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244 results on '"Cribier, M"'

1. The Double Chooz antineutrino detectors

Author

Double Chooz Collaboration, de Kerret, H., Abe, Y., Aberle, C., Abrahão, T., Ahijado, J. M., Akiri, T., Alarcón, J. M., Alba, J., Almazan, H., Anjos, J. C. dos, Appel, S., Ardellier, F., Barabanov, I., Barriere, J. C., Baussan, E., Baxter, A., Bekman, I., Bergevin, M., Bernstein, A., Bertoli, W., Bezerra, T. J. C., Bezrukov, L., Blanco, C., Bleurvacq, N., Blucher, E., Bonet, H., Bongrand, M., Bowden, N. S, Brugière, T., Buck, C., Avanzini, M. Buizza, Busenitz, J., Cabrera, A., Calvo, E., Camilleri, L., Carr, R., Cazaux, S., Cela, J. M., Cerrada, M., Chang, P. J., Charon, P., Chauveau, E., Chimenti, P., Classen, T., Collin, A. P., Conover, E., Conrad, J. M, Cormon, S., Corpace, O., Courty, B., Crespo-Anadón, J. I., Cribier, M., Crum, K., Cuadrado, S., Cucoanes, A., D'Agostino, M., Damon, E., Dawson, J. V., Dazeley, S., Dierckxsens, M., Dietrich, D., Djurcic, Z., Dorigo, F., Dracos, M., Durand, V., Efremekov, Y., Elnimr, M., Etenko, A., Falk, E., Fallot, M., Fechner, M., Felde, J., Fernandes, S. M., Fernández-Bedoya, C., Francia, D., Franco, D., Fischer, V., Franke, A. J., Franke, M., Furuta, H., Garcia, F., Garcia, J., Gil-Botella, I., Giot, L., Givaudan, A., Göger-Neff, M., Gomez, H., Gonzalez, L. F. G., Goodenough, L., Goodman, M. C., Goon, J., Gramlich, B., Greiner, D., Guertin, A., Guillon, B., Habib, S. M., Haddad, Y., Hara, T., Hartmann, F. X., Hartnell, J., Haser, J., Hatzikoutelis, A., Hellwig, D., Hervé, S., Hofacker, R., Horton-Smith, G., Hourlier, A., Ishitsuka, M., Jänner, K., Jiménez, S., Jochum, J., Jollet, C., Kaether, F., Kale, K., Kalousis, L., Kamyshkov, Y., Kaneda, M., Kaplan, D. M., Karakac, M., Kawasaki, T., Kemp, E., Kibe, Y., Kirchner, T., Konno, T., Kryn, D., Kutter, T., Kuze, M., Lachenmaier, T., Lane, C. E., Langbrandtner, C., Lasserre, T., Lastoria, C., Latron, L., Leonardo, C., Letourneau, A., Lhuillier, D., Lima Jr, H. P., Lindner, M., López-Castaño, J. M., LoSecco, J. M., Lubsandorzhiev, B., Lucht, S., Maeda, J., Maesano, C. N., Mariani, C., Maricic, J., Marie, F., Martinez, J. J., Martino, J., Matsubara, T., McKee, D., Meigner, F., Mention, G., Meregaglia, A., Meyer, J. P., Miletic, T., Milincic, R., Millot, J. F., Minotti, A., Mirones, V., Miyata, H., Mueller, Th. A., Nagasaka, Y., Nakajima, K., Navas-Nicolás, D., Nikitenko, Y., Novella, P., Oberauer, L., Obolensky, M., Onillon, A., Oralbaev, A., Ostrovskiy, I., Palomares, C., Peeters, S. J. M., Pepe, I. M., Perasso, S., Perrin, P., Pfahler, P., Porta, A., Pronost, G., Puras, J. C., Quéval, R., Ramirez, J. L., Reichenbacher, J., Reinhold, B., Reissfelder, M., Remoto, A., Reyna, D., Rodriguez, I., Röhling, M., Roncin, R., Rudolf, N., Rybolt, B., Sakamoto, Y., Santorelli, R., Sato, F., Schwan, U., Scola, L., Settimo, M., Schönert, S., Schoppmann, S., Shaevitz, M. A., Sharankova, R., Sibille, V., Sida, J. L., Sinev, V., Shrestha, D., Skorokhvatov, M., Soldin, P., Spitz, J., Stahl, A., Stancu, I., Starzynski, P., Stock, M. R., Stokes, L. F. F., Strait, M., Stüken, A., Suekane, F., Sukhotin, S., Sumiyoshi, T., Sun, Y., Sun, Z., Svoboda, R., Tabata, H., Tamura, N., Terao, K., Tonazzo, A., Toral, F., Toups, M., Thi, H. Trinh, Valdivia, F., Valdiviesso, G., Vassilopoulos, N., Verdugo, A., Veyssiere, C., Viaud, B., Vignaud, D., Vivier, M., Wagner, S., Wiebusch, C., White, B., Winslow, L., Worcester, M., Wurm, M., Wurtz, J., Yang, G., Yáñez, J., Yermia, F., and Zbiri, K.

Subjects
Physics - Instrumentation and Detectors
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. 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., Comment: 49 pages, 29 figures

Published
2022
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2. The Double Chooz antineutrino detectors

Author

de Kerret, H., Abe, Y., Aberle, C., Abrahão, T., Ahijado, J. M., Akiri, T., Alarcón, J. M., Alba, J., Almazan, H., dos Anjos, J. C., Appel, S., Ardellier, F., Barabanov, I., Barriere, J. C., Baussan, E., Baxter, A., Bekman, I., Bergevin, M., Bernstein, A., Bertoli, W., Bezerra, T. J. C., Bezrukov, L., Blanco, C., Bleurvacq, N., Blucher, E., Bonet, H., Bongrand, M., Bowden, N. S, Brugière, T., Buck, C., Avanzini, M. Buizza, Busenitz, J., Cabrera, A., Caden, E., Calvo, E., Camilleri, L., Carr, R., Cazaux, S., Cela, J. M., Cerrada, M., Chang, P. J., Charon, P., Chauveau, E., Chimenti, P., Classen, T., Collin, A. P., Conover, E., Conrad, J. M, Cormon, S., Corpace, O., Courty, B., Crespo-Anadón, J. I., Cribier, M., Crum, K., Cuadrado, S., Cucoanes, A., D’Agostino, M., Damon, E., Dawson, J. V., Dazeley, S., Dierckxsens, M., Dietrich, D., Djurcic, Z., Dorigo, F., Dracos, M., Durand, V., Efremeko, Y., Elnimr, M., Etenko, A., Falk, E., Fallot, M., Fechner, M., Felde, J., Fernandes, S. M., Fernández-Bedoya, C., Francia, D., Franco, D., Fischer, V., Franke, A. J., Franke, M., Furuta, H., Garcia, F., Garcia, J., Gil-Botella, I., Giot, L., Givaudan, A., Göger-Neff, M., Gomez, H., Gonzalez, L. F. G., Goodenough, L., Goodman, M. C., Goon, J., Gramlich, B., Greiner, D., Guertin, A., Guillon, B., Habib, S. M., Haddad, Y., Hara, T., Hartmann, F. X., Hartnell, J., Haser, J., Hatzikoutelis, A., Hellwig, D., Hervé, S., Hofacker, R., Horton-Smith, G., Hourlier, A., Ishitsuka, M., Jänner, K., Jiménez, S., Jochum, J., Jollet, C., Kaether, F., Kale, K., Kalousis, L., Kamyshkov, Y., Kaneda, M., Kaplan, D. M., Karakac, M., Kawasaki, T., Kemp, E., Kibe, Y., Kirchner, T., Konno, T., Kryn, D., Kutter, T., Kuze, M., Lachenmaier, T., Lane, C. E., Langbrandtner, C., Lasserre, T., Lastoria, C., Latron, L., Leonardo, C., Letourneau, A., Lhuillier, D., Lima, Jr, H. P., Lindner, M., López-Castaño, J. M., LoSecco, J. M., Lubsandorzhiev, B., Lucht, S., Maeda, J., Maesano, C. N., Mariani, C., Maricic, J., Marie, F., Martinez, J. J., Martino, J., Matsubara, T., McKee, D., Meigner, F., Mention, G., Meregaglia, A., Meyer, J. P., Miletic, T., Milincic, R., Millot, J. F., Minotti, A., Mirones, V., Miyata, H., Mueller, Th. A., Nagasaka, Y., Nakajima, K., Navas-Nicolás, D., Nikitenko, Y., Novella, P., Oberauer, L., Obolensky, M., Onillon, A., Oralbaev, A., Ostrovskiy, I., Palomares, C., Peeters, S. J. M., Pepe, I. M., Perasso, S., Perrin, P., Pfahler, P., Porta, A., Pronost, G., Puras, J. C., Quéval, R., Ramirez, J. L., Reichenbacher, J., Reinhold, B., Reissfelder, M., Remoto, A., Reyna, D., Rodriguez, I., Röhling, M., Roncin, R., Rudolf, N., Rybolt, B., Sakamoto, Y., Santorelli, R., Sato, F., Schwan, U., Schönert, S., Schoppmann, S., Scola, L., Settimo, M., Shaevitz, M. A., Sharankova, R., Sibille, V., Sida, J.-L., Sinev, V., Shrestha, D., Skorokhvatov, M., Soldin, P., Spitz, J., Stahl, A., Stancu, I., Starzynski, P., Stock, M. R., Stokes, L. F. F., Strait, M., Stüken, A., Suekane, F., Sukhotin, S., Sumiyoshi, T., Sun, Y., Sun, Z., Svoboda, R., Tabata, H., Tamura, N., Terao, K., Tonazzo, A., Toral, F., Toups, M., Thi, H. Trinh, Valdivia, F., Valdiviesso, G., Vassilopoulos, N., Verdugo, A., Veyssiere, C., Viaud, B., Vignaud, D., Vivier, M., Wagner, S., Wiebusch, C., White, B., Winslow, L., Worcester, M., Wurm, M., Wurtz, J., Yang, G., Yáñez, J., Yermia, F., and Zbiri, K.

Published
2022
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3. Direct Search for keV Sterile Neutrino Dark Matter with a Stable Dysprosium Target

Author

Lasserre, T., Altenmueller, K., Cribier, M., Merle, A., Mertens, S., and Vivier, M.

Subjects
High Energy Physics - Experiment, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Phenomenology
Abstract

We investigate a new method to search for keV-scale sterile neutrinos that could account for Dark Matter. Neutrinos trapped in our galaxy could be captured on stable $^{163}$Dy if their mass is greater than 2.83 keV. Two experimental realizations are studied, an integral counting of $^{163}$Ho atoms in dysprosium-rich ores and a real-time measurement of the emerging electron spectrum in a dysprosium-based detector. The capture rates are compared to the solar neutrino and radioactive backgrounds. An integral counting experiment using several kilograms of $^{163}$Dy could reach a sensitivity for the sterile-to-active mixing angle $\sin^2\theta_{e4}$ of $10^{-5}$ significantly exceeding current laboratory limits. Mixing angles as low as $\sin^2\theta_{e4} \sim 10^{-7}$ / $\rm m_{^{163}\rm Dy}\rm{(ton)}$ could possibly be explored with a real-time experiment., Comment: 7 pages, 5 figures - v2 add references

Published
2016

4. Online Monitoring of the Osiris Reactor with the Nucifer Neutrino Detector

Author

Boireau, G., Bouvet, L., Collin, A. P., Coulloux, G., Cribier, M., Deschamp, H., Durand, V., Fechner, M., Fischer, V., Gaffiot, J., Castaing, N. Gerard, Granelli, R., Kato, Y., Lasserre, T., Latron, L., Legou, P., Letourneau, A., Lhuillier, D., Mention, G., Mueller, T., Nghiem, T-A., Pedrol, N., Pelzer, J., Pequignot, M., Piret, Y., Prono, G., Scola, L., Starzinski, P., Vivier, M., Dumonteil, E., Varignon, C., Buck, C., Lindner, M., Bazoma, J., Bouvier, S., Bui, V. M., Communeau, V., Cucoanes, A., Fallot, M., Gautier, M., Giot, L., Guilloux, G., Lenoir, M., Martino, J., Mercier, G., Milleto, T., Peuvrel, N., Porta, A., Quere, N. Le, Renard, C., Rigalleau, L. M., Roy, D., Vilajosana, T., and Yermia, F.

