Full simulation of the Sudbury Neutrino Observatory proportional counters
Author(s)
Beltran, B.; Bichsel, H.; Cai, B.; Cox, G. A.; Deng, H.; Detwiler, J.; Formaggio, Joseph A.; Habib, S.; Hallin, A. L.; Hime, A.; Huang, M.; Kraus, C.; Leslie, H. R.; Loach, J. C.; Martin, R.; McGee, S.; Peeters, S. J. M.; Poon, A. W. P.; Prior, G.; Rielage, K.; Robertson, R. G. H.; Smith, M. W. E.; Stonehill, L. C.; Tolich, N.; Van Wechel, T.; Tseung, H. Wan Chan; Wendland, J.; Wilkerson, J. F.; Wright, A.; ... Show more Show less
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The third phase of the Sudbury Neutrino Observatory (SNO) experiment added an array of [superscript 3]He 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 [superscript 3]He through NCD array signal-processing electronics. This NCD array MC simulation was used to model the alpha-decay background in SNO's third-phase ⁸B solar-neutrino measurement.
Date issued
2011-07Department
Massachusetts Institute of Technology. Department of Physics; Massachusetts Institute of Technology. Laboratory for Nuclear ScienceJournal
New Journal of Physics
Publisher
Institute of Physics Publishing
Citation
Beltran, B et al. “Full Simulation of the Sudbury Neutrino Observatory Proportional Counters.” New Journal of Physics 13.7 (2011): 073006. Web.
Version: Final published version