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The Monte Carlo simulation of the Borexino detector

Authors :
Marcocci, S.
Agostini, M.
Bonfini, G.
Wurm, M.
Yokley, Z.
Zaimidoroga, O.
Zavatarelli, S.
Zuber, K.
Zuzel, G.
BOREXINO Collaboration
Bravo, D.
Caccianiga, B.
Calaprice, F.
Caminata, A.
Caprioli, S.
Carlini, M.
Cavalcante, P.
Chepurnov, A.
Choi, K.
Altenmüller, K.
Collica, L.
D'Angelo, D.
Davini, S.
Derbin, A.
Ding, X. F.
Ludovico, A. Di
Noto, L. Di
Drachnev, I.
Fomenko, K.
Formozov, A.
Appel, S.
Franco, D.
Gabriele, F.
Galbiati, C.
Ghiano, C.
Giammarchi, M.
Goretti, A.
Gromov, M.
Guffanti, D.
Hagner, C.
Houdy, T.
Atroshchenko, V.
Hungerford, E.
Ianni, Aldo
Ianni, Andrea
Jany, A.
Jeschke, D.
Kobychev, V.
Korablev, D.
Korga, G.
Kryn, D.
Laubenstein, M.
Bagdasarian, Zara
Litvinovich, E.
Lombardi, F.
Lombardi, P.
Ludhova, Livia
Lukyanchenko, G.
Lukyanchenko, L.
Machulin, I.
Manuzio, G.
Martyn, J.
Meroni, E.
Basilico, D.
Meyer, M.
Miramonti, L.
Misiaszek, M.
Muratova, V.
Neumair, B.
Oberauer, L.
Opitz, B.
Orekhov, V.
Ortica, F.
Pallavicini, M.
Bellini, G.
Papp, L.
Penek, Ömer
Pilipenko, N.
Pocar, A.
Porcelli, A.
Ranucci, G.
Razeto, A.
Re, A.
Redchuk, Mariia
Romani, A.
Benziger, J.
Roncin, R.
Rossi, N.
Schönert, S.
Semenov, D.
Skorokhvatov, M.
Smirnov, O.
Sotnikov, A.
Stokes, L. F. F.
Suvorov, Y.
Tartaglia, R.
Bick, D.
Testera, G.
Thurn, J.
Toropova, M.
Unzhakov, E.
Vishneva, A.
Vogelaar, R. B.
von Feilitzsch, F.
Wang, H.
Weinz, S.
Wojcik, M.
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)
Borexino
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
BOREXINO
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Source :
J.Phys.Conf.Ser., 15th International Conference on Topics in Astroparticle and Underground Physics, 15th International Conference on Topics in Astroparticle and Underground Physics, Jul 2017, Sudbury, Canada. pp.012035, ⟨10.1088/1742-6596/1342/1/012035⟩, Journal of physics / Conference Series 1342(1), 012035 (2020). doi:10.1088/1742-6596/1342/1/012035, 15th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2017, Sudbury, Canada, 2017-07-24-2017-07-28
Publication Year :
2017
Publisher :
HAL CCSD, 2017.

Abstract

Borexino is a 300 ton sub-MeV liquid scintillator solar neutrino detector which has been running at the Laboratori Nazionali del Gran Sasso (Italy) since 2007. Thanks to its unprecedented radio-purity, it was able to measure the flux of 7Be, 8B, pp, and pep solar neutrinos and to detect geo-neutrinos. A reliable simulation of the detector is an invaluable tool for all Borexino physics analyses. The simulation accounts for the energy loss of particles in all the detector components, the generation of the scintillation photons, their propagation within the liquid scintillator volume, and a detailed simulation of the electronics chain. A novel efficient method for simulating the external background which survives the Borexino passive shield was developed. This technique allows to reliably predict the effect of the contamination in the peripheral construction materials. The techniques developed to simulate the Borexino detector and their level of refinement are of possible interest to the neutrino and dark matter communities, especially for current and future large-volume liquid scintillator experiments.

Details

Language :
English
Database :
OpenAIRE
Journal :
J.Phys.Conf.Ser., 15th International Conference on Topics in Astroparticle and Underground Physics, 15th International Conference on Topics in Astroparticle and Underground Physics, Jul 2017, Sudbury, Canada. pp.012035, ⟨10.1088/1742-6596/1342/1/012035⟩, Journal of physics / Conference Series 1342(1), 012035 (2020). doi:10.1088/1742-6596/1342/1/012035, 15th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2017, Sudbury, Canada, 2017-07-24-2017-07-28
Accession number :
edsair.doi.dedup.....16a81f9a16b66a37225ee911b31ccd41