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract

Originally designed as a new nuclear reactor monitoring device, the Nucifer detector has successfully detected its first neutrinos. We provide the second shortest baseline measurement of the reactor neutrino flux. The detection of electron antineutrinos emitted in the decay chains of the fission products, combined with reactor core simulations, provides an new tool to assess both the thermal power and the fissile content of the whole nuclear core and could be used by the Inter- national Agency for Atomic Energy (IAEA) to enhance the Safeguards of civil nuclear reactors. Deployed at only 7.2m away from the compact Osiris research reactor core (70MW) operating at the Saclay research centre of the French Alternative Energies and Atomic Energy Commission (CEA), the experiment also exhibits a well-suited configuration to search for a new short baseline oscillation. We report the first results of the Nucifer experiment, describing the performances of the 0.85m3 detector remotely operating at a shallow depth equivalent to 12m of water and under intense background radiation conditions. Based on 145 (106) days of data with reactor ON (OFF), leading to the detection of an estimated 40760 electron antineutrinos, the mean number of detected antineutrinos is 281 +- 7(stat) +- 18(syst) electron antineutrinos/day, in agreement with the prediction 277(23) electron antineutrinos/day. Due the the large background no conclusive results on the existence of light sterile neutrinos could be derived, however. As a first societal application we quantify how antineutrinos could be used for the Plutonium Management and Disposition Agreement., Comment: 22 pages, 16 figures - Version 4

Published
2015
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5. Prompt directional detection of galactic supernova by combining large liquid scintillator neutrino detectors

Author

Fischer, V., Chirac, T., Lasserre, T., Volpe, C., Cribier, M., Durero, M., Gaffiot, J., Houdy, T., Letourneau, A., Mention, G., Pequignot, M., Sibille, V., and Vivier, M.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Phenomenology, Physics - Instrumentation and Detectors
Abstract

Core-collapse supernovae produce an intense burst of electron antineutrinos in the few-tens-of-MeV range. Several Large Liquid Scintillator-based Detectors (LLSD) are currently operated worldwide, being very effective for low energy antineutrino detection through the Inverse Beta Decay (IBD) process. In this article, we develop a procedure for the prompt extraction of the supernova location by revisiting the details of IBD kinematics over the broad energy range of supernova neutrinos. Combining all current scintillator-based detector, we show that one can locate a canonical supernova at 10 kpc with an accuracy of 45 degrees (68% C.L.). After the addition of the next generation of scintillator-based detectors, the accuracy could reach 12 degrees (68% C.L.), therefore reaching the performances of the large water Cerenkov neutrino detectors. We also discuss a possible improvement of the SuperNova Early Warning System (SNEWS) inter-experiment network with the implementation of a directionality information in each experiment. Finally, we discuss the possibility to constrain the neutrino energy spectrum as well as the mass of the newly born neutron star with the LLSD data, Comment: 25 pages, 21 figures, accepted for Publication in Journal of Cosmology and Astroparticle Physics (JCAP); v2 with added references, corrected typos and errors in Section 6; v3 is the published version

Published
2015
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6. Experimental Parameters for a Cerium 144 Based Intense Electron Antineutrino Generator Experiment at Very Short Baselines

Author

Gaffiot, J., Lasserre, T., Mention, G., Vivier, M., Cribier, M., Durero, M., Fischer, V., Letourneau, A., Dumonteil, E., Saldikov, I. S., and Tikhomirov, G. V.

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract

The standard three-neutrino oscillation paradigm, associated with small squared mass splittings $\ll 0.1\ \mathrm{eV^2}$, has been successfully built up over the last 15 years using solar, atmospheric, long baseline accelerator and reactor neutrino experiments. However, this well-established picture might suffer from anomalous results reported at very short baselines in some of these experiments. If not experimental artifacts, such results could possibly be interpreted as the existence of at least an additional fourth sterile neutrino species, mixing with the known active flavors with an associated mass splitting $\ll 0.1\ \mathrm{eV^2}$, and being insensitive to standard weak interactions. Precision measurements at very short baselines (5 to 15 m) with intense MeV electronic antineutrino emitters can be used to probe these anomalies. In this article, the expected antineutrino signal and backgrounds of a generic experiment which consists of deploying an intense beta minus radioactive source inside or in the vicinity of a large liquid scintillator detector are studied. The technical challenges to perform such an experiment are identified, along with quantifying the possible source and detector induced systematics, and their impact on the sensitivity to the observation of neutrino oscillations at short baselines., Comment: 21 pages, 27 figures, generated with pdflatex, accepted for publication in Phys. Rev. D

Published
2014
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7. CeLAND: search for a 4th light neutrino state with a 3 PBq 144Ce-144Pr electron antineutrino generator in KamLAND

Author

Gando, A., Gando, Y., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, H., Koga, M., Matsuda, R., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Oki, Y., Otani, M., Shimizu, I., Shirai, J., Suekane, F., Suzuki, A., Takemoto, Y., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Yamada, S., Yamauchi, Y., Yoshida, H., Cribier, M., Durero, M., Fischer, V., Gaffiot, J., Jonqueres, N., Kouchner, A., Lasserre, T., Leterme, D., Letourneau, A., Lhuillier, D., Mention, G., Rampal, G., Scola, L., Veyssiere, Ch., Vivier, M., Yala, P., Berger, B. E., Kozlov, A., Banks, T., Dwyer, D., Fujikawa, B. K., Han, K., Kolomensky, Yu. G., Mei, Y., O'Donnell, T., Decowski, P., Markoff, D. M., Yoshida, S., Kornoukhov, V. N., Gelis, T. V. M., Tikhomirov, G. V., Learned, J. G., Maricic, J., Matsuno, S., Milincic, R., Karwowski, H. J., Efremenko, Y., Detwiler, A., and Enomoto, S.

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract

The reactor neutrino and gallium anomalies can be tested with a 3-4 PBq (75-100 kCi scale) 144Ce-144Pr antineutrino beta-source deployed at the center or next to a large low-background liquid scintillator detector. The antineutrino generator will be produced by the Russian reprocessing plant PA Mayak as early as 2014, transported to Japan, and deployed in the Kamioka Liquid Scintillator Anti-Neutrino Detector (KamLAND) as early as 2015. KamLAND's 13 m diameter target volume provides a suitable environment to measure the energy and position dependence of the detected neutrino flux. A characteristic oscillation pattern would be visible for a baseline of about 10 m or less, providing a very clean signal of neutrino disappearance into a yet-unknown, sterile neutrino state. This will provide a comprehensive test of the electron dissaperance neutrino anomalies and could lead to the discovery of a 4th neutrino state for Delta_m^2 > 0.1 eV^2 and sin^2(2theta) > 0.05., Comment: 67 pages, 50 figures. Th. Lasserre thanks the European Research Council for support under the Starting Grant StG-307184

Published
2013

8. White paper: CeLAND - Investigation of the reactor antineutrino anomaly with an intense 144Ce-144Pr antineutrino source in KamLAND

Author

Gando, A., Gando, Y., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, H., Koga, M., Matsuda, R., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Oki, Y., Otani, M., Shimizu, I., Shirai, J., Suekane, F., Suzuki, A., Takemoto, Y., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Yamada, S., Yamauchi, Y., Yoshida, H., Banks, T., Berger, B. E., Cribier, M., Decowski, P., Detwiler, J. A., Durero, M., Dwyer, D., Efremenko, Y., Enomoto, S., Fischer, V., Fujikawa, B. K., Gaffiot, J., Gelis, V. M., Karwowski, H. J., Kolomensky, Yu. G., Kozlov, A., Kornoukhov, V. N., Lasserre, T., Learned, J. G., Letourneau, A., Lhuillier, D., Maricic, J., Markoff, D. M., Matsuno, S., Mention, G., Milincic, R., ODonnell, T., Saldikov, I. S., Scola, L., Tikhomirov, G. V., Veyssiere, Ch., Vivier, M., and Yoshida, S.

Subjects
High Energy Physics - Experiment
Abstract

We propose to test for short baseline neutrino oscillations, implied by the recent reevaluation of the reactor antineutrino flux and by anomalous results from the gallium solar neutrino detectors. The test will consist of producing a 75 kCi 144Ce - 144Pr antineutrino source to be deployed in the Kamioka Liquid Scintillator Anti-Neutrino Detector (KamLAND). KamLAND's 13m diameter target volume provides a suitable environment to measure energy and position dependence of the detected neutrino flux. A characteristic oscillation pattern would be visible for a baseline of about 10 m or less, providing a very clean signal of neutrino disappearance into a yet-unknown, "sterile" state. Such a measurement will be free of any reactor-related uncertainties. After 1.5 years of data taking the Reactor Antineutrino Anomaly parameter space will be tested at > 95% C.L., Comment: White paper prepared for Snowmass-2013; slightly different author list

Published
2013

9. Light Sterile Neutrinos: A White Paper

Author

Abazajian, K. N., Acero, M. A., Agarwalla, S. K., Aguilar-Arevalo, A. A., Albright, C. H., Antusch, S., Arguelles, C. A., Balantekin, A. B., Barenboim, G., Barger, V., Bernardini, P., Bezrukov, F., Bjaelde, O. E., Bogacz, S. A., Bowden, N. S., Boyarsky, A., Bravar, A., Berguno, D. Bravo, Brice, S. J., Bross, A. D., Caccianiga, B., Cavanna, F., Chun, E. J., Cleveland, B. T., Collin, A. P., Coloma, P., Conrad, J. M., Cribier, M., Cucoanes, A. S., D'Olivo, J. C., Das, S., de Gouvea, A., Derbin, A. V., Dharmapalan, R., Diaz, J. S., Ding, X. J., Djurcic, Z., Donini, A., Duchesneau, D., Ejiri, H., Elliott, S. R., Ernst, D. J., Esmaili, A., Evans, J. J., Fernandez-Martinez, E., Figueroa-Feliciano, E., Fleming, B. T., Formaggio, J. A., Franco, D., Gaffiot, J., Gandhi, R., Gao, Y., Garvey, G. T., Gavrin, V. N., Ghoshal, P., Gibin, D., Giunti, C., Gninenko, S. N., Gorbachev, V. V., Gorbunov, D. S., Guenette, R., Guglielmi, A., Halzen, F., Hamann, J., Hannestad, S., Haxton, W., Heeger, K. M., Henning, R., Hernandez, P., Huber, P., Huelsnitz, W., Ianni, A., Ibragimova, T. V., Karadzhov, Y., Karagiorgi, G., Keefer, G., Kim, Y. D., Kopp, J., Kornoukhov, V. N., Kusenko, A., Kyberd, P., Langacker, P., Lasserre, Th., Laveder, M., Letourneau, A., Lhuillier, D., Li, Y. F., Lindner, M., Link, J. M., Littlejohn, B. L., Lombardi, P., Long, K., Lopez-Pavon, J., Louis, W. C., Ludhova, L., Lykken, J. D., Machado, P. A. N., Maltoni, M., Mann, W. A., Marfatia, D., Mariani, C., Matveev, V. A., Mavromatos, N. E., Melchiorri, A., Meloni, D., Mena, O., Mention, G., Merle, A., Meroni, E., Mezzetto, M., Mills, G. B., Minic, D., Miramonti, L., Mohapatra, D., Mohapatra, R. N., Montanari, C., Mori, Y., Mueller, Th. A., Mumm, H. P., Muratova, V., Nelson, A. E., Nico, J. S., Noah, E., Nowak, J., Smirnov, O. Yu., Obolensky, M., Pakvasa, S., Palamara, O., Pallavicini, M., Pascoli, S., Patrizii, L., Pavlovic, Z., Peres, O. L. G., Pessard, H., Pietropaolo, F., Pitt, M. L., Popovic, M., Pradler, J., Ranucci, G., Ray, H., Razzaque, S., Rebel, B., Robertson, R. G. H., Rodejohann, W., Rountree, S. D., Rubbia, C., Ruchayskiy, O., Sala, P. R., Scholberg, K., Schwetz, T., Shaevitz, M. H., Shaposhnikov, M., Shrock, R., Simone, S., Skorokhvatov, M., Sorel, M., Sousa, A., Spergel, D. N., Spitz, J., Stanco, L., Stancu, I., Suzuki, A., Takeuchi, T., Tamborra, I., Tang, J., Testera, G., Tian, X. C., Tonazzo, A., Tunnell, C. D., Van de Water, R. G., Verde, L., Veretenkin, E. P., Vignoli, C., Vivier, M., Vogelaar, R. B., Wascko, M. O., Wilkerson, J. F., Winter, W., Wong, Y. Y. Y., Yanagida, T. T., Yasuda, O., Yeh, M., Yermia, F., Yokley, Z. W., Zeller, G. P., Zhan, L., and Zhang, H.

Subjects
High Energy Physics - Phenomenology, Astrophysics - Cosmology and Extragalactic Astrophysics, High Energy Physics - Experiment, Nuclear Experiment, Nuclear Theory
Abstract

This white paper addresses the hypothesis of light sterile neutrinos based on recent anomalies observed in neutrino experiments and the latest astrophysical data.

