Feb. 1, 2024, 12:45 p.m. | Sajad Abbar Meng-Ru Wu Zewei Xiong

cs.LG updates on arXiv.org arxiv.org

Neutrinos can undergo fast flavor conversions (FFCs) within extremely dense astrophysical environments such as core-collapse supernovae (CCSNe) and neutron star mergers (NSMs). In this study, we explore FFCs in a \emph{multi-energy} neutrino gas, revealing that when the FFC growth rate significantly exceeds that of the vacuum Hamiltonian, all neutrinos (regardless of energy) share a common survival probability dictated by the energy-integrated neutrino spectrum. We then employ physics-informed neural networks (PINNs) to predict the asymptotic outcomes of FFCs within such a …

application astro-ph.he core cs.ai cs.lg energy environments explore growth mergers networks neural networks neutrinos rate star study supernova supernovae

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