, Milzstajn A, Miyata H, Motta D, Mueller TA, Nagasaka Y, Nakajima K, Novella P, Obolensky M, Oberauer L, Onillon A, Osborn A, Ostrovskiy I, Palomares C, Peeters SJ, Pepe IM, Perasso S, Perrin P, Pfahler P, Porta A, Potzel W, Queval R, Reichenbacher J, Reinhold B, Remoto A, Reyna D, Röhling M, Roth S, Rubin HA, Sakamoto Y, Santorelli R, Sato F, Schönert S, Schoppmann S, Schwan U, Schwetz T, Shaevitz MH, Shrestha D, Sida JL, Sinev V, Skorokhvatov M, Smith E, Spitz J, Stahl A, Stancu I, Strait M, Stüken A, Suekane F, Sukhotin S, Sumiyoshi T, Sun Y, Sun Z, Svoboda R, Tabata H, Tamura N, Terao K, Tonazzo A, Toups M, Trinh Thi HH, Veyssiere C, Wagner S, Watanabe H, White B, Wiebusch C, Winslow L, Worcester M, Wurm M, Yanovitch E, Yermia F, Zbiri K, and Zimmer V
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., 0.017
Published: 2012
Full Text: View/download PDF

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

Author: Bellini G, Benziger J, Bick D, Bonetti S, Bonfini G, Bravo D, Buizza Avanzini M, Caccianiga B, Cadonati L, Calaprice F, Carraro C, Cavalcante P, Chavarria A, Chepurnov A, D'Angelo D, Davini S, 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 A, Ianni A, Korablev D, Korga G, Koshio Y, Kryn D, Laubenstein M, Lewke T, Litvinovich E, Loer B, Lombardi F, Lombardi P, 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, Otis K, Pallavicini M, Papp L, Perasso L, Perasso S, Pocar A, Quirk J, Raghavan RS, Ranucci G, Razeto A, Re A, Romani A, Sabelnikov A, Saldanha R, Salvo C, Schönert S, Simgen H, Skorokhvatov M, Smirnov O, Sotnikov A, Sukhotin S, Suvorov Y, Tartaglia R, Testera G, Vignaud D, Vogelaar RB, von Feilitzsch F, Winter J, Wojcik M, Wright A, Wurm M, Xu J, Zaimidoroga O, Zavatarelli S, and Zuzel G
Abstract: We observed, for the first time, solar neutrinos in the 1.0-1.5 MeV energy range. We determined the rate of pep solar neutrino interactions in Borexino to be 3.1±0.6{stat}±0.3{syst} counts/(day·100 ton). Assuming the pep neutrino flux predicted by the standard solar model, we obtained a constraint on the CNO solar neutrino interaction rate of <7.9 counts/(day·100 ton) (95% C.L.). The absence of the solar neutrino signal is disfavored at 99.97% C.L., while the absence of the pep signal is disfavored at 98% C.L. The necessary sensitivity was achieved by adopting data analysis techniques for the rejection of cosmogenic {11}C, the dominant background in the 1-2 MeV region. Assuming the Mikheyev-Smirnov-Wolfenstein large mixing angle solution to solar neutrino oscillations, these values correspond to solar neutrino fluxes of (1.6±0.3)×10{8} cm{-2} s^{-1} and <7.7×10{8} cm{-2} s{-1} (95% C.L.), respectively, in agreement with both the high and low metallicity standard solar models. These results represent the first direct evidence of the pep neutrino signal and the strongest constraint of the CNO solar neutrino flux to date.
Published: 2012
Full Text: View/download PDF

45. Precision measurement of the (7)Be solar neutrino interaction rate in Borexino.

Author: Bellini G, Benziger J, Bick D, Bonetti S, Bonfini G, Buizza Avanzini M, Caccianiga B, Cadonati L, Calaprice F, Carraro C, Cavalcante P, Chavarria A, D'Angelo D, Davini S, 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 A, Ianni A, Kobychev V, Korablev D, Korga G, Koshio Y, Kryn D, Laubenstein M, Lewke T, Litvinovich E, Loer B, Lombardi F, Lombardi P, 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, Peña-Garay C, Perasso L, Perasso S, Pocar A, Raghavan RS, Ranucci G, Razeto A, Re A, Romani A, Sabelnikov A, Saldanha R, Salvo C, Schönert S, Simgen H, Skorokhvatov M, Smirnov O, Sotnikov A, Sukhotin S, Suvorov Y, Tartaglia R, Testera G, Vignaud D, Vogelaar RB, von Feilitzsch F, Winter J, Wojcik M, Wright A, Wurm M, Xu J, Zaimidoroga O, Zavatarelli S, and Zuzel G
Abstract: The rate of neutrino-electron elastic scattering interactions from 862 keV (7)Be solar neutrinos in Borexino is determined to be 46.0±1.5(stat)(-1.6)(+1.5)(syst) counts/(day·100 ton). This corresponds to a ν(e)-equivalent (7)Be solar neutrino flux of (3.10±0.15)×10(9) cm(-2) s(-1) and, under the assumption of ν(e) transition to other active neutrino flavours, yields an electron neutrino survival probability of 0.51±0.07 at 862 keV. The no flavor change hypothesis is ruled out at 5.0 σ. A global solar neutrino analysis with free fluxes determines Φ(pp)=6.06(-0.06)(+0.02)×10(10) cm(-2) s(-1) and Φ(CNO)<1.3×10(9) cm(-2) s(-1) (95% C.L.). These results significantly improve the precision with which the Mikheyev-Smirnov-Wolfenstein large mixing angle neutrino oscillation model is experimentally tested at low energy.
Published: 2011
Full Text: View/download PDF

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

Publication Type

Journal

Database

Publisher

45 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