Published
2012

10. Indication for the disappearance of reactor electron antineutrinos in the Double Chooz experiment

Author

Abe, Y., Aberle, C., Akiri, T., Anjos, J. C. dos, Ardellier, F., Barbosa, A. F., Baxter, A., Bergevin, M., Bernstein, A., Bezerra, T. J. C., Bezrukhov, L., Blucher, E., Bongrand, M., Bowden, N. S., Buck, C., Busenitz, J., Cabrera, A., Caden, E., Camilleri, L., Carr, R., Cerrada, M., Chang, P. -J., Chimenti, P., Classen, T., Collin, A. P., Conover, E., Conrad, J. M., Cormon, S., Crespo-Anadón, J. I., Cribier, M., Crum, K., Cucoanes, A., D'Agostino, M. V., Damon, E., Dawson, J. V., 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, S. M., Franco, D., Franke, A. J., Franke, M., Furuta, H., Gama, R., Gil-Botella, I., Giot, L., Göger-Neff, M., Gonzalez, L. F. G., Goodman, M. C., Goon, J. TM., Greiner, D., Guillon, B., Haag, N., Hagner, C., Hara, T., Hartmann, F. X., Hartnell, J., Haruna, T., Haser, J., Hatzikoutelis, A., Hayakawa, T., Hofmann, M., Horton-Smith, G. A., Ishitsuka, M., Jochum, J., Jollet, C., Jones, C. L., Kaether, F., Kalousis, L., Kamyshkov, Y., Kaplan, D. M., Kawasaki, T., Keefer, G., Kemp, E., de Kerret, H., Kibe, Y., Konno, T., Kryn, D., Kuze, M., Lachenmaier, T., Lane, C. E., Langbrandtner, C., Lasserre, T., Letourneau, A., Lhuillier, D., Lima Jr, H. P., Lindner, M., Liu, Y., López-Castanõ, J. M., LoSecco, J. M., Lubsandorzhiev, B. K., Lucht, S., McKee, D., Maeda, J., Maesano, C. N., Mariani, C., Maricic, J., Martino, J., Matsubara, T., Mention, G., Meregaglia, A., Miletic, T., Milincic, R., Milzstajn, A., Miyata, H., Motta, D., Mueller, Th. A., Nagasaka, Y., Nakajima, K., Novella, P., Obolensky, M., Oberauer, L., Onillon, A., Osborn, A., Ostrovskiy, I., Palomares, C., Peeters, S. J. M., Pepe, I. M., 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, H. A., Sakamoto, Y., Santorelli, R., Sato, F., Schönert, S., Schoppmann, S., Schwan, U., Schwetz, T., Shaevitz, M. H., Shrestha, D., Sida, J-L., 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., Thi, H. H. Trinh, 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.

Subjects
High Energy Physics - Experiment
Abstract

The Double Chooz Experiment presents an indication of reactor electron antineutrino disappearance consistent with neutrino oscillations. A ratio of 0.944 $\pm$ 0.016 (stat) $\pm$ 0.040 (syst) observed to predicted events 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 measurement as an anchor point. The deficit can be interpreted as an indication of a non-zero value of the still unmeasured neutrino mixing parameter \sang. Analyzing both the rate of the prompt positrons and their energy spectrum we find \sang = 0.086 $\pm$ 0.041 (stat) $\pm$ 0.030 (syst), or, at 90% CL, 0.015 $<$ \sang $\ <$ 0.16., Comment: 7 pages, 4 figures, (new version after PRL referee's comments)

Published
2011
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11. The Reactor Antineutrino Anomaly

Author

Mention, G., Fechner, M., Lasserre, Th., Mueller, Th. A., Lhuillier, D., Cribier, M., and Letourneau, A.

Subjects
High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract

Recently new reactor antineutrino spectra have been provided for 235U, 239Pu, 241Pu and 238U, increasing the mean flux by about 3 percent. To good approximation, this reevaluation applies to all reactor neutrino experiments. The synthesis of published experiments at reactor-detector distances <100 m leads to a ratio of observed event rate to predicted rate of 0.976(0.024). With our new flux evaluation, this ratio shifts to 0.943(0.023), leading to a deviation from unity at 98.6% C.L. which we call the reactor antineutrino anomaly. The compatibility of our results with the existence of a fourth non-standard neutrino state driving neutrino oscillations at short distances is discussed. The combined analysis of reactor data, gallium solar neutrino calibration experiments, and MiniBooNE-neutrino data disfavors the no-oscillation hypothesis at 99.8% C.L. The oscillation parameters are such that |Delta m_{new}^2|>1.5 eV^2 (95%) and sin^2(2\theta_{new})=0.14(0.08) (95%). Constraints on the theta13 neutrino mixing angle are revised., Comment: 19 pages, 15 figures ; v2/3 include typos corrected ; v4 final version: add 5 Rovno & 2 Savannah River results + add additional constistency checks + add a discussion on the inverse beta decay cross section normlization

Published
2011
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12. CeLAND: search for a 4th light neutrino state with a 3 PBq 144Ce-144Pr electron antineutrino generator in KamLAND

Author

Gando, A, Gando, Y, Hayashida, S, Ikeda, H, Inoue, K, Ishidoshiro, K, Ishikawa, H, Koga, M, Matsuda, R, Matsuda, S, Mitsui, T, Motoki, D, Nakamura, K, Oki, Y, Otani, M, Shimizu, I, Shirai, J, Suekane, F, Suzuki, A, Takemoto, Y, Tamae, K, Ueshima, K, Watanabe, H, Xu, BD, Yamada, S, Yamauchi, Y, Yoshida, H, Cribier, M, Durero, M, Fischer, V, Gaffiot, J, Jonqueres, N, Kouchner, A, Lasserre, T, Leterme, D, Letourneau, A, Lhuillier, D, Mention, G, Rampal, G, Scola, L, Veyssiere, Ch, Vivier, M, Yala, P, Berger, BE, Kozlov, A, Banks, T, Dwyer, D, Fujikawa, BK, Han, K, Kolomensky, Yu G, Mei, Y, O'Donnell, T, Decowski, P, Markoff, DM, Yoshida, S, Kornoukhov, VN, Gelis, TVM, Tikhomirov, GV, Learned, JG, Maricic, J, Matsuno, S, Milincic, R, Karwowski, HJ, Efremenko, Y, Detwiler, A, and Enomoto, S

Subjects
physics.ins-det, hep-ex
Abstract

The reactor neutrino and gallium anomalies can be tested with a 3-4 PBq(75-100 kCi scale) 144Ce-144Pr antineutrino beta-source deployed at the centeror next to a large low-background liquid scintillator detector. Theantineutrino generator will be produced by the Russian reprocessing plant PAMayak as early as 2014, transported to Japan, and deployed in the KamiokaLiquid Scintillator Anti-Neutrino Detector (KamLAND) as early as 2015.KamLAND's 13 m diameter target volume provides a suitable environment tomeasure the energy and position dependence of the detected neutrino flux. Acharacteristic oscillation pattern would be visible for a baseline of about 10m or less, providing a very clean signal of neutrino disappearance into ayet-unknown, sterile neutrino state. This will provide a comprehensive test ofthe electron dissaperance neutrino anomalies and could lead to the discovery ofa 4th neutrino state for Delta_m^2 > 0.1 eV^2 and sin^2(2theta) > 0.05.

Published
2013

13. Reactor Monitoring with Neutrinos

Author

Cribier, M.

Subjects
Nuclear Experiment
Abstract

The fundamental knowledge on neutrinos acquired in the recent years open the possibility of applied neutrino physics. Among it the automatic and non intrusive monitoring of nuclear reactor by its antineutrino signal could be very valuable to IAEA in charge of the control of nuclear power plants. Several efforts worldwide have already started., Comment: 5 pages - XXII International Conference On Neutrino Physics And Astrophysics (Neutrino 2006)

Published
2007
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14. Neutrinos and Non-proliferation in Europe

Author

Cribier, M.

Subjects
Nuclear Experiment
Abstract

Triggered by the demand of the IAEA, neutrino physicists in Europe involved with the Double Chooz experiment are studying the potential of neutrino detection to monitor nuclear reactors. In particular a new set of experiments at the ILL is planned to improve the knowledge of the neutrino spectrum emitted in the fission of 235U and 239Pu.

Published
2007
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15. Complete results for five years of GNO solar neutrino observations

Author

GNO COLLABORATION, Altmann, M., Balata, M., Belli, P., Bellotti, E., Bernabei, R., Burkert, E., Cattadori, C., Cerulli, R., Chiarini, M., Cribier, M., d'Angelo, S., Del Re, G., Ebert, K. H., Feilitzsch, F. v., Ferrari, N., Hampel, W., Hartmann, F. X., Henrich, E., Heusser, G., Kaether, F., Kiko, J., Kirsten, T., Lachenmaier, T., Lanfranchi, J., Laubenstein, M., Luetzenkirchen, K., Mayer, K., Moegel, P., Motta, D., Nisi, S., Oehm, J., Pandola, L., Petricca, F., Potzel, W., Richter, H., Schoenert, S., Wallenius, M., Wojcik, M., and Zanotti, L.

Subjects
High Energy Physics - Experiment, Astrophysics
Abstract

We report the complete GNO solar neutrino results for the measuring periods GNO III, GNO II, and GNO I. The result for GNO III (last 15 solar runs) is [54.3 + 9.9 - 9.3 (stat.)+- 2.3 (syst.)] SNU (1 sigma) or [54.3 + 10.2 - 9.6 (incl. syst.)] SNU (1 sigma) with errors combined. The GNO experiment is now terminated after altogether 58 solar exposure runs that were performed between May 20, 1998 and April 9, 2003. The combined result for GNO (I+II+III) is [62.9 + 5.5 - 5.3 (stat.) +- 2.5 (syst.)] SNU (1 sigma) or [62.9 + 6.0 - 5.9] SNU (1 sigma) with errors combined in quadrature. Overall, gallium based solar observations at LNGS (first in GALLEX, later in GNO) lasted from May 14, 1991 through April 9, 2003. The joint result from 123 runs in GNO and GALLEX is [69.3 +- 5.5 (incl. syst.)] SNU (1 sigma). The distribution of the individual run results is consistent with the hypothesis of a neutrino flux that is constant in time. Implications from the data in particle- and astrophysics are reiterated., Comment: 22 pages incl. 9 Figures and 8 Tables. to appear in: Physics Letters B (accepted April 13, 2005) PACS: 26.65.+t ; 14.60.Pq

Published
2005
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16. Letter of Intent for Double-CHOOZ: a Search for the Mixing Angle Theta13

Author

Ardellier, F., Barabanov, I., Barriere, J. C., Bauer, M., Bezrukov, L., Buck, C., Cattadori, C., Courty, B., Cribier, M., Dalnoki-Veress, F., Danilov, N., de Kerret, H., Di Vacri, A., Etenko, A., Fallot, M., Grieb, Ch., Goeger, M., Guertin, A., Kirchner, T., Krylov, Y. S., Kryn, D., Hagner, C., Hampel, W., Hartmann, F. X., Huber, P., Jochum, J., Lachenmaier, T., Lasserre, Th., Lendvai, Ch., Lindner, M., Marie, F., Martino, J., Mention, G., Milsztajn, A., Meyer, J. P., Motta, D., Oberauer, L., Obolensky, M., Pandola, L., Potzel, W., Schoenert, S., Schwan, U., Schwetz, T., Scholl, S., Scola, L., Skorokhvatov, M., Sukhotin, S., Letourneau, A., Vignaud, D., von Feilitzsch, F., Winter, W., and Yanovich, E.

Subjects
High Energy Physics - Experiment
Abstract

Tremendous progress has been achieved in neutrino oscillation physics during the last few years. However, the smallness of the $\t13$ neutrino mixing angle still remains enigmatic. The current best constraint comes from the CHOOZ reactor neutrino experiment $\s2t13 < 0.2$ (at 90% C.L., for $\adm2=2.0 10^{-3} \text{eV}^2$). We propose a new experiment on the same site, Double-CHOOZ, to explore the range of $\s2t13$ from 0.2 to 0.03, within three years of data taking. The improvement of the CHOOZ result requires an increase in the statistics, a reduction of the systematic error below one percent, and a careful control of the cosmic ray induced background. Therefore, Double-CHOOZ will use two identical detectors, one at $\sim$150 m and another at 1.05 km distance from the nuclear cores. The plan is to start data taking with two detectors in 2008, and to reach a sensitivity of 0.05 in 2009, and 0.03 in 2011., Comment: 102 pages, 9 chapters, 3 appendix. 43 figures

Published
2004

17. White paper: CeLAND - Investigation of the reactor antineutrino anomaly with an intense 144Ce-144Pr antineutrino source in KamLAND

Author

Gando, A, Gando, Y, Hayashida, S, Ikeda, H, Inoue, K, Ishidoshiro, K, Ishikawa, H, Koga, M, Matsuda, R, Matsuda, S, Mitsui, T, Motoki, D, Nakamura, K, Oki, Y, Otani, M, Shimizu, I, Shirai, J, Suekane, F, Suzuki, A, Takemoto, Y, Tamae, K, Ueshima, K, Watanabe, H, Xu, BD, Yamada, S, Yamauchi, Y, Yoshida, H, Banks, T, Berger, BE, Cribier, M, Decowski, P, Detwiler, JA, Durero, M, Dwyer, D, Efremenko, Y, Enomoto, S, Fischer, V, Fujikawa, BK, Gaffiot, J, Gelis, VM, Karwowski, HJ, Kolomensky, Yu G, Kozlov, A, Kornoukhov, VN, Lasserre, T, Learned, JG, Letourneau, A, Lhuillier, D, Maricic, J, Markoff, DM, Matsuno, S, Mention, G, Milincic, R, ODonnell, T, Saldikov, IS, Scola, L, Tikhomirov, GV, Veyssiere, Ch, Vivier, M, and Yoshida, S

Subjects
hep-ex
Abstract

We propose to test for short baseline neutrino oscillations, implied by therecent reevaluation of the reactor antineutrino flux and by anomalous resultsfrom the gallium solar neutrino detectors. The test will consist of producing a75 kCi 144Ce - 144Pr antineutrino source to be deployed in the Kamioka LiquidScintillator Anti-Neutrino Detector (KamLAND). KamLAND's 13m diameter targetvolume provides a suitable environment to measure energy and positiondependence of the detected neutrino flux. A characteristic oscillation patternwould be visible for a baseline of about 10 m or less, providing a very cleansignal of neutrino disappearance into a yet-unknown, "sterile" state. Such ameasurement will be free of any reactor-related uncertainties. After 1.5 yearsof data taking the Reactor Antineutrino Anomaly parameter space will be testedat > 95% C.L.

