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The Monte Carlo simulation of the Borexino detector

  • M. Agostini
  • , K. Altenmüller
  • , S. Appel
  • , V. Atroshchenko
  • , Z. Bagdasarian
  • , D. Basilico
  • , G. Bellini
  • , J. Benziger
  • , D. Bick
  • , G. Bonfini
  • , L. Borodikhina
  • , D. Bravo
  • , B. Caccianiga
  • , F. Calaprice
  • , A. Caminata
  • , M. Canepa
  • , S. Caprioli
  • , M. Carlini
  • , P. Cavalcante
  • , A. Chepurnov
  • K. Choi, D. D'Angelo, S. Davini, A. Derbin, X. F. Ding, L. Di Noto, I. Drachnev, K. Fomenko, A. Formozov, D. Franco, F. Froborg, F. Gabriele, C. Galbiati, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, M. Gromov, C. Hagner, T. Houdy, E. Hungerford, Aldo Ianni, Andrea Ianni, A. Jany, D. Jeschke, V. Kobychev, D. Korablev, G. Korga, D. Kryn, M. Laubenstein, E. Litvinovich, F. Lombardi, P. Lombardi, L. Ludhova, G. Lukyanchenko, I. Machulin, M. Magnozzi, G. Manuzio, S. Marcocci, J. Martyn, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, V. Muratova, B. Neumair, L. Oberauer, B. Opitz, F. Ortica, M. Pallavicini, L. Papp, A. Pocar, G. Ranucci, A. Razeto, A. Re, A. Romani, R. Roncin, N. Rossi, S. Schönert, D. Semenov, P. Shakina, M. Skorokhvatov, O. Smirnov, A. Sotnikov, L. F.F. Stokes, Y. Suvorov, R. Tartaglia, G. Testera, J. Thurn, M. Toropova, E. Unzhakov, A. Vishneva, R. B. Vogelaar, F. von Feilitzsch, H. Wang, S. Weinz, M. Wojcik, M. Wurm, Z. Yokley, O. Zaimidoroga, S. Zavatarelli, K. Zuber, G. Zuzel
  • Gran Sasso Science Institute
  • Cluster of Excellence E-conversion
  • National Research Centre "Kurchatov Institute"
  • Forschungszentrum Jülich (FZJ)
  • University of Milan
  • Department of Chemical Engineering
  • Universität Hamburg
  • Max-Planck-Institut für Kernphysik
  • Laboratori Nazionali del Gran Sasso
  • Virginia Polytechnic Institute and State University
  • Princeton University
  • Istituto Nazionale per la Fisica della Materia
  • University of Genova
  • Moscow State University
  • University of Hawaii
  • Petersburg Nuclear Phys. Inst.
  • Joint Inst. for Nuclear Research
  • Université Paris Diderot
  • Center for Nuclear Receptors and Cell Signaling, University of Houston
  • Laboratorio Subterráneo de Canfranc
  • Jagiellonian University
  • Institute for Nuclear Research
  • National Research Nuclear University MEPhI
  • University of California, San Diego
  • RWTH Aachen University
  • Johannes Gutenberg University
  • Università di Perugia
  • University of Massachusetts Amherst
  • University of California at Los Angeles
  • Technische Universität Dresden

Research output: Contribution to journalArticlepeer-review

40 Scopus citations

Abstract

We 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.

Original languageEnglish
Pages (from-to)136-159
Number of pages24
JournalAstroparticle Physics
Volume97
DOIs
StatePublished - Jan 2018
Externally publishedYes

Keywords

  • Large volume liquid scintillator detectors
  • Monte Carlo simulations
  • Solar neutrinos

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