The ratio of branching fractions , where is an electron or muon, is measured using a Belle II data sample with an integrated luminosity of at the SuperKEKB asymmetric-energy collider. Data is collected at the resonance, and one meson in the decay is fully reconstructed in hadronic decay modes. The accompanying signal meson is reconstructed as using leptonic decays. The normalization decay, , produces the same observable final-state particles. The ratio of branching fractions is extracted in a simultaneous fit to two signal-discriminating variables in both channels and yields . This result is consistent with the current world average and with Standard Model predictions. Published by the American Physical Society2024
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This content will become publicly available on August 1, 2025
Enhanced muonization by active-sterile neutrino mixing in protoneutron stars
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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- Award ID(s):
- 2020275
- PAR ID:
- 10597769
- 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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