Published
2013

18. Light Sterile Neutrinos: A White Paper

Author

Abazajian, KN, Acero, MA, Agarwalla, SK, Aguilar-Arevalo, AA, Albright, CH, Antusch, S, Arguelles, CA, Balantekin, AB, Barenboim, G, Barger, V, Bernardini, P, Bezrukov, F, Bjaelde, OE, Bogacz, SA, Bowden, NS, Boyarsky, A, Bravar, A, Berguno, D Bravo, Brice, SJ, Bross, AD, Caccianiga, B, Cavanna, F, Chun, EJ, Cleveland, BT, Collin, AP, Coloma, P, Conrad, JM, Cribier, M, Cucoanes, AS, D'Olivo, JC, Das, S, Gouvea, A de, Derbin, AV, Dharmapalan, R, Diaz, JS, Ding, XJ, Djurcic, Z, Donini, A, Duchesneau, D, Ejiri, H, Elliott, SR, Ernst, DJ, Esmaili, A, Evans, JJ, Fernandez-Martinez, E, Figueroa-Feliciano, E, Fleming, BT, Formaggio, JA, Franco, D, Gaffiot, J, Gandhi, R, Gao, Y, Garvey, GT, Gavrin, VN, Ghoshal, P, Gibin, D, Giunti, C, Gninenko, SN, Gorbachev, VV, Gorbunov, DS, Guenette, R, Guglielmi, A, Halzen, F, Hamann, J, Hannestad, S, Haxton, W, Heeger, KM, Henning, R, Hernandez, P, Huber, P, Huelsnitz, W, Ianni, A, Ibragimova, TV, Karadzhov, Y, Karagiorgi, G, Keefer, G, Kim, YD, Kopp, J, Kornoukhov, VN, Kusenko, A, Kyberd, P, Langacker, P, Lasserre, Th, Laveder, M, Letourneau, A, Lhuillier, D, Li, YF, Lindner, M, Link, JM, Littlejohn, BL, Lombardi, P, Long, K, Lopez-Pavon, J, Louis, WC, Ludhova, L, Lykken, JD, Machado, PAN, Maltoni, M, Mann, WA, and Marfatia, D

Subjects
hep-ph, astro-ph.CO, hep-ex, nucl-ex, nucl-th
Abstract

This white paper addresses the hypothesis of light sterile neutrinos based onrecent anomalies observed in neutrino experiments and the latest astrophysicaldata.

Published
2012

19. GNO Solar Neutrino Observations: Results for GNOI

Author

GNO Collaboration, Altmann, M., Balata, M., Belli, P., Bellotti, E., Bernabei, R., Burkert, E., Cattadori, C., Cerichelli, G., Chiarini, M., Cribier, M., d'Angelo, S., Del Re, G., Ebert, K. H., Feilitzsch, F. v., Ferrari, N., Hampel, W., Handt, J., Henrich, E., Heusser, G., Kiko, J., Kirsten, T., Lachenmaier, T., Lanfranchi, J., Laubenstein, M., Motta, D., Rau, W., Richter, H., Waenninger, S., Wojcik, M., and Zanotti, L.

Subjects
High Energy Physics - Experiment, Astrophysics
Abstract

We report the first GNO solar neutrino results for the measuring period GNOI, solar exposure time May 20, 1998 till January 12, 2000. In the present analysis, counting results for solar runs SR1 - SR19 were used till April 4, 2000. With counting completed for all but the last 3 runs (SR17 - SR19), the GNO I result is [65.8 +10.2 -9.6 (stat.) +3.4 -3.6 (syst.)]SNU (1sigma) or [65.8 + 10.7 -10.2 (incl. syst.)]SNU (1sigma) with errors combined. This may be compared to the result for Gallex(I-IV), which is [77.5 +7.6 -7.8 (incl. syst.)] SNU (1sigma). A combined result from both GNOI and Gallex(I-IV) together is [74.1 + 6.7 -6.8 (incl. syst.)] SNU (1sigma)., Comment: submitted to Physics Letters B, June 2000. PACS: 26.65. +t ; 14.60 Pq. Corresponding author: till.kirsten@mpi-hd.mpg.de ; bellotti@mi.infn.it

Published
2000
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20. Gamow-Teller Strengths of the Inverse-Beta Transition 176Yb --> 176Lu for Spectroscopy of Proton-Proton and other sub-MeV Solar Neutrinos

Author

Fujiwara, M., Akimune, H., Berg, A. M. van den, Cribier, M., Daito, I., Ejiri, H., Fujimura, H., Fujita, Y., Goodman, C. D., Hara, K., Harakeh, M. N., Ihara, F., Ishikawa, T., Janecke, J., Kawabata, T., Raghavan, R. S., Schwarz, K., Tanaka, M., Yamanaka, T., Yosoi, M., and Zegers, R. G. T.

Subjects
Nuclear Experiment
Abstract

Discrete Gamow-Teller (GT) transitions, 176Yb-->176Lu at low excitation energies have been measured via the (3He,t) reaction at 450 MeV and at 0 degrees. For 176Yb, two low-lying states are observed, setting low thresholds Q(neutrino)=301 and 445 keV for neutrino capture. Capture rates estimated from the measured GT strengths, the simple two-state excitation structure, and the low Q(neutrino) in Yb--Lu indicate that Yb-based neutrino-detectors are well suited for a direct measurement of the complete sub-MeV solar electron-neutrino spectrum (including pp neutrinos) where definitive effects of flavor conversion are expected.

Published
2000
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21. White paper report on using nuclear reactors to search for a value of theta13

Author

Anderson, K., Anjos, J.C., Ayres, D., Beacom, J., Bediaga, I., de Bellefon, A., Berger, B.E., Bilenky, S., Blucher, E., Bolton, T., Buck, C., Bugg, W., Busenitz, J., Choubey, S., Conrad, J., Cribier, M., Dadoun, O., Dalnoki-Veress, F., Decowski, M., de Gouvea, Andre, Demutrh, D., Dessages-Ardellier, F., Efremenko, Y., von Feilitzsch, F., Finley, D., Formaggio, J.A., Freedman, S.J., Fujikawa, B.K., Garbini, M., Giusti, P., Goger-Neff, M., Goodman, M., Gray, F., Grieb, C., Grudzinski, J.J., Guarino, V.J., Hartmann, F., Hagner, C., Heeger, K.M., Hofmann, W., Horton-Smith, G., Huber, P., Inzhechik, L., Jochum, J., Jostlein, H., Kadel, R., Kamyshkov, Y., Kaplan, D., Kasper, P., de Kerret, H., Kersten, J., Klein, J., Knopfle, K.T., Kopeikin, V., Kozlov, Yu., Kryn, D., Kuchler, V., Kuze, M., Lachenmaier, T., Lasserre, T., Laughton, C., Lendvai, C., Li, J., Lindner, M., Link, J., Longo, M., Lu, Y.S., Luk, K.B., Ma, Y.Q., Martemyanov, V.P., Mauger, C., Manghetti, H., McKeown, R., Mention, G., Meyer, J.P., Mikaelyan, L., Minakata, H., Naples, D., Nunokawa, H., Oberauer, L., Obolensky, M., Parke, S., Petcov, S.T., Peres, O.L.G., Potzel, W., Pilcher, J., Plunkett, R., Raffelt, G., Rapidis, P., Reyna, D., Roe, B., Rolinec, M., Sakamoto, Y., Sartorelli, G., Schonert, S., Schwertz, T., Selvi, M., Shaevitz, M., Shellard, R., and Shrock, R.

Subjects
Physics of elementary particles and fields, neutrino oscillations theta13 reactor neutrino experiment Diablo Canyon Daya Bay
Published
2004

22. SOX: Short Distance Neutrino Oscillations with Borexino

Author

Agostini, M., Althenmüller, K., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Caccianiga, B., Cadonati, L., Calaprice, F., Caminata, A., Cavalcante, P., Chavarria, A., Chepurnov, A., Cribier, M., D'Angelo, D., Davini, S., Derbin, A., di Noto, L., Durero, M., Empl, A., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Göger-Neff, M., Goretti, A., Grandi, L., Gromov, M., Hagner, C., Houdy, Th., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonquères, N., Kobychev, V., Korablev, D., Korga, G., Kryn, D., Lasserre, T., Laubenstein, M., Lehnert, B., Lewke, T., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Meindl, Q., Mention, G., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Musenich, R., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Rossi, N., Saldanha, R., Salvo, C., Schönert, S., Scola, L., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Veyssière, C., Vivier, M., Vogelaar, R.B., von Feilitzsch, F., Wang, H., Winter, J., Wojcik, M., Wright, A., Wurm, M., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G., and Bravo-Berguño, D.

Published
2016
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23. GALLEX results from the first 30 solar neutrino runs

Author

Anselmann, P., primary, Hampel, W., additional, Heusser, G., additional, Kiko, J., additional, Kirsten, T., additional, Laubenstein, M., additional, Pernicka, E., additional, Pezzoni, S., additional, Rönn, U., additional, Sann, M., additional, Schlosser, C., additional, Wink, R., additional, Wojcik, M., additional, Ammon, R. v., additional, Ebert, K.H., additional, Fritsch, T., additional, Hellriegel, K., additional, Henrich, E., additional, Stieglitz, L., additional, Weirich, F., additional, Balata, M., additional, Ferrari, N., additional, Lalla, H., additional, Bellotti, E., additional, Cattadori, C., additional, Cremonesi, O., additional, Fiorini, E., additional, Zanotti, L., additional, Altmann, M., additional, Feilitzsch, F. v., additional, Mößbauer, R., additional, Schanda, U., additional, Berthomieu, G., additional, Schatzman, E., additional, Carmi, I., additional, Dostrovsky, I., additional, Bacci, C., additional, Belli, P., additional, Bernabei, R., additional, d’Angelo, S., additional, Paoluzi, L., additional, Bevilacqua, A., additional, Charbit, S., additional, Cribier, M., additional, Gösset, L., additional, Rich, J., additional, Spiro, M., additional, Stolarczyk, T., additional, Tao, C., additional, Vignaud, D., additional, Hahn, R.L., additional, Hartmann, F.X., additional, Rowley, J.K., additional, Stoenner, R.W., additional, and Weneser, J., additional

Published
2018
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24. Solar neutrinos observed by GALLEX at Gran Sasso

Author

Anselmann, P., primary, Hampel, W., additional, Heusser, G., additional, Kiko, J., additional, Kirsten, T., additional, Pernicka, E., additional, Plaga, R., additional, Rönn, U., additional, Sann, M., additional, Schlosser, C., additional, Wink, R., additional, Wójcik, M., additional, Ammon, R. von, additional, Ebert, K.H., additional, Fritsch, T., additional, Hellriegel, K., additional, Henrich, E., additional, Stieglitz, L., additional, Weyrich, F., additional, Balata, M., additional, Bellotti, E., additional, Ferrari, N., additional, Lalla, H., additional, Stolarczyk, T., additional, Cattadori, C., additional, Cremonesi, O., additional, Fiorini, E., additional, Pezzoni, S., additional, Zanotti, L., additional, Feilitzsch, F. von, additional, Mößbauer, R., additional, Schanda, U., additional, Berthomieu, G., additional, Schatzman, E., additional, Carmi, I., additional, Dostrovsky, I., additional, Bacci, C., additional, Belli, P., additional, Bernabei, R., additional, d’Angelo, S., additional, Paoluzi, L., additional, Charbit, S., additional, Cribier, M., additional, Dupont, G., additional, Gösset, L., additional, Rich, J., additional, Spiro, M., additional, Tao, C., additional, Vignaud, D., additional, Hahn, R.L., additional, Hartmann, F.X., additional, Rowley, J.K., additional, Stoenner, R.W., additional, and Weneser, J., additional

Published
2018
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25. The search for sterile neutrinos with SOX-Borexino

Author

Altenmüller, K., Agostini, M., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cavalcante, P., Chepurnov, A., Cribier, M., D’Angelo, D., Davini, S., Derbin, A., di Noto, L., Drachnev, I., Durero, M., Empl, A., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Ghiano, C., Giammarchi, M., Göger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Houdy, Th., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonqures, N., Kaiser, M., Kobychev, V., Korablev, D., Korga, G., Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Lehnert, B., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Maneschg, W., Marcocci, S., Maricic, J., Mention, G., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Pagani, L., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Roncin, R., Romani, A., Rossi, N., Schönert, S., Scola, L., Semenov, D., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Toropova, M., Unzhakov, E., Veyssière, C., Vivier, M., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., and Zuzel, G.

