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Title: Enhanced muonization by active-sterile neutrino mixing in protoneutron stars
We study ν μ ν s and ν ¯ μ ν ¯ s 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 ν μ lepton number. We show that for our adopted mixing parameters δ m 2 10 2 keV 2 and sin 2 2 θ consistent with the current constraints, sterile neutrino production is dominated by the Mikheyev–Smirnov–Wolfenstein conversion of ν ¯ μ into ν ¯ s and that the subsequent escape of ν ¯ s increases the ν μ lepton number, which in turn enhances muonization of the PNS primarily through ν μ + n p + μ . While these results are qualitatively robust, their quantitative effects on the dynamics and active neutrino emission of core-collapse supernovae should be evaluated by including ν μ ν s and ν ¯ μ ν ¯ s mixing in the simulations. Published by the American Physical Society2024  more » « less
Award ID(s):
2020275
PAR ID:
10597769
Author(s) / Creator(s):
;
Publisher / Repository:
APS
Date Published:
Journal Name:
Physical Review D
Volume:
110
Issue:
4
ISSN:
2470-0010
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
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