Enhanced Muonization by Active-Sterile Neutrino Mixing in Protoneutron Stars
arXiv:2404.14485 · doi:10.1103/PhysRevD.110.043007
Abstract
We study - and - mixing in the protoneutron star (PNS) created in a core-collapse supernova (CCSN). We point out the importance of the feedback on the general composition of the PNS in addition to the obvious feedback on the lepton number. We show that for our adopted mixing parameters ~keV and consistent with the current constraints, sterile neutrino production is dominated by the Mikheyev-Smirnov-Wolfenstein conversion of into and that the subsequent escape of increases the lepton number, which in turn enhances muonization of the PNS primarily through . While these results are qualitatively robust, their quantitative effects on the dynamics and active neutrino emission of CCSNe should be evaluated by including - and - mixing in the simulations.
v2: 11 pages, 7 figures. Minor clarifications added, conclusion unchanged. Matches version published in PRD
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