Published
2016
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26. Recent Borexino results and perspectives of the SOX measurement

Author

Porcelli A., Agostini M., Altenmüller K., Appel S., Atroshchenko V., Bagdasarian Z., Basilico D., Bellini G., Benziger J., Bick D., Bonfini G., Bravo D., Caccianiga B., Calaprice F., Caminata A., Caprioli S., Carlini M., Cavalcante P., Chepurnov A., Choi K., Cloué O., Cribier M., D'Angelo D., Davini S., Derbin A., Ding X.F., Di Ludovico A., Di Noto L., Drachnev I., Durero M., Farinon S., Fischer V., Fomenko K., Formozov A., Franco D., Froborg F., Gabriele F., Gaffiot J., Galbiati C., Ghiano C., Giammarchi M., Goretti A., Gromov M., Gschwender M., Hagner C., Houdy T., Hungerford E., Ianni Aldo, Ianni Andrea, Jonquères N., Jany A., Jeschke D., Kobychev V., Korablev D., Korga G., Kornoukhov V., Kryn D., Lachenmaier T., Lasserre T., Laubenstein M., Litvinovich E., Lombardi F., Lombardi P., Ludhova L., Lukyanchenko G., Lukyanchenko L., Machulin I., Manuzio G., Marcocci S., Maricic J., Mention G., Martyn J., Meroni E., Meyer M., Miramonti L., Misiaszek M., Muratova V., Musenich R., Neumair B., Oberauer L., Opitz B., Ortica F., Pallavicini M., Papp L., Pilipenko N., Pocar A., Ranucci G., Razeto A., Re A., Romani A., Roncin R., Rossi N., Rottenanger S., Schönert S., Scola M., Semenov D., Skorokhvatov M., Smirnov O., Sotnikov A., Stokes L.F.F., Suvorov Y., Tartaglia R., Testera G., Thurn J., Toropova M., Unzhakov E., Veyssiére C., Vishneva A., Vivier M., Vogelaar R.B., von Feilitzsch F., Wang H., Weinz S., Wojcik M., Wurm M., Yokley Z., Zaimidoroga O., Zavatarelli S., Zuber K., and Zuzel G.

Subjects
Physics, QC1-999
Abstract

Borexino is a liquid scintillator detector sited underground in the Laboratori Nazionali del Gran Sasso (Italy). Its physics program, until the end of this year, is focussed on the study of solar neutrinos, in particular from the Beryllium, pp, pep and CNO fusion reactions. Knowing the reaction chains in the sun provides insights towards physics disciplines such as astrophysics (star physics, star formation, etc.), astroparticle and particle physics. Phase II started in 2011 and its aim is to improve the phase I results, in particular the measurements of the neutrino fluxes from the pep and CNO processes. By the end of this year, data taking from the sun will be over and a new project is scheduled to launch: Short distance Oscillation with boreXino (SOX), which uses a Cerium source for neutrinos (100÷150 kCi of activity) and aims to confirm or rule out the presence of sterile neutrinos. This particle is hypothesised to justify the reactor, Gallium and LSND anomalies found and can reject extensions to the standard model. The work presented is a summary of the solar neutrino results achieved so far, which lead not only to a precise study of the processes in the sun, but also to more Standard Model oriented measurements (such as the stability of the charge, i.e. the life time of the electron). Furthermore, the perspectives of the SOX program are discussed showing the experiment sensitivity to a fourth neutrino state covering almost entirely 3σ of the preferred region of the anomalous neutrino experiments, and additional applications of the detector such as the study of geo-neutrinos.

Published
2018
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28. Short distance neutrino oscillations with Borexino

Author

Caminata A., Agostini M., Altenmüller K., Appel S., Bellini G., Benziger J., Berton N., Bick D., Bonfini G., Bravo D., Caccianiga B., Calaprice F., Cavalcante P., Chepurnov A., Cribier M., D'Angelo D., Davini S., Derbin A., Noto L. di, Durero M., Empl A., Etenko A., Farinon S., Fischer V., Fomenko K., Franco D., Gabriele F., Gaffiot J., Galbiati C., Ghiano C., Giammarchi M., Göger-Neff M., Goretti A., Gromov M., Hagner C., Houdy Th., Hungerford E., Ianni Aldo, Ianni Andrea, Jonquères N., Kaiser M., Kobychev V., Korablev D., Korga G., Kryn D., Lachenmaier T., Lasserre T., Laubenstein M., Lehnert B., Link J., Litvinovich E., Lombardi F., Lombardi P., Ludhova L., Lukyanchenko G., Machulin I., Maneschg W., Marcocci S., Maricic J., Mention G., Meroni E., Meyer M., Miramonti L., Misiaszek M., Montuschi M., Muratova V., Musenich R., Neumair B., Oberauer L., Obolensky M., Ortica F., Pallavicini M., Papp L., Perasso L., Pocar A., Ranucci G., Razeto A., Re A., Romani A., Rossi N., Schönert S., Scola L., Simgen H., Skorokhvatov M., Smirnov O., Sotnikov A., Sukhotin S., Suvorov Y., Tartaglia R., Testera G., Veyssière C., Vivier M., Vogelaar R.B., Feilitzsch F. von, Wang H., Winter J., Wojcik M., Wurm M., Zaimidoroga O., Zavatarelli S., Zuber K., and Zuzel G.

Subjects
Physics, QC1-999
Abstract

The Borexino detector has convincingly shown its outstanding performances in the low energy, sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection. These performances make it the ideal tool to accomplish a state-of-the-art experiment able to test unambiguously the long-standing issue of the existence of a sterile neutrino, as suggested by the several anomalous results accumulated over the past two decades, i.e. the outputs of the LSND and Miniboone experiments, the results of the source calibration of the two Gallium solar neutrino experiments, and the recently hinted reactor anomaly. The SOX project will exploit two sources, based on Chromium and Cerium, respectively, which deployed under the experiment, in a location foreseen on purpose at the time of the construction of the detector, will emit two intense beams of neutrinos (Cr) and anti-neutrinos (Ce). Interacting in the active volume of the liquid scintillator, each beam would create an unmistakable spatial wave pattern in case of oscillation of the νe (or ν̅e) into the sterile state: such a pattern would be the smoking gun proving the existence of the new sterile member of the neutrino family. Otherwise, its absence will allow setting a very stringent limit on its existence.

Published
2016
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29. Status report on theGALLEX experiment

Author

Anselmann, P., Hampel, W., Heusser, G., Kiko, J., Kirsten, T., Pernicka, E., Plaga, R., Rönn, U., Sann, M., Schlosser, C., Wink, R., Wojcik, M., Von Ammon, R., Ebert, K., Fritsch, T., Hellriegel, K., Henrich, E., Stieglitz, L., Weyrich, F., Balata, M., Bellotti, E., Ferrari, N., Lalla, H., Stolarczyk, T., Cattadori, C., Cremonesi, O., Fiorini, E., Pezzoni, S., Zanotti, L., Von Feilitzsch, F., Möβbauer, R., Schanda, U., Berthomieu, G., Schatzman, E., CaRmi, I., Dostrovsky, I., Bacci, C., Belli, P., Bernabei, R., D’Angelo, S., Paoluzi, L., Charbit, S., Cribier, M., Pont, G. Du, Gösset, L., Rich, J., Spiro, M., Tao, C., Vignaud, D., Hahn, R. L., Hartmann, F. X., Rowley, J. K., Stoenner, R. W., Weneser, J., and GALLEX Collaboration

Published
1992
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30. White paper: CeLAND - Investigation of the reactor antineutrino anomaly with an intense 144Ce-144Pr antineutrino source in KamLAND

Author

Gando, A., primary, Gando, Y., additional, Hayashida, S., additional, Ikeda, H., additional, Inoue, K., additional, Ishidoshiro, K., additional, Ishikawa, H., additional, Koga, M., additional, Matsuda, R., additional, Matsuda, S., additional, Mitsui, T., additional, Motoki, D., additional, Nakamura, K., additional, Oki, Y., additional, Otani, M., additional, Shimizu, I., additional, Shirai, J., additional, Suekane, F., additional, Suzuki, A., additional, Takemoto, Y., additional, Tamae, K., additional, Ueshima, K., additional, Watanabe, H., additional, Xu, B. D., additional, Yamada, S., additional, Yamauchi, Y., additional, Yoshida, H., additional, Banks, T., additional, Berger, B. E., additional, Cribier, M., additional, Decowski, P., additional, Detwiler, J. A., additional, Durero, M., additional, Dwyer, D., additional, Efremenko, Y., additional, Enomoto, S., additional, Fischer, V., additional, Fujikawa, B. K., additional, Gaffiot, J., additional, Gelis, V. M., additional, Karwowski, H. J., additional, Kolomensky, Y. G., additional, Kozlov, A., additional, Kornoukhov, V. N., additional, Lasserre, T., additional, Learned, J. G., additional, Letourneau, A., additional, Lhuillier, D., additional, Maricic, J., additional, Markoff, D. M., additional, Matsuno, S., additional, Mention, G., additional, Milincic, R., additional, O' Donnell, T., additional, Saldikov, I. S., additional, Scola, L., additional, Tikhomirov, G. V., additional, Veyssiere, C., additional, Vivier, M., additional, and Yoshida, S., additional

Published
2013
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31. GALLEX results from the first 30 solar neutrino runs

Author

Gallex, C, Anselmann, P, Hampel, W, Heusser, G, Kiko, J, Kirsten, T, Laubenstein, M, Pernicka, E, Pezzoni, S, Rönn, U, Sann, M, Schlosser, C, Wink, R, Wojcik, M, Ammon, R, Ebert, K, Fritsch, T, Hellriegel, K, Henrich, E, Stieglitz, L, Weirich, F, Balata, M, Ferrari, N, Lalla, H, Bellotti, E, Cattadori, C, Cremonesi, O, Fiorini, E, Zanotti, L, Altmann, M, Feilitzsch, F, Mößbauer, R, Schanda, U, Berthomieu, G, Schatzman, E, Carmi, I, Dostrovsky, I, Bacci, C, Belli, P, Bernabei, R, D'Angelo, S, Paoluzi, L, Bevilacqua, A, Charbit, S, Cribier, M, Gosset, L, Rich, J, Spiro, M, Stolarczyk, T, Tao, C, Vignaud, D, Hahn, R, Hartmann, F, Rowley, J, Stoenner, R, Weneser, J, Max Planck Institute for Nuclear Physics (MPIK), Max-Planck-Gesellschaft, 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), Lantz, Simone, Tran Thanh Van J., Physique Corpusculaire et Cosmologie - Collège de France (PCC), and 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)

Subjects
Nuclear and High Energy Physics, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], Solar neutrino, 01 natural sciences, UNCERTAINTIES, Settore FIS/04 - Fisica Nucleare e Subnucleare, PHYSICS, Nuclear physics, Resonance oscillation, 0103 physical sciences, OSCILLATIONS, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Combined result, 010306 general physics, Neutrino oscillation, [SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces, environment, DETECTOR, ComputingMilieux_MISCELLANEOUS, Physics, [SDU.OCEAN]Sciences of the Universe [physics]/Ocean, Atmosphere, 010308 nuclear & particles physics, Settore FIS/01 - Fisica Sperimentale, SUN, MODEL, Exposure period, Neutrino, GALLEX, MATTER
Abstract

We report new GALLEX solar neutrino results from 15 runs covering 406 days (live time) within the exposure period 19 August 1992–13 October 1993 (“GALLEX II”). With counting data considered until 4 January 1994, the new result is [78±13 (stat.) ±5 (stat.)] SNU (1σ). It confirms our previous result for the 15 initial runs (“GALLEX I”) of [81±17( stat .)±9( syst .)] SNU. After two years of recording the solar neutrino flux with the GALLEX detector the combined result from 30 solar runs (GALLEX I + GALLEX II) is [79±10( stat .)±6( syst .)] SNU (1 σ ). In addition, 19 “blank” runs gave the expected null result. GALLEX neutrino experiments are continuing.

Published
2018

35. The Ce-144 source for SOX

Author

Durero, M., Vivier, M., Agostini, M., Altenmueller, K., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cavalcante, P., Chepurnov, A., Choi, K., Cribier, M., D'Angelo, D., Davini, S., Derbin, A., Di Noto, L., Drachnev, I., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gabriele, F., Gafflot, J., Galbiati, C., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Houdy, T., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonqueres, N., Jedrzejczak, K., Kaisers, M., Kobychev, V., Korablev, D., Korga, G., Kornoukhov, Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Lehnert, B., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Mention, G., Meroni, E., Meyers, M., Miramonti, L., Misiaszek, M., Montuschi, M., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Roncin, R., Rossi, N., Schoenert, S., Scola, L., Semenov, D., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Veyssiere, C., Unzhakov, E., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Weinz, S., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G., Durero, M., Vivier, M., Agostini, M., Altenmueller, K., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cavalcante, P., Chepurnov, A., Choi, K., Cribier, M., D'Angelo, D., Davini, S., Derbin, A., Di Noto, L., Drachnev, I., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gabriele, F., Gafflot, J., Galbiati, C., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Houdy, T., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonqueres, N., Jedrzejczak, K., Kaisers, M., Kobychev, V., Korablev, D., Korga, G., Kornoukhov, Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Lehnert, B., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Mention, G., Meroni, E., Meyers, M., Miramonti, L., Misiaszek, M., Montuschi, M., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Roncin, R., Rossi, N., Schoenert, S., Scola, L., Semenov, D., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Veyssiere, C., Unzhakov, E., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Weinz, S., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., and Zuzel, G.

