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Article Navigation >  Nuclear Physics Review  > 2011  >  28(2): 179-184

HUANG Ming-yang, GUO Xin-heng, #, YONG Bing-lin. Detecting Supernova Neutrinos in Daya Bay Neutrino Laboratory[J]. Nuclear Physics Review, 2011, 28(2): 179-184. doi: 10.11804/NuclPhysRev.28.02.179
Citation: HUANG Ming-yang, GUO Xin-heng, #, YONG Bing-lin. Detecting Supernova Neutrinos in Daya Bay Neutrino Laboratory[J]. Nuclear Physics Review, 2011, 28(2): 179-184. doi: 10.11804/NuclPhysRev.28.02.179
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Detecting Supernova Neutrinos in Daya Bay Neutrino Laboratory

doi: 10.11804/NuclPhysRev.28.02.179

  • 1 College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China; 2 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China; 3 Department of Physics and Astronomy, Iowa State University, Ames, Iowa 5001, USA; 4 Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China

  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2011-06-20
  • While detecting supernova neutrinos in the Daya Bay neutrino laboratory， several supernova neutrino effects need to be considered， including the supernova shock effects， the neutrino collective effects， the MikheyevSmirnovWolfenstein (MSW) effects， and the Earth matter effects. The phenomena of neutrino oscillation is affected by the above effects. Using some ratios of the event numbers of different supernova neutrinos， we propose some possible methods to identify the mass hierarchy and acquire information about the neutrino mixing angle θ13 and neutrino masses.
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Detecting Supernova Neutrinos in Daya Bay Neutrino Laboratory

doi: 10.11804/NuclPhysRev.28.02.179
  • 1 College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China; 2 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China; 3 Department of Physics and Astronomy, Iowa State University, Ames, Iowa 5001, USA; 4 Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China
  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2011-06-20

Abstract: While detecting supernova neutrinos in the Daya Bay neutrino laboratory， several supernova neutrino effects need to be considered， including the supernova shock effects， the neutrino collective effects， the MikheyevSmirnovWolfenstein (MSW) effects， and the Earth matter effects. The phenomena of neutrino oscillation is affected by the above effects. Using some ratios of the event numbers of different supernova neutrinos， we propose some possible methods to identify the mass hierarchy and acquire information about the neutrino mixing angle θ13 and neutrino masses.

HUANG Ming-yang, GUO Xin-heng, #, YONG Bing-lin. Detecting Supernova Neutrinos in Daya Bay Neutrino Laboratory[J]. Nuclear Physics Review, 2011, 28(2): 179-184. doi: 10.11804/NuclPhysRev.28.02.179
Citation: HUANG Ming-yang, GUO Xin-heng, #, YONG Bing-lin. Detecting Supernova Neutrinos in Daya Bay Neutrino Laboratory[J]. Nuclear Physics Review, 2011, 28(2): 179-184. doi: 10.11804/NuclPhysRev.28.02.179
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