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of core-collapse supernovae and neutron stars; 2) neutrino-nucleus reactions: exploring the interaction mechanisms between neutrinos and nuclei; 3) neutrino multi-messenger physics: constrain the dense
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supernova neutrino background • Supernova burst neutrinos in the multi-messenger era • Numerical simulation of core-collapse supernovae IHEP values diversity and welcomes candidates from all backgrounds
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