Abstract

The SOX (Short distance neutrino Oscillations with BoreXino) project aims at testing the light sterile neutrino hypothesis. To do so, two artificials sources of antineutrinos and neutrinos respectively will be consecutively deployed at the Laboratori Nazionali del Gran Sasso (LNGS) in close vicinity to Borexino, a large liquid scintillator detector. This document reports on the 0, source production and transportation. The source should exhibit a long lifetime and a high decay energy, a requirement fullfilled by the Ce-144-Pr-144 pair at secular equilibrium. It will be produced at FSUE "Mayak" PA using spent nuclear fuel. It will then be shielded and packed according to international regulation and shipped to LNGS across Europe. Knowledge of the Cerium antineutrino generator (CeANG) parameters is crucial for SOX as it can strongly impact the experiment sensitivity. Several apparatuses are being used or designed to characterize CeANG activity, radioactive emission and content. An overview of the measurements performed so far is presented here.

Published
2016

36. Incineration of 241Am induced by thermal neutrons

Author

Fioni, G., Cribier, M., Marie, F., Aubert, M., Ayrault, S., Bolognese, T., Cavedon, J.-M., Chartier, F., Deruelle, O., Doneddu, F., Faust, H., Gaudry, A., Gunsing, F., Leconte, Ph., Lelievre, F., Martino, J., Oliver, R., Pluquet, A., Röttger, S., Spiro, M., and Veyssiere, C.

Published
2001
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37. CeSOX: An experimental test of the sterile neutrino hypothesis with Borexinoo

Author

Gromov, M., Agostini, M., Altenmüller, K., Appel, S., Atroshchenko, V., Bagdasarian, Z., Basilico, D., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Caprioli, S., Carlini, M., Cavalcante, P., Chepurnov, A., Choi, K., Cloué, O., Collica, L., Cribier, M., D’Angelo, D., Davini, S., Derbin, A., Ding, X. F., Di Ludovico, A., Di Noto, L., Drachnev, I., Durero, M., Farinon, S., Fischer, V., Fomenko, K., Formozov, A., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Gschwender, M., Ghiano, C., Giammarchi, M., Goretti, A., Guffanti, D., Hagner, C., Houdy, T., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonquères, N., Jany, A., Jeschke, D., Kobychev, V., Korablev, D., Korga, G., Kornoukhov, V., Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Lukyanchenko, L., Machulin, I., Manuzio, G., Marcocci, S., Maricic, J., Mention, G., Martyn, J., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Opitz, B., Orekhov, V., Ortica, F., Pallavicini, M., Papp, L., Penek, Ö, Pilipenko, N., Pocar, A., Porcelli, A., Ranucci, G., Razeto, A., Re, A., Redchuk, M., Romani, A., Roncin, R., Rossi, N., Rottenanger, S., Schönert, S., Scola, L., Semenov, D., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Stokes, L. F. F., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Trantel, A., Unzhakov, E., Veyssiére, C., Vishneva, A., Vivier, M., Vogelaar, R. B., Von Feilitzsch, F., Wang, H., Weinz, S., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., and Zuzel, G.

Abstract

3rd International Conference on Particle Physics and Astrophysics, ICPPA 2017, Moscow, Russia, 2 Oct 2017 - 5 Oct 2017; Journal of physics / Conference Series 934, 012003 - (2017). doi:10.1088/1742-6596/934/1/012003, Published by IOP Publ., Bristol

Published
2017
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38. Search for sterile neutrinos with the SOX experiment

Author

Caminata, A., Agostini, M., Altenmueller, K., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Cavalcante, P., Chepurnov, A., Choi, K., Cribier, M., D'Angelo, D., Davini, S., Derbin, A., Di Noto, L., Drachnev, I., Durero, M., Empl, A., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Houdy, Th., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonqueres, N., Jedrzejczak, K., Kaiser, M., Kobychev, V., Korablev, D., Korga, G., Kornoukhov, V., Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Lehnert, B., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Mention, G., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pagani, L., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Roncin, R., Rossi, N., Schoenert, S., Scola, L., Semenov, D., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Unzhakov, E., Veyssiere, C., Vivier, M., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Weinz, S., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, 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), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), 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), 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), Caminata, A., Agostini, M., Altenmueller, K., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Cavalcante, P., Chepurnov, A., Choi, K., Cribier, M., D'Angelo, D., Davini, S., Derbin, A., Di Noto, L., Drachnev, I., Durero, M., Empl, A., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Houdy, Th., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonqueres, N., Jedrzejczak, K., Kaiser, M., Kobychev, V., Korablev, D., Korga, G., Kornoukhov, V., Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Lehnert, B., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Mention, G., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pagani, L., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Roncin, R., Rossi, N., Schoenert, S., Scola, L., Semenov, D., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Unzhakov, E., Veyssiere, C., Vivier, M., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Weinz, S., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., and Zuzel, G.

Subjects
neutrino: sterile: search for, Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, High Energy Physics::Phenomenology, Astronomy and Astrophysics, Physics::Geophysics, Gran Sasso, talk: Rome 2015/04/08, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], High Energy Physics::Experiment, Borexino, neutrino: oscillation, experimental results
Abstract

International audience; In the recent years, the Borexino detector has proven its outstanding performances in detecting neutrinos and antineutrinos in the low energy regime. Consequently, it is an ideal tool to investigate the existence of sterile neutrinos, whose presence has been suggested by several anomalies over the past two decades. The SOX (Short distance neutrino Oscillations with boreXino) project will investigate the presence of sterile neutrinos placing a neutrino and an antineutrino sources in a location under the detector foreseen for this purpose since the construction of Borexino. Interacting in the detector active volume, each beam would create a well detectable spatial wave pattern in case of oscillation of neutrino or antineutrino in a sterile state. Otherwise, the experiment will set a very stringent limit on the existence of a sterile state.

Published
2015

39. The SOX experiment in the neutrino physics

Author

Di Noto, L., Agostini, M., Althenmüller, K., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo-Berguño, D., Caccianiga, B., Cadonati, L., Calaprice, F., Caminata, A., Cavalcante, P., Chavarria, A., Chepurnov, A., Cribier, M., D'Angelo, D., Davini, S., Derbin, A., Durero, M., Empl, A., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gaffiot, F., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Göger-Neff, M., Goretti, A., Grandi, L., Gromov, M., Hagner, C., Houdy, Th., Hungerford, E., Ianni, Al., Ianni, An., Jonquères, N., Kobychev, V., Korablev, D., Korga, G., Kryn, D., Lasserre, T., Laubenstein, M., Lehnert, T., Lewke, T., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Meindl, Q., Mention, G., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, Marcin, Montuschi, M., Mosteiro, P., Musenich, R., Muratova, V., 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., Saldanha, R., Salvo, C., Schönert, S., Scola, L., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Veyssière, C., Vivier, M., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Winter, J., Wójcik, Marcin, Wright, A., Wurm, M., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, Grzegorz, Gabriele, J., Di Noto, L., Agostini, M., Althenmueller, K., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo-Berguno, D., Caccianiga, B., Cadonati, L., Calaprice, F., Caminata, A., Cavalcante, P., Chavarria, A., Chepurnov, A., Cribier, M., Dangelo, D., Davini, S., Derbin, A., Durero, M., Empl, A., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Grandi, L., Gromov, M., Hagner, C., Houdy, Th., Hungerford, E., Ianni, Al., Ianni, An., Jonqueres, N., Kobychev, V., Korablev, D., Korga, G., Kryn, D., Lasserre, T., Laubenstein, M., Lehnert, T., Lewke, T., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Meindl, Q., Mention, G., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Musenich, R., Muratova, V., 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., Saldanha, R., Salvo, C., Schoenert, S., Scola, L., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Veyssiere, C., Vivier, M., Vogelaar, R. B., Von Feilitzsch, F., Wang, H., Winter, J., Wojcik, M., Wright, A., Wurm, M., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G., Dipartimento di Fisica, Università di Genova e Sezione INFN, Department de Física, Universitat de les Illes Balears, Dipartimento di Fisica, Universita degli Studi e INFN, Chemical Engineering Department, Princeton University, Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Institut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), INFN Laboratori Nazionali del Gran Sasso, Physics Department, Virginia Polytechnic Institute and State University, Physics Department, University of Massachusetts, Physics Department, Princeton University, Lomonosov Moscow State University Skobeltsyn Institute of Nuclear Physics, 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), Department of Physics, University of Houston, StPetersburg Nuclear Physics Institute, Kurchatov Institute, Joint Institute for Nuclear Research (JINR), Bureau de Conception Calculs et Réalisations (BCCR), Service d'Etudes Mécaniques et Thermiques (SEMT), Département de Modélisation des Systèmes et Structures (DM2S), CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département de Modélisation des Systèmes et Structures (DM2S), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Kiev Institute for Nuclear Research, Max-Planck-Institut fur Kernphysik, Gran Sasso Science Institute, INFN, Department of Physics and Astronomy, University of Hawaii, M. Smoluchowski Institute of Physics, Jagellonian University, Dipartimento di Chimica, Biologia e Biotecnologie, Universita degli Studi e INFN, Physics and Astronomy Department, University of California Los Angeles, Los Angeles, Institut für Physik und Astronomie, Universität Potsdam, and Department of Physics, Technische Universitat Dresden

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; SOX (Short distance neutrino Oscillations with BoreXino) is a new experiment that takes place at the Laboratori Nazionali del Gran Sasso (LNGS) and it exploits the Borexino detector to study the neutrino oscillations at short distance. In different phases, by using two artificial sources 51Cr and 144Ce-144Pr, neutrino and antineutrino fluxes of measured intensity will be detected by Borexino in order to observe possible neutrino oscillations in the sterile state. In this paper an overview of the experiment is given and one of the two calorimeters that will be used to measure the source activity is described. At the end the expected sensitivity to determine the neutrino sterile mass is shown.

Published
2015

40. CeSOX: An experimental test of the sterile neutrino hypothesis with Borexino

Author

Gromov, M, primary, Agostini, M, additional, Altenmüller, K, additional, Appel, S, additional, Atroshchenko, V, additional, Bagdasarian, Z, additional, Basilico, D, additional, Bellini, G, additional, Benziger, J, additional, Bick, D, additional, Bonfini, G, additional, Bravo, D, additional, Caccianiga, B, additional, Calaprice, F, additional, Caminata, A, additional, Caprioli, S, additional, Carlini, M, additional, Cavalcante, P, additional, Chepurnov, A, additional, Choi, K, additional, Cloué, O, additional, Collica, L, additional, Cribier, M, additional, D’Angelo, D, additional, Davini, S, additional, Derbin, A, additional, Ding, X F, additional, Di Ludovico, A, additional, Di Noto, L, additional, Drachnev, I, additional, Durero, M, additional, Farinon, S, additional, Fischer, V, additional, Fomenko, K, additional, Formozov, A, additional, Franco, D, additional, Gabriele, F, additional, Gaffiot, J, additional, Galbiati, C, additional, Gschwender, M, additional, Ghiano, C, additional, Giammarchi, M, additional, Goretti, A, additional, Guffanti, D, additional, Hagner, C, additional, Houdy, T, additional, Hungerford, E, additional, Ianni, Aldo, additional, Ianni, Andrea, additional, Jonquères, N, additional, Jany, A, additional, Jeschke, D, additional, Kobychev, V, additional, Korablev, D, additional, Korga, G, additional, Kornoukhov, V, additional, Kryn, D, additional, Lachenmaier, T, additional, Lasserre, T, additional, Laubenstein, M, additional, Litvinovich, E, additional, Lombardi, F, additional, Lombardi, P, additional, Ludhova, L, additional, Lukyanchenko, G, additional, Lukyanchenko, L, additional, Machulin, I, additional, Manuzio, G, additional, Marcocci, S, additional, Maricic, J, additional, Mention, G, additional, Martyn, J, additional, Meroni, E, additional, Meyer, M, additional, Miramonti, L, additional, Misiaszek, M, additional, Muratova, V, additional, Musenich, R, additional, Neumair, B, additional, Oberauer, L, additional, Opitz, B, additional, Orekhov, V, additional, Ortica, F, additional, Pallavicini, M, additional, Papp, L, additional, Penek, Ö, additional, Pilipenko, N, additional, Pocar, A, additional, Porcelli, A, additional, Ranucci, G, additional, Razeto, A, additional, Re, A, additional, Redchuk, M, additional, Romani, A, additional, Roncin, R, additional, Rossi, N, additional, Rottenanger, S, additional, Schönert, S, additional, Scola, L, additional, Semenov, D, additional, Skorokhvatov, M, additional, Smirnov, O, additional, Sotnikov, A, additional, Stokes, L F F, additional, Suvorov, Y, additional, Tartaglia, R, additional, Testera, G, additional, Thurn, J, additional, Toropova, M, additional, Trantel, A, additional, Unzhakov, E, additional, Veyssiére, C, additional, Vishneva, A, additional, Vivier, M, additional, Vogelaar, R B, additional, von Feilitzsch, F, additional, Wang, H, additional, Weinz, S, additional, Wojcik, M, additional, Wurm, M, additional, Yokley, Z, additional, Zaimidoroga, O, additional, Zavatarelli, S, additional, Zuber, K, additional, and Zuzel, G, additional

