2015/11/30 by Ming-Yang Huang, Xin-Heng Guo, Bing-Lin Young
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Cosmic neutrino background #Measurements of neutrino speed #Neutrino #Neutrino Physics Research #Neutrino astronomy #Neutrino detector #Neutrino oscillation #Neutron #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Solar neutrino #Solar neutrino problem #Spallation #Spallation Neutron Source #Spectral line #Supernova #Type II supernova #hep-ph
paper · pdf · doi:10.1088/1674-1137/40/7/073102
published as Chinese Physics C, 40(7), 073102, 2016 · 7 pages, 2 figures
arxiv created 2016/01/12 · arxiv updated 2016/03/29 · openalex publication_date 2016/06/29 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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.