skip to main content
US FlagAn official website of the United States government
dot gov icon
Official websites use .gov
A .gov website belongs to an official government organization in the United States.
https lock icon
Secure .gov websites use HTTPS
A lock ( lock ) or https:// means you've safely connected to the .gov website. Share sensitive information only on official, secure websites.

Attention:

The DOI auto-population feature in the Public Access Repository (PAR) will be unavailable from 4:00 PM ET on Tuesday, July 8 until 4:00 PM ET on Wednesday, July 9 due to scheduled maintenance. We apologize for the inconvenience caused.


This content will become publicly available on August 1, 2025

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
More Like this
  1. The ratio of branching fractions R ( D * ) = B ( B ¯ D * τ ν ¯ τ ) / B ( B ¯ D * ν ¯ ) , where is an electron or muon, is measured using a Belle II data sample with an integrated luminosity of 189 fb 1 at the SuperKEKB asymmetric-energy e + e collider. Data is collected at the ϒ ( 4 S ) resonance, and one B meson in the ϒ ( 4 S ) B B ¯ decay is fully reconstructed in hadronic decay modes. The accompanying signal B meson is reconstructed as B ¯ D * τ ν ¯ τ using leptonic τ decays. The normalization decay, B ¯ D * ν ¯ , 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 R ( D * ) = 0.262 0.039 + 0.041 ( stat ) 0.032 + 0.035 ( syst ) . This result is consistent with the current world average and with Standard Model predictions. Published by the American Physical Society2024 
    more » « less
  2. We measure the complete set of angular coefficients J i for exclusive B ¯ D * ν ¯ decays ( = e , μ ). Our analysis uses the full 711 fb 1 Belle dataset with hadronic tag-side reconstruction. The results allow us to extract the form factors describing the B ¯ D * transition and the Cabibbo-Kobayashi-Maskawa matrix element | V cb | . Using recent lattice QCD calculations for the hadronic form factors, we find | V cb | = ( 40.7 ± 0.7 ) × 10 3 using the Boyd-Grinstein-Lebed parametrization, compatible with determinations from inclusive semileptonic decays. We search for lepton flavor universality violation as a function of the hadronic recoil parameter w and investigate the differences of the electron and muon angular distributions. We find no deviation from standard model expectations. Published by the American Physical Society2024 
    more » « less
  3. This Letter reports a search for charge-parity ( C P ) 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 ν μ ( ν ¯ μ ) ν μ ( ν ¯ μ ) and ν μ ( ν ¯ μ ) ν e ( ν ¯ e ) oscillation channels are used to measure the effect of the NSI parameters ϵ e μ and ϵ e τ . With 90% CL the magnitudes of the NSI couplings are constrained to be | ϵ e μ | 0.3 and | ϵ e τ | 0.4 . A degeneracy at | ϵ e τ | 1.8 is reported, and we observe that the presence of NSI limits sensitivity to the standard C P phase δ C P . Published by the American Physical Society2024 
    more » « less
  4. The first results of the study of high-energy electron neutrino ( ν e ) and muon neutrino ( ν μ ) charged-current interactions in the FASER ν emulsion-tungsten detector of the FASER experiment at the LHC are presented. A 128.8 kg subset of the FASER ν volume was analyzed after exposure to 9.5 fb 1 of s = 13.6 TeV p p data. Four (eight) ν e ( ν μ ) interaction candidate events are observed with a statistical significance of 5.2 σ ( 5.7 σ ). This is the first direct observation of ν e interactions at a particle collider and includes the highest-energy ν e and ν μ ever detected from an artificial source. The interaction cross section per nucleon σ / E ν is measured over an energy range of 560–1740 GeV (520–1760 GeV) for ν e ( ν μ ) to be ( 1.2 0.7 + 0.8 ) × 10 38 cm 2 GeV 1 [ ( 0.5 ± 0.2 ) × 10 38 cm 2 GeV 1 ], consistent with standard model predictions. These are the first measurements of neutrino interaction cross sections in those energy ranges. Published by the American Physical Society2024 
    more » « less
  5. We report the results of the first search for B decays to the Ξ ¯ c 0 Λ ¯ c final state using 711 fb 1 of data collected at the ϒ ( 4 S ) resonance with the Belle detector at the KEKB asymmetric-energy e + e collider. The results are interpreted in terms of both direct baryon-number-violating B decay and Ξ c 0 Ξ ¯ c 0 oscillations which follow the standard model decay B Ξ c 0 Λ ¯ c . We observe no evidence for baryon number violation and set the 95% confidence-level upper limits on the ratio of baryon-number-violating and standard model branching fractions B ( B Ξ ¯ c 0 Λ ¯ c ) / B ( B Ξ c 0 Λ ¯ c ) to be < 2.7 % and on the effective angular frequency of mixing ω in Ξ c 0 Ξ ¯ c 0 oscillations to be < 0.76 ps 1 (equivalent to τ mix > 1.3 ps ). Published by the American Physical Society2024 
    more » « less