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 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 core-collapse supernovae should be evaluated by including and mixing in the simulations. Published by the American Physical Society2024
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This content will become publicly available on November 1, 2025
Search for CP -Violating Neutrino Nonstandard Interactions with the NOvA Experiment
This Letter reports a search for charge-parity ( ) symmetry violating nonstandard interactions (NSI) of neutrinos with matter using the NOvA Experiment, and examines their effects on the determination of the standard oscillation parameters. Data from and oscillation channels are used to measure the effect of the NSI parameters and . With 90% CL the magnitudes of the NSI couplings are constrained to be and . A degeneracy at is reported, and we observe that the presence of NSI limits sensitivity to the standard phase . Published by the American Physical Society2024
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- PAR ID:
- 10588185
- Author(s) / Creator(s):
- ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »
- Publisher / Repository:
- American Physical Society
- Date Published:
- Journal Name:
- Physical Review Letters
- Volume:
- 133
- Issue:
- 20
- ISSN:
- 0031-9007
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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