Detection of supernova neutrinos at spallation neutron sources

  • After considering supernova shock effects, Mikheyev-Smirnov-Wolfenstein effects, neutrino collective effects, and Earth matter effects, the detection of supernova neutrinos at the China Spallation Neutron Source is studied and the expected numbers of different flavor supernova neutrinos observed through various reaction channels are calculated with the neutrino energy spectra described by the Fermi-Dirac distribution and the "beta fit" distribution respectively. Furthermore, the numerical calculation method of supernova neutrino detection on Earth is applied to some other spallation neutron sources, and the total expected numbers of supernova neutrinos observed through different reactions channels are given.
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Ming-Yang Huang, Xin-Heng Guo and Bing-Lin Young. Detection of supernova neutrinos at spallation neutron sources[J]. Chinese Physics C, 2016, 40(7): 073102. doi: 10.1088/1674-1137/40/7/073102
Ming-Yang Huang, Xin-Heng Guo and Bing-Lin Young. Detection of supernova neutrinos at spallation neutron sources[J]. Chinese Physics C, 2016, 40(7): 073102.  doi: 10.1088/1674-1137/40/7/073102 shu
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Received: 2015-11-05
Revised: 2016-02-06
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    Supported by National Natural Science Foundation of China (11205185, 11175020, 11275025, 11575023)

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Detection of supernova neutrinos at spallation neutron sources

    Corresponding author: Ming-Yang Huang,
    Corresponding author: Xin-Heng Guo,
    Corresponding author: Bing-Lin Young,
Fund Project:  Supported by National Natural Science Foundation of China (11205185, 11175020, 11275025, 11575023)

Abstract: After considering supernova shock effects, Mikheyev-Smirnov-Wolfenstein effects, neutrino collective effects, and Earth matter effects, the detection of supernova neutrinos at the China Spallation Neutron Source is studied and the expected numbers of different flavor supernova neutrinos observed through various reaction channels are calculated with the neutrino energy spectra described by the Fermi-Dirac distribution and the "beta fit" distribution respectively. Furthermore, the numerical calculation method of supernova neutrino detection on Earth is applied to some other spallation neutron sources, and the total expected numbers of supernova neutrinos observed through different reactions channels are given.

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