Enhanced antineutrino emission from β decay in core-collapse supernovae with self-consistent weak decay rates
- 15 June 2026
- journal article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 113 (12)
Abstract
No abstract availableFunding Information
- U.S. Department of Energy (DOE-DE-NA0004245)
- Office of Science (DE-SC0023175)
- Vetenskapsrådet (2020-00452)
- National Science Foundation (OISE-1927130)
- Michigan State University
- Texas A and M University (PHY250120)
- Stewardship Science Academic (DE-SC0023688)
- Stewardship Science Academic (DE-SC0023128)
- Advanced Cyberinfrastructure Coordination Ecosystem (2138259)
- Advanced Cyberinfrastructure Coordination Ecosystem (2138286)
- Advanced Cyberinfrastructure Coordination Ecosystem (2138307)
- Advanced Cyberinfrastructure Coordination Ecosystem (2137603)
- Advanced Cyberinfrastructure Coordination Ecosystem (2138296)
This publication has 55 references indexed in Scilit:
- Nuclear weak rates and nuclear weak processes in starsProgress in Particle and Nuclear Physics, 2022
- Improved estimate of electron capture rates on nuclei during stellar core collapseNuclear Physics A, 2010
- Theory of core-collapse supernovaePhysics Reports, 2007
- Detection possibility of the pair-annihilation neutrinos from the neutrino-cooled pre-supernova starAstroparticle Physics, 2004
- RATE TABLES FOR THE WEAK PROCESSES OF pf-SHELL NUCLEI IN STELLAR ENVIRONMENTSAtomic Data and Nuclear Data Tables, 2001
- Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environmentsNuclear Physics A, 2000
- Supernova electron capture rates on odd-odd nucleiPhysics Letters B, 1999
- Rate Tables for the Weak Processes of sd-Shell Nuclei in Stellar MatterAtomic Data and Nuclear Data Tables, 1994
- Detection of the neutrino signal from SN 1987A in the LMC using the INR Baksan underground scintillation telescopePhysics Letters B, 1988
- Stellar weak interaction rates for intermediate-mass nuclei. II - A = 21 to A = 60The Astrophysical Journal, 1982