Full simulation of the Sudbury Neutrino Observatory proportional counters

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 ha...

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Bibliographic Details
Main Authors: 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.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Institute of Physics Publishing 2012
Online Access:http://hdl.handle.net/1721.1/70602
https://orcid.org/0000-0002-3757-9883
Description
Summary: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.