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The Monte Carlo simulation of the Borexino detector

Author(s): Agostini, M; Altenmueller, K; Appel, S; Atroshchenko, V; Bagdasarian, Z; et al

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dc.contributor.authorAgostini, M-
dc.contributor.authorAltenmueller, K-
dc.contributor.authorAppel, S-
dc.contributor.authorAtroshchenko, V-
dc.contributor.authorBagdasarian, Z-
dc.contributor.authorBasilico, D-
dc.contributor.authorBellini, G-
dc.contributor.authorBenziger, Jay B.-
dc.contributor.authorBick, D-
dc.contributor.authorBonfini, G-
dc.contributor.authorBorodikhina, L-
dc.contributor.authorBravo, D-
dc.contributor.authorCaccianiga, B-
dc.contributor.authorCalaprice, Frank P.-
dc.contributor.authorCaminata, A-
dc.contributor.authorCanepa, M-
dc.contributor.authorCaprioli, S-
dc.contributor.authorCarlini, M-
dc.contributor.authorCavalcante, P-
dc.contributor.authorChepurnov, A-
dc.contributor.authorChoi, K-
dc.contributor.authorD Angelo, D-
dc.contributor.authorDavini, S-
dc.contributor.authorDerbin, A-
dc.contributor.authorDing, XF-
dc.contributor.authorDi Noto, L-
dc.contributor.authorDrachnev, I-
dc.contributor.authorFomenko, K-
dc.contributor.authorFormozov, A-
dc.contributor.authorFranco, D-
dc.contributor.authorFroborg, F-
dc.contributor.authorGabriele, F-
dc.contributor.authorGalbiati, Cristiano-
dc.contributor.authorGhiano, C-
dc.contributor.authorGiammarchi, M-
dc.contributor.authorGoeger-Neff, M-
dc.contributor.authorGoretti, A-
dc.contributor.authorGromov, M-
dc.contributor.authorHagner, C-
dc.contributor.authorHoudy, T-
dc.contributor.authorHungerford, E-
dc.contributor.authorIanni, Aldo-
dc.contributor.authorIanni, Andrea-
dc.contributor.authorJany, A-
dc.contributor.authorJeschke, D-
dc.contributor.authorKobychev, V-
dc.contributor.authorKorablev, D-
dc.contributor.authorKorga, G-
dc.contributor.authorKryn, D-
dc.contributor.authorLaubenstein, M-
dc.contributor.authorLitvinovich, E-
dc.contributor.authorLombardi, F-
dc.contributor.authorLombardi, P-
dc.contributor.authorLudhova, L-
dc.contributor.authorLukyanchenko, G-
dc.contributor.authorMachulin, I-
dc.contributor.authorMagnozzi, M-
dc.contributor.authorManuzio, G-
dc.contributor.authorMarcocci, S-
dc.contributor.authorMartyn, J-
dc.contributor.authorMeroni, E-
dc.contributor.authorMeyer, M-
dc.contributor.authorMiramonti, L-
dc.contributor.authorMisiaszek, M-
dc.contributor.authorMuratova, V-
dc.contributor.authorNeumair, B-
dc.contributor.authorOberauer, L-
dc.contributor.authorOpitz, B-
dc.contributor.authorOrtica, F-
dc.contributor.authorPallavicini, M-
dc.contributor.authorPapp, L-
dc.contributor.authorPocar, A-
dc.contributor.authorRanucci, G-
dc.contributor.authorRazeto, A-
dc.contributor.authorRe, A-
dc.contributor.authorRomani, A-
dc.contributor.authorRoncin, R-
dc.contributor.authorRossi, N-
dc.contributor.authorSchoenert, S-
dc.contributor.authorSemenov, D-
dc.contributor.authorShakina, P-
dc.contributor.authorSkorokhvatov, M-
dc.contributor.authorSmirnov, O-
dc.contributor.authorSotnikov, A-
dc.contributor.authorStokes, LFF-
dc.contributor.authorSuvorov, Y-
dc.contributor.authorTartaglia, R-
dc.contributor.authorTestera, G-
dc.contributor.authorThurn, J-
dc.contributor.authorToropova, M-
dc.contributor.authorUnzhakov, E-
dc.contributor.authorVishneva, A-
dc.contributor.authorVogelaar, RB-
dc.contributor.authorvon Feilitzsch, F-
dc.contributor.authorWang, H-
dc.contributor.authorWeinz, S-
dc.contributor.authorWojcik, M-
dc.contributor.authorWurm, M-
dc.contributor.authorYokley, Z-