Published
2017
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41. White paper report on using nuclear reactors to search for a value of theta13

Author

Anderson, K., primary, Anjos, J.C., additional, Ayres, D., additional, Beacom, J., additional, Bediaga, I., additional, de Bellefon, A., additional, Berger, B.E., additional, Bilenky, S., additional, Blucher, E., additional, Bolton, T., additional, Buck, C., additional, Bugg, W., additional, Busenitz, J., additional, Choubey, S., additional, Conrad, J., additional, Cribier, M., additional, Dadoun, O., additional, Dalnoki-Veress, F., additional, Decowski, M., additional, de Gouvea, Andre, additional, Demutrh, D., additional, Dessages-Ardellier, F., additional, Efremenko, Y., additional, von Feilitzsch, F., additional, Finley, D., additional, Formaggio, J.A., additional, Freedman, S.J., additional, Fujikawa, B.K., additional, Garbini, M., additional, Giusti, P., additional, Goger-Neff, M., additional, Goodman, M., additional, Gray, F., additional, Grieb, C., additional, Grudzinski, J.J., additional, Guarino, V.J., additional, Hartmann, F., additional, Hagner, C., additional, Heeger, K.M., additional, Hofmann, W., additional, Horton-Smith, G., additional, Huber, P., additional, Inzhechik, L., additional, Jochum, J., additional, Jostlein, H., additional, Kadel, R., additional, Kamyshkov, Y., additional, Kaplan, D., additional, Kasper, P., additional, de Kerret, H., additional, Kersten, J., additional, Klein, J., additional, Knopfle, K.T., additional, Kopeikin, V., additional, Kozlov, Yu., additional, Kryn, D., additional, Kuchler, V., additional, Kuze, M., additional, Lachenmaier, T., additional, Lasserre, T., additional, Laughton, C., additional, Lendvai, C., additional, Li, J., additional, Lindner, M., additional, Link, J., additional, Longo, M., additional, Lu, Y.S., additional, Luk, K.B., additional, Ma, Y.Q., additional, Martemyanov, V.P., additional, Mauger, C., additional, Manghetti, H., additional, McKeown, R., additional, Mention, G., additional, Meyer, J.P., additional, Mikaelyan, L., additional, Minakata, H., additional, Naples, D., additional, Nunokawa, H., additional, Oberauer, L., additional, Obolensky, M., additional, Parke, S., additional, Petcov, S.T., additional, Peres, O.L.G., additional, Potzel, W., additional, Pilcher, J., additional, Plunkett, R., additional, Raffelt, G., additional, Rapidis, P., additional, Reyna, D., additional, Roe, B., additional, Rolinec, M., additional, Sakamoto, Y., additional, Sartorelli, G., additional, Schonert, S., additional, Schwertz, T., additional, Selvi, M., additional, Shaevitz, M., additional, Shellard, R., additional, Shrock, R., additional, Sidwell, R., additional, Sims, J., additional, Sinev, V., additional, Stanton, N., additional, Stancu, I., additional, Stefanski, R., additional, Seukane, F., additional, Sugiyama, H., additional, Sukhotin, S., additional, Sumiyoshi, T., additional, Svoboda, R., additional, Talaga, R., additional, Tamura, N., additional, Tanimoto, M., additional, Thron, J., additional, von Toerne, E., additional, Vignaud, D., additional, Wagner, C., additional, Wang, Y.F., additional, Wang, Z., additional, Winter, W., additional, Wong, H., additional, Yakushev, E., additional, Yang, C.G., additional, and Yasuda, O., additional

Published
2004
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42. GALLEX solar neutrino observations: results for GALLEX IV

Author

Hampel, W., Handt, J., Heusser, G., Kiko, J., Kirsten, T., Laubenstein, M., Pernicka, E., Rau, W., Wojcik, M., Zakharov, Y., Ammon, R.v., Ebert, K.H., Fritsch, T., Heidt, D., Henrich, E., Stielglitz, L., Weirich, F., Balata, M., Sann, M., Hartmann, F.X., Bellotti, E., Cattadori, C., Cremonesi, O., Ferrari, N., Fiorini, E., Zanotti, L., Altmann, M., Feilitzsch, F.v., Mößbauer, R., Wänninger, S., Berthomieu, G., Schatzman, E., Carmi, I., Dostrovsky, I., Bacci, C., Belli, P., Bernabei, R., d'Angelo, S., Paoluzi, L., Cribier, M., Rich, J., Spiro, M., Tao, C., Vignaud, D., Boger, J., Hahn, R.L., Rowley, J.K., Stoenner, R.W., and Weneser, J.

Published
1999
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43. Monte Carlo simulations in neutrino physics: the example of the SOX experiment

Author

Caminata, A., Agostini, M., Altenmüller, K., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, Daniel, Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Carlini, M., Cavalcante, P., Chepurnov, A., Choi, K., Cribier, M., D'Angelo, D., Davini, S., Derbin, A., Noto, L. Di, Drachnev, I., Durero, M., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Formozov, A., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, Caren, Houdy, Th., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonqueres, N., Jedrzejczak, K., Jeschke, D., Kaiser, M., Kobychev, V., Korablev, D., Korga, G., Kornoukhov, V., Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Lehnert, B., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Mention, G., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, Adelia, Re, A., Romani, A., Roncin, R., Rossi, N., Schönert, S., Scola, L., Semenov, D., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Veyssiere, C., Vivier, M., Unzhakov, E., Vogelaar, R. B., Feilitzsch, F. Von, Wang, H., Weinz, S., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G., Suvorov, Y., Département de Physique Nucléaire (ex SPhN) (DPHN), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, 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), 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)-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)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)

Subjects
Physics::Instrumentation and Detectors, High Energy Physics::Phenomenology, scintillation counter: liquid, anomaly, neutrino: sterile, antineutrino, 7. Clean energy, electroweak interaction: model, neutrino: detector, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], High Energy Physics::Experiment, Borexino, [INFO]Computer Science [cs], talk: Hamburg 2016/03/17, numerical calculations: Monte Carlo
Abstract

Caminata, A. "Monte Carlo simulations in neutrino physics: the example of the SOX experiment" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg Magellan Workshop, Hamburg, Germany, 17 Mar 2016 - 18 Mar 2016 ; DESY-PROC 105-112(2016). doi:10.3204/DESY-PROC-2016-05/21, The SOX project aims to test the existence of light sterile neutrinos. A solid signal would mean the discovery of the first particles beyond the Standard Electroweak Model and would have profound implications in our understanding of the Universe and of fundamental particle physics. In case of a negative result, it is able to close a long standing debate about the reality of the neutrino anomalies. The SOX experiment will use a \mbox{$^{144}$Ce-$^{144}$Pr} antineutrino generator placed at short distance from the Borexino liquid scintillator detector. Particular emphasis is devoted in describing how a simulation of a neutrino detector is implemented and how it can be used to obtain useful information for the future data analysis., Published by Deutsches Elektronen-Synchrotron, DESY, Hamburg

Published
2016

44. The SOX experiment: understanding the detector behavior using calibration sources

Author

Caminata, A., Agostini, M., Altenmüller, K., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, Daniel, Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Carlini, M., Cavalcante, P., Chepurnov, A., Choi, K., Cribier, M., D'Angelo, D., Davini, S., Derbin, A., Di Noto, L., Drachnev, I., Durero, M., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Formozov, A., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, Caren, Houdy, Th., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonqueres, N., Jedrzejczak, K., Jeschke, D., Kaiser, Markus, Kobychev, V., Korablev, D., Korga, G., Kornoukhov, V., Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Lehnert, B., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Mention, G., Meroni, E., Meyer, Mikko, Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Roncin, R., Rossi, N., Schönert, S., Scola, L., Semenov, D., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Tartaglia, R., Testera, G., Thurn, J., Toropova, M., Veyssiere, C., Vivier, M., Unzhakov, E., Vogelaar, R. B., Vo Feilitzsch, F., Wang, H., Weinz, S., Winter, J., Wojcik, M., Wurm, M., Yokley, Z., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G., Suvorov, Y., Département de Physique Nucléaire (ex SPhN) (DPHN), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, 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), 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 Paris Cité (UPCité), 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, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)

Subjects
Physics::Instrumentation and Detectors, measurement methods, scintillation counter: liquid, High Energy Physics::Experiment, Borexino, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], neutrino: sterile, antineutrino: particle source, calibration, Computer Science::Computers and Society
Abstract

Caminata, A. "The SOX experiment: understanding the detector behavior using calibration sources" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg Magellan Workshop, Hamburg, Germany, 17 Mar 2016 - 18 Mar 2016 ; DESY-PROC 175-180(2016). doi:10.3204/DESY-PROC-2016-05/22, The SOX experiment investigates the existence of light sterile neutrinos. A solid signal would mean the discovery of the first particles beyond the Standard Electroweak Model and would have profound implications in our understanding of the Universe and of fundamental particle physics. In case of a negative result, it is able to close a long standing debate about the reality of the neutrino anomalies. The SOX experiment will use a $^{144}Ce-^{144}Pr$ antineutrino generator placed 8.5~m below the Borexino liquid scintillator detector. In view of the SOX experiment, a precise knowledge of the energy response and the spatial reconstruction of the antineutrino events is very important. Consequently, a calibration campaign of the Borexino detector is foreseen before the beginning of the SOX data taking. This paper briefly reviews the techniques used for calibrate the Borexino detector., Published by Verlag Deutsches Elektronen-Synchrotron, Hamburg

Published
2016

45. Improvements in the simulation code of the SOX experiment

Author

Caminata, A., primary, Agostini, M., additional, Altenmüeller, K., additional, Appel, S., additional, Atroshchenko, V., additional, Bellini, G., additional, Benziger, J., additional, Bick, D., additional, Bonfini, G., additional, Bravo, D., additional, Caccianiga, B., additional, Calaprice, F., additional, Carlini, M., additional, Cavalcante, P., additional, Chepurnov, A., additional, Choi, K., additional, Cribier, M., additional, D’Angelo, D., additional, Davini, S., additional, Derbin, A., additional, Noto, L. Di, additional, Drachnev, I., additional, Durero, M., additional, Etenko, A., additional, Farinon, S., additional, Fischer, V., additional, Fomenko, K., additional, Franco, D., additional, Gabriele, F., additional, Gaffiot, J., additional, Galbiati, C., additional, Gschwender, M., additional, Ghiano, C., additional, Giammarchi, M., additional, Goeger-Neff, M., additional, Goretti, A., additional, Gromov, M., additional, Hagner, C., additional, Houdy, Th., additional, Hungerford, E., additional, Ianni, Aldo, additional, Ianni, Andrea, additional, Jonquères, N., additional, Jany, A., additional, Jedrzejczak, K., additional, Jeschke, D., additional, Kobychev, V., additional, Korablev, D., additional, Korga, G., additional, Kornoukhov, V., additional, Kryn, D., additional, Lachenmaier, T., additional, Lasserre, T., additional, Laubenstein, M., additional, Lehnert, B., additional, Link, J., additional, Litvinovich, E., additional, Lombardi, F., additional, Lombardi, P., additional, Ludhova, L., additional, Lukyanchenko, G., additional, Machulin, I., additional, Manecki, S., additional, Maneschg, W., additional, Manuzio, G., additional, Marcocci, S., additional, Maricic, J., additional, Mention, G., additional, Meroni, E., additional, Meyer, M., additional, Miramonti, L., additional, Misiaszek, M., additional, Montuschi, M., additional, Mosteiro, P., additional, Muratova, V., additional, Musenich, R., additional, Neumair, B., additional, Oberauer, L., additional, Obolensky, M., additional, Ortica, F., additional, Pallavicini, M., additional, Papp, L., additional, Pocar, A., additional, Ranucci, G., additional, Razeto, A., additional, Re, A., additional, Romani, A., additional, Roncin, R., additional, Rossi, N., additional, Schönert, S., additional, Scola, L., additional, Semenov, D., additional, Skorokhvatov, M., additional, Smirnov, O., additional, Sotnikov, A., additional, Sukhotin, S., additional, Suvorov, Y., additional, Tartaglia, R., additional, Testera, G., additional, Thurn, J., additional, Toropova, M., additional, Unzhakov, E., additional, Veyssiére, C., additional, Vishneva, A., additional, Vivier, M., additional, Vogelaar, R.B., additional, von Feilitzsch, F., additional, Wang, H., additional, Weinz, S., additional, Winter, J., additional, Wojcik, M., additional, Wurm, M., additional, Yokley, Z., additional, Zaimidoroga, O., additional, Zavatarelli, S., additional, Zuber, K., additional, and Zuzel, G., additional

Published
2017
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46. Search for Sterile Neutrinos with the Borexino Detector

