/ Experiment-HEP

Monte Carlo simulations in neutrino physics: the example of the SOX experiment

Caminata, A. (INFN, Genoa) ; Agostini, M. (Munich, Tech. U., Universe) ; Altenmüller, K. (Munich, Tech. U., Universe) ; Appel, S. (Munich, Tech. U., Universe) ; Bellini, G. (INFN, Milan Bicocca) ; Benziger, J. (Princeton U., Chem. Eng. Dept.) ; Berton, N. (IRFU, SPhN, Saclay) ; Bick, Daniel (Hamburg U.) ; Bonfini, G. (Gran Sasso) ; Bravo, D. (Virginia Tech.) ; Caccianiga, B. (INFN, Milan Bicocca) ; Calaprice, F. (Princeton U.) ; Carlini, M. (Gran Sasso) ; Cavalcante, P. (Gran Sasso) ; Chepurnov, A. (SINP, Moscow) ; Choi, K. (Hawaii U.) ; Cribier, M. (IRFU, SPhN, Saclay) ; D'Angelo, D. (INFN, Milan Bicocca) ; Davini, S. (L'Aquila U.) ; Derbin, A. (St. Petersburg, INP) ; Di Noto, L. (INFN, Genoa) ; Drachnev, I. (L'Aquila U.) ; Durero, M. (IRFU, SPhN, Saclay) ; Etenko, A. (Kurchatov Inst., Moscow) ; Farinon, S. (INFN, Genoa) ; Fischer, V. (IRFU, SPhN, Saclay) ; Fomenko, K. (Dubna, JINR) ; Formozov, A. (Dubna, JINR) ; Franco, D. (APC, Paris) ; Gabriele, F. (Gran Sasso) ; Gaffiot, J. (IRFU, SPhN, Saclay) ; Galbiati, C. (Princeton U.) ; Ghiano, C. (INFN, Genoa) ; Giammarchi, M. (INFN, Milan Bicocca) ; Goeger-Neff, M. (Munich, Tech. U., Universe) ; Goretti, A. (Princeton U.) ; Gromov, M. (SINP, Moscow) ; Hagner, Caren (Hamburg U.) ; Houdy, Th. (IRFU, SPhN, Saclay) ; Hungerford, E. (Houston U.) ; Ianni, Aldo (Gran Sasso) ; Ianni, Andrea (Princeton U.) ; Jonqueres, N. (Saclay) ; Jedrzejczak, K. (Jagiellonian U. (main)) ; Jeschke, D. (Munich, Tech. U., Universe) ; Kaiser, M. (Hamburg U.) ; Kobychev, V. (Kiev, INR) ; Korablev, D. (Dubna, JINR) ; Korga, G. (Gran Sasso) ; Kornoukhov, V. (Moscow, ITEP) ; Kryn, D. (APC, Paris) ; Lachenmaier, T. (Tubingen U.) ; Lasserre, T. (IRFU, SPhN, Saclay) ; Laubenstein, M. (Gran Sasso) ; Lehnert, B. (Dresden, Tech. U.) ; Link, J. (Virginia Tech.) ; Litvinovich, E. (Moscow Inst. Engineers Geodesy) ; Lombardi, F. (Gran Sasso) ; Lombardi, P. (Milan U.) ; Ludhova, L. (INFN, Milan Bicocca) ; Lukyanchenko, G. (Kurchatov Inst., Moscow) ; Machulin, I. (Moscow Inst. Engineers Geodesy) ; Manecki, S. (Virginia Tech.) ; Maneschg, W. (Heidelberg, Max Planck Inst.) ; Marcocci, S. (L'Aquila U.) ; Maricic, J. (Hawaii U.) ; Mention, G. (IRFU, SPhN, Saclay) ; Meroni, E. (INFN, Milan Bicocca) ; Meyer, M. (Hamburg U.) ; Miramonti, L. (INFN, Milan Bicocca) ; Misiaszek, M. (Jagiellonian U. (main)) ; Montuschi, M. (INFN, Ferrara) ; Mosteiro, P. (Princeton U.) ; Muratova, V. (St. Petersburg, INP) ; Musenich, R. (INFN, Genoa) ; Neumair, B. (Munich, Tech. U., Universe) ; Oberauer, L. (Munich, Tech. U., Universe) ; Obolensky, M. (APC, Paris) ; Ortica, F. (INFN, Perugia) ; Pallavicini, M. (INFN, Genoa) ; Papp, L. (Munich, Tech. U., Universe) ; Perasso, L. (INFN, Genoa) ; Pocar, A. (Massachusetts U., Amherst) ; Ranucci, G. (INFN, Milan Bicocca) ; Razeto, Adelia (Gran Sasso) ; Re, A. (INFN, Milan Bicocca) ; Romani, A. (INFN, Perugia) ; Roncin, R. (APC, Paris) ; Rossi, N. (Gran Sasso) ; Schönert, S. (Munich, Tech. U., Universe) ; Scola, L. (IRFU, SPhN, Saclay) ; Semenov, D. (St. Petersburg, INP) ; Simgen, H. (Heidelberg, Max Planck Inst.) ; Skorokhvatov, M. (Moscow Inst. Engineers Geodesy) ; Smirnov, O. (Dubna, JINR) ; Sotnikov, A. (Dubna, JINR) ; Sukhotin, S. (St. Petersburg, INP) ; Tartaglia, R. (Gran Sasso) ; Testera, G. (INFN, Genoa) ; Thurn, J. (Dresden, Tech. U.) ; Toropova, M. (Kurchatov Inst., Moscow) ; Veyssiere, C. (IRFU, SPhN, Saclay) ; Vivier, M. (IRFU, SPhN, Saclay) ; Unzhakov, E. (St. Petersburg, INP) ; Vogelaar, R. B. (Virginia Tech.) ; von Feilitzsch, F. (Munich, Tech. U., Universe) ; Wang, H. (UCLA) ; Weinz, S. (U. Mainz, PRISMA) ; Winter, J. (U. Mainz, PRISMA) ; Wojcik, M. (Kiev, INR) ; Wurm, M. (U. Mainz, PRISMA) ; Yokley, Z. (Virginia Tech.) ; Zaimidoroga, O. (Dubna, JINR) ; Zavatarelli, S. (INFN, Genoa) ; Zuber, K. (Dresden, Tech. U.) ; Zuzel, G. (Jagiellonian U. (main)) ; Suvorov, Y. (UCLA)

Year: 2016
Page No: 105-112
Pages: 8
Year: 2016 published

Abstract: 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.

Web-Page: http://inspirehep.net/record/1501320/files/fulltext.pdf

Total numbers of views: 478
Numbers of unique views: 139
DOI: 10.3204/DESY-PROC-2016-05/21
 Record created 2017-01-09, last modified 2017-01-09

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