Detecting Supernova Neutrinos in  Daya Bay Neutrino Laboratory

HUANG Ming-yang; GUO  Xin-heng; #; YONG Bing-lin

doi:10.11804/NuclPhysRev.28.02.179

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

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

Detecting Supernova Neutrinos in Daya Bay Neutrino Laboratory

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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

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