dc.contributor.authorZaimidoroga, O-
dc.contributor.authorZavatarelli, S-
dc.contributor.authorZuber, K-
dc.contributor.authorZuzel, G-
dc.date.accessioned2019-08-29T17:07:14Z-
dc.date.available2019-08-29T17:07:14Z-
dc.date.issued2018-01en_US
dc.identifier.citationAgostini, M, Altenmueller, K, Appel, S, Atroshchenko, V, Bagdasarian, Z, Basilico, D, Bellini, G, Benziger, J, Bick, D, Bonfini, G, Borodikhina, L, Bravo, D, Caccianiga, B, Calaprice, F, Caminata, A, Canepa, M, Caprioli, S, Carlini, M, Cavalcante, P, Chepurnov, A, Choi, K, D Angelo, D, Davini, S, Derbin, A, Ding, XF, Di Noto, L, Drachnev, I, Fomenko, K, Formozov, A, Franco, D, Froborg, F, Gabriele, F, Galbiati, C, Ghiano, C, Giammarchi, M, Goeger-Neff, M, Goretti, A, Gromov, M, Hagner, C, Houdy, T, Hungerford, E, Ianni, Aldo, Ianni, Andrea, Jany, A, Jeschke, D, Kobychev, V, Korablev, D, Korga, G, Kryn, D, Laubenstein, M, Litvinovich, E, Lombardi, F, Lombardi, P, Ludhova, L, Lukyanchenko, G, Machulin, I, Magnozzi, M, Manuzio, G, Marcocci, S, Martyn, J, Meroni, E, Meyer, M, Miramonti, L, Misiaszek, M, Muratova, V, Neumair, B, Oberauer, L, Opitz, B, Ortica, F, Pallavicini, M, Papp, L, Pocar, A, Ranucci, G, Razeto, A, Re, A, Romani, A, Roncin, R, Rossi, N, Schoenert, S, Semenov, D, Shakina, P, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Stokes, LFF, Suvorov, Y, Tartaglia, R, Testera, G, Thurn, J, Toropova, M, Unzhakov, E, Vishneva, A, Vogelaar, RB, von Feilitzsch, F, Wang, H, Weinz, S, Wojcik, M, Wurm, M, Yokley, Z, Zaimidoroga, O, Zavatarelli, S, Zuber, K, Zuzel, G. (2018). The Monte Carlo simulation of the Borexino detector. ASTROPARTICLE PHYSICS, 97 (136 - 159. doi:10.1016/j.astropartphys.2017.10.003en_US
dc.identifier.issn0927-6505-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1z14d-
dc.description.abstractWe describe the Monte Carlo (MC) simulation of the Borexino detector and the agreement of its output with data. The Borexino MC “ab initio” simulates the energy loss of particles in all detector components and generates the resulting scintillation photons and their propagation within the liquid scintillator volume. The simulation accounts for absorption, reemission, and scattering of the optical photons and tracks them until they either are absorbed or reach the photocathode of one of the photomultiplier tubes. Photon detection is followed by a comprehensive simulation of the readout electronics response. The MC is tuned using data collected with radioactive calibration sources deployed inside and around the scintillator volume. The simulation reproduces the energy response of the detector, its uniformity within the fiducial scintillator volume relevant to neutrino physics, and the time distribution of detected photons to better than 1% between 100 keV and several MeV. The techniques developed to simulate the Borexino detector and their level of refinement are of possible interest to the neutrino community, especially for current and future large-volume liquid scintillator experiments such as Kamland-Zen, SNO+, and Juno. (C) 2017 Elsevier B.V. All rights reserved.en_US
dc.format.extent136 - 159en_US
dc.language.isoen_USen_US
dc.relation.ispartofASTROPARTICLE PHYSICSen_US
dc.rightsAuthor's manuscripten_US
dc.titleThe Monte Carlo simulation of the Borexino detectoren_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1016/j.astropartphys.2017.10.003-
dc.date.eissued2017-10-17en_US
dc.identifier.eissn1873-2852-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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