Full simulation of the Sudbury Neutrino Observatory proportional counters

نویسندگان

  • B Beltran
  • H Bichsel
  • B Cai
  • G A Cox
  • H Deng
  • J Detwiler
  • J A Formaggio
  • S Habib
  • A L Hallin
  • A Hime
  • M Huang
  • C Kraus
  • H R Leslie
  • J C Loach
  • R Martin
  • S McGee
  • M L Miller
  • B Monreal
  • J Monroe
  • N S Oblath
  • S J M Peeters
  • A W P Poon
  • G Prior
  • K Rielage
  • R G H Robertson
  • M W E Smith
  • L C Stonehill
  • N Tolich
  • T Van Wechel
  • H Wan Chan Tseung
  • J Wendland
  • J F Wilkerson
چکیده

The third phase of the Sudbury Neutrino Observatory (SNO) experiment added an array of 3He proportional counters to the detector. The purpose of this neutral-current detection (NCD) array was to observe neutrons resulting from neutral-current solar-neutrino–deuteron interactions. We have developed a detailed simulation of current pulses from NCD array proportional counters, from the primary neutron capture on 3He through NCD array signalprocessing electronics. This NCD array MC simulation was used to model the alpha-decay background in SNO’s third-phase 8B solar-neutrino measurement.

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تاریخ انتشار 2011