Author

Agostini, M., Altenmüller, K., Appel, S., Bellini, G., Benziger, J., Berton, N., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Cadonati, L., Calaprice, F., Caminata, A., Cavalcante, P., Chavarria, A., Chepurnov, A., Cribier, M., D’Angelo, D., Davini, S., Derbin, A., di Noto, L., Durero, M., Empl, A., Etenko, A., Farinon, S., Fischer, V., Fomenko, K., Franco, D., Gabriele, F., Gaffiot, J., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goger-Neff, M., Goretti, A., Grandi, L., Gromov, M., Hagner, C., Houdy, Th., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Jonquères, N., Kaiser, M., Kobychev, V., Korablev, D., Korga, G., Kryn, D., Lachenmaier, T., Lasserre, T., Laubenstein, M., Lehnert, B., Lewke, T., Link, J., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Maricic, J., Meindl, Q., Mention, G., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, Marcin, Montuschi, M., Mosteiro, P., Muratova, V., Musenich, R., Neumair, B., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Rossi, N., Saldanha, R., Salvo, C., Schonert, S., Scola, L., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Veyssiere, C., Vignaud, D., Vivier, M., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Winter, J., Wójcik, Marcin, Wright, A., Wurm, M., Zaimidoroga, O., Zavatarelli, S., Zuber, K., and Zuzel, Grzegorz

Subjects
Physics::Instrumentation and Detectors, background, Astrophysics::High Energy Astrophysical Phenomena, Physics, High Energy Physics::Phenomenology, oscillation [neutrino], Weinberg angle, anomaly, mass difference [neutrino], sterile: search for [neutrino], low [energy], mixing angle [electroweak interaction], High Energy Physics::Experiment, Borexino, magnetic moment [neutrino], Hamburg 2014/08/24 [talk], experimental results
Abstract

Contribution to Proceedings, Proc. of PANIC 2014, 317 - 320; DESY-PROC-2014-02; ISSN 1435-8077

Published
2014
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47. GNO solar neutrino observations: results for GNO I

Author

GNO Collaboration, Altmann, M., Balata, M., Belli, P., Bellotti, E., Bernabei, R., Burkert, E., Cattadori, C., Cerichelli, G., Chiarini, M., Cribier, M., d'Angelo, S., Del Re, G., Ebert, K. H., Feilitzsch, F. v., Ferrari, N., Hampel, W., Handt, J., Henrich, E., Heusser, G., Kiko, J., Kirsten, T., Lachenmaier, T., Lanfranchi, J., Laubenstein, M., Motta, D., Rau, W., Richter, H., Waenninger, S., Wojcik, M., and Zanotti, L.

Subjects
Physics, GALLEX, Nuclear and High Energy Physics, Particle physics, Solar neutrino, Astrophysics (astro-ph), Solar neutrinos, Settore FIS/01 - Fisica Sperimentale, FOS: Physical sciences, Astrophysics, Settore FIS/04 - Fisica Nucleare e Subnucleare, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Neutrino mass, Gallium experiment, Combined result, GNO
Abstract

We report the first GNO solar neutrino results for the measuring period GNOI, solar exposure time May 20, 1998 till January 12, 2000. In the present analysis, counting results for solar runs SR1 - SR19 were used till April 4, 2000. With counting completed for all but the last 3 runs (SR17 - SR19), the GNO I result is [65.8 +10.2 -9.6 (stat.) +3.4 -3.6 (syst.)]SNU (1sigma) or [65.8 + 10.7 -10.2 (incl. syst.)]SNU (1sigma) with errors combined. This may be compared to the result for Gallex(I-IV), which is [77.5 +7.6 -7.8 (incl. syst.)] SNU (1sigma). A combined result from both GNOI and Gallex(I-IV) together is [74.1 + 6.7 -6.8 (incl. syst.)] SNU (1sigma)., submitted to Physics Letters B, June 2000. PACS: 26.65. +t ; 14.60 Pq. Corresponding author: till.kirsten@mpi-hd.mpg.de ; bellotti@mi.infn.it

Published
2000

48. SOX: Short Distance Neutrino Oscillations with Borexino

Author

Bravo-Berguño, D., primary, Agostini, M., additional, Althenmüller, K., additional, Bellini, G., additional, Benziger, J., additional, Berton, N., additional, Bick, D., additional, Bonfini, G., additional, Caccianiga, B., additional, Cadonati, L., additional, Calaprice, F., additional, Caminata, A., additional, Cavalcante, P., additional, Chavarria, A., additional, Chepurnov, A., additional, Cribier, M., additional, D'Angelo, D., additional, Davini, S., additional, Derbin, A., additional, di Noto, L., additional, Durero, M., additional, Empl, A., additional, Etenko, A., additional, Farinon, S., additional, Fischer, V., additional, Fomenko, K., additional, Franco, D., additional, Gabriele, F., additional, Gaffiot, J., additional, Galbiati, C., additional, Gazzana, S., additional, Ghiano, C., additional, Giammarchi, M., additional, Göger-Neff, M., additional, Goretti, A., additional, Grandi, L., additional, Gromov, M., additional, Hagner, C., additional, Houdy, Th., additional, Hungerford, E., additional, Ianni, Aldo, additional, Ianni, Andrea, additional, Jonquères, N., additional, Kobychev, V., additional, Korablev, D., additional, Korga, G., additional, Kryn, D., additional, Lasserre, T., additional, Laubenstein, M., additional, Lehnert, B., additional, Lewke, T., additional, Link, J., additional, Litvinovich, E., additional, Lombardi, F., additional, Lombardi, P., additional, Ludhova, L., additional, Lukyanchenko, G., additional, Machulin, I., additional, Manecki, S., additional, Maneschg, W., additional, Marcocci, S., additional, Maricic, J., additional, Meindl, Q., additional, Mention, G., additional, Meroni, E., additional, Meyer, M., additional, Miramonti, L., additional, Misiaszek, M., additional, Montuschi, M., additional, Mosteiro, P., additional, Muratova, V., additional, Musenich, R., additional, Oberauer, L., additional, Obolensky, M., additional, Ortica, F., additional, Otis, K., additional, Pallavicini, M., additional, Papp, L., additional, Perasso, L., additional, Pocar, A., additional, Ranucci, G., additional, Razeto, A., additional, Re, A., additional, Romani, A., additional, Rossi, N., additional, Saldanha, R., additional, Salvo, C., additional, Schönert, S., additional, Scola, L., additional, Simgen, H., additional, Skorokhvatov, M., additional, Smirnov, O., additional, Sotnikov, A., additional, Sukhotin, S., additional, Suvorov, Y., additional, Tartaglia, R., additional, Testera, G., additional, Veyssière, C., additional, Vivier, M., additional, Vogelaar, R.B., additional, von Feilitzsch, F., additional, Wang, H., additional, Winter, J., additional, Wojcik, M., additional, Wright, A., additional, Wurm, M., additional, Zaimidoroga, O., additional, Zavatarelli, S., additional, Zuber, K., additional, and Zuzel, G., additional

Published
2016
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49. Understanding the detector behavior through Montecarlo and calibration studies in view of the SOX measurement

Author

Caminata, A, primary, Agostini, M, additional, Altenmüller, K, additional, Appel, S, additional, Bellini, G, additional, Benziger, J, additional, Berton, N, additional, Bick, D, additional, Bonfini, G, additional, Bravo, D, additional, Caccianiga, B, additional, Calaprice, F, additional, Cavalcante, P, additional, Chepurnov, A, additional, Choi, K, additional, Cribier, M, additional, D'Angelo, D, additional, Davini, S, additional, Derbin, A, additional, Noto, L Di, additional, Drachnev, I, additional, Durero, M, additional, Empl, A, additional, Etenko, A, additional, Farinon, S, additional, Fischer, V, additional, Fomenko, K, additional, Franco, D, additional, Gabriele, F, additional, Gaffiot, J, additional, Galbiati, C, additional, Ghiano, C, additional, Giammarchi, M, additional, Goeger-Neff, M, additional, Goretti, A, additional, Gromov, M, additional, Hagner, C, additional, Houdy, T, additional, Hungerford, E, additional, Ianni, Aldo, additional, Ianni, Andrea, additional, Jonquères, N, additional, Jedrzejczak, K, additional, Kaiser, M, additional, Kobychev, V, additional, Korablev, D, additional, Korga, G, additional, Kornoukhov, V, additional, Kryn, D, additional, Lachenmaier, T, additional, Lasserre, T, additional, Laubenstein, M, additional, Lehnert, B, additional, Link, J, additional, Litvinovich, E, additional, Lombardi, F, additional, Lombardi, P, additional, Ludhova, L, additional, Lukyanchenko, G, additional, Machulin, I, additional, Manecki, S, additional, Maneschg, W, additional, Marcocci, S, additional, Maricic, J, additional, Mention, G, additional, Meroni, E, additional, Meyer, M, additional, Miramonti, L, additional, Misiaszek, M, additional, Montuschi, M, additional, Mosteiro, P, additional, Muratova, V, additional, Musenich, R, additional, Neumair, B, additional, Oberauer, L, additional, Obolensky, M, additional, Ortica, F, additional, Pallavicini, M, additional, Papp, L, additional, Perasso, L, additional, Pocar, A, additional, Ranucci, G, additional, Razeto, A, additional, Re, A, additional, Romani, A, additional, Roncin, R, additional, Rossi, N, additional, Schönert, S, additional, Scola, L, additional, Semenov, D, additional, Simgen, H, additional, Skorokhvatov, M, additional, Smirnov, O, additional, Sotnikov, A, additional, Sukhotin, S, additional, Suvorov, Y, additional, Tartaglia, R, additional, Testera, G, additional, Thurn, J, additional, Toropova, M, additional, Unzhakov, E, additional, Veyssiere, C, additional, Vishneva, A, additional, Vivier, M, additional, Vogelaar, R B, additional, von Feilitzsch, F, additional, Wang, H, additional, Weinz, S, additional, Winter, J, additional, Wojcik, M, additional, Wurm, M, additional, Yokley, Z, additional, Zaimidoroga, O, additional, Zavatarelli, S, additional, Zuber, K, additional, and Zuzel, G, additional

Published
2016
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50. The high precision measurement of the144Ce activity in the SOX experiment

Author

Noto, L Di, primary, Agostini, M, additional, Althenmüller, K, additional, Appel, S, additional, Bellini, G, additional, Benziger, J, additional, Berton, N, additional, Bick, D, additional, Bonfini, G, additional, Bravo—Berguño, D, additional, Caccianiga, B, additional, Calaprice, F, additional, Caminata, A, additional, Cavalcante, P, additional, Cereseto, R, additional, Chepurnov, A, additional, Choi, K, additional, Cribier, M, additional, DAngelo, D, additional, Davini, S, additional, Derbin, A, additional, Drachnev, I, additional, Durero, M, additional, Etenko, A, additional, Farinon, S, additional, Fischer, V, additional, Fomenko, K, additional, Franco, D, additional, Gabriele, F, additional, Gaffiot, J, additional, Galbiati, C, additional, Ghiano, C, additional, Giammarchi, M, additional, Göeger-Neff, M, additional, Goretti, A, additional, Gromov, M, additional, Hagner, C, additional, Houdy, Th, additional, Hungerford, E, additional, Ianni, Aldo, additional, Ianni, Andrea, additional, Jonquères, N, additional, Jedrzejczak, K, additional, Kaiser, M, additional, Kobychev, V, additional, Korablev, D, additional, Korga, G, additional, Kornoukhov, V, additional, Kryn, D, additional, Lachenmaier, T, additional, Lasserre, T, additional, Laubenstein, M, additional, Lehnert, T, additional, Link, J, additional, Litvinovich, E, additional, Lombardi, F, additional, Lombardi, P, additional, Ludhova, L, additional, Lukyanchenko, G, additional, Machulin, I, additional, Manecki, S, additional, Maneschg, W, additional, Marcocci, S, additional, Maricic, J, additional, Mention, G, additional, Meroni, E, additional, Meyer, M, additional, Miramonti, L, additional, Misiaszek, M, additional, Montuschi, M, additional, Mosteiro, P, additional, Muratova, V, additional, Musenich, R, additional, Neumair, B, additional, Oberauer, L, additional, Obolensky, M, additional, Ortica, F, additional, Pallavicini, M, additional, Papp, L, additional, Perasso, L, additional, Pocar, A, additional, Ranucci, G, additional, Razeto, A, additional, Re, A, additional, Romani, A, additional, Roncin, R, additional, Rossi, C, additional, Rossi, N, additional, Schönert, S, additional, Scola, L, additional, Semenov, D, additional, Simgen, H, additional, Skorokhvatov, M, additional, Smirnov, O, additional, Sotnikov, A, additional, Sukhotin, S, additional, Suvorov, Y, additional, Tartaglia, R, additional, Testera, G, additional, Thurn, J, additional, Toropova, M, additional, Veyssière, C, additional, Vivier, M, additional, Unzhakov, E, additional, Vogelaar, R B, additional, von Feilitzsch, F, additional, Wang, H, additional, Weinz, S, additional, Winter, J, additional, Wojcik, M, additional, Wurm, M, additional, Yokley, Z, additional, Zaimidoroga, O, additional, Zavatarelli, S, additional, Zuber, K, additional, and Zuzel, G, additional

Published
2016
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