Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Self-consistent microscopic calculations for electron captures on nuclei in core-collapse supernovae

Journal Article · · Physical Review. C
DOI:https://doi.org/10.1103/5r9z-ygmx· OSTI ID:3021380
Calculations for electron capture rates on nuclei with atomic numbers between 𝑍 = 20 and 𝑍 = 52 are performed in a self-consistent finite-temperature covariant energy density functional theory within the relativistic quasiparticle random-phase approximation. Electron captures on these nuclei contribute most to reducing the electron fraction during the collapse phase of core-collapse supernovae. The rates include contributions from allowed (Gamow-Teller) and first-forbidden (FF) transitions, and it is shown that the latter become dominant at high stellar densities and temperatures. Temperature-dependent effects such as Pauli unblocking and transitions from thermally excited states are also included. The new rates are implemented in a spherically symmetric one-dimensional simulation of the core-collapse phase. The results indicate that the increase in electron capture rates, due to inclusion of FF transitions, leads to reductions of the electron fraction at nuclear saturation density, the peak neutrino luminosity, and enclosed mass at core bounce. The new rates reaffirm that the most relevant nuclei for the deleptonization situate around the 𝑁 = 50 and 82 shell closures, but, compared to previous simulations, nuclei are less proton rich. Here, the new rates developed in this work are available, and will be of benefit to improve the accuracy of multidimensional supernova simulations.
Research Organization:
Michigan State University, East Lansing, MI (United States)
Sponsoring Organization:
U.S. National Science Foundation (NSF); USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
NA0004074
Other Award/Contract Number:
NSF-2209429
PHY-1927130
OSTI ID:
3021380
Journal Information:
Physical Review. C, Journal Name: Physical Review. C Journal Issue: 3 Vol. 112; ISSN 2469-9985; ISSN 2469-9993
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

References (53)

Rate Tables for the Weak Processes of sd-Shell Nuclei in Stellar Matter journal March 1994
RATE TABLES FOR THE WEAK PROCESSES OF pf-SHELL NUCLEI IN STELLAR ENVIRONMENTS journal September 2001
Hydrodynamics of core-collapse supernovae and their progenitors journal June 2020
Equation of state in the gravitational collapse of stars journal July 1979
Electron capture in stellar collapse journal June 1984
Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments journal June 2000
A statistical model for a complete supernova equation of state journal June 2010
Improved estimate of electron capture rates on nuclei during stellar core collapse journal December 2010
The 76Se Gamow–Teller strength distribution and its importance for stellar electron capture rates journal June 2011
Relativistic Hartree?Bogoliubov theory: static and dynamic aspects of exotic nuclear structure journal April 2005
Theory of core-collapse supernovae journal April 2007
Nuclear weak rates and nuclear weak processes in stars journal September 2022
Super-AGB Stars and their Role as Electron Capture Supernova Progenitors journal January 2017
Strong neutrino cooling by cycles of electron capture and β− decay in neutron star crusts journal December 2013
Sensitivity of Type Ia supernovae to electron capture rates journal April 2019
Stellar weak-interaction rates for sd-shell nuclei. I - Nuclear matrix element systematics with application to Al-26 and selected nuclei of importance to the supernova problem journal February 1980
Stellar weak interaction rates for intermediate mass nuclei. III - Rate tables for the free nucleons and nuclei with A = 21 to A = 60 journal January 1982
The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis journal November 1995
The Accuracy, Consistency, and Speed of Five Equations of State for Stellar Hydrodynamics journal November 1999
Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning‐Front Propagation
  • Iwamoto, Koichi; Brachwitz, Franziska; Nomoto, Ken’ichi
  • The Astrophysical Journal Supplement Series, Vol. 125, Issue 2 https://doi.org/10.1086/313278
journal December 1999
Proton-rich Nuclear Statistical Equilibrium journal September 2008
Core-Collapse Supernova Equations of State Based on Neutron star Observations journal August 2013
An Open-Source Neutrino Radiation Hydrodynamics code for Core-Collapse Supernovae journal August 2015
Impact of electron-captures on nuclei near N = 50 on core-collapse supernovae journal December 2017
Electron capture in stars journal May 2021
Core-collapse supernovae as supercomputing science: A status report toward six-dimensional simulations with exact Boltzmann neutrino transport in full general relativity journal January 2012
Constraints for stellar electron-capture rates on Kr 86 via the Kr 86 ( t , He 3 + γ ) Br 86 reaction and the implications for core-collapse supernovae journal October 2019
Impact of electron capture rates for nuclei far from stability on core-collapse supernovae journal January 2020
Unblocking of stellar electron capture for neutron-rich N=50 nuclei at finite temperature journal February 2020
Gamow-Teller excitations at finite temperature: Competition between pairing and temperature effects journal April 2020
Stellar electron-capture rates based on finite-temperature relativistic quasiparticle random-phase approximation journal December 2020
Impact of complex many-body correlations on electron capture in thermally excited nuclei around Ni78 journal February 2021
Evolution of β -decay half-lives in stellar environments journal November 2021
Finite-temperature electron-capture rates for neutron-rich nuclei near N=50 and effects on core-collapse supernova simulations journal May 2022
Global properties of nuclei at finite-temperature within the covariant energy density functional theory journal January 2024
Semileptonic Weak Interactions with C 12 journal September 1972
Neutrino spectra from stellar electron capture journal October 2001
Relativistic model for nuclear matter and atomic nuclei with momentum-dependent self-energies journal June 2005
Gamow-Teller strength distributions at finite temperatures and electron capture in stellar environments journal January 2010
Statistical description of complex nuclear phases in supernovae and proto-neutron stars journal December 2010
Gamow-Teller strengths and electron-capture rates for p f -shell nuclei of relevance for late stellar evolution journal July 2012
Large-scale evaluation of β -decay rates of r -process nuclei with the inclusion of first-forbidden transitions journal February 2016
Stellar electron capture rates on neutron-rich nuclei and their impact on stellar core collapse journal February 2017
Multipole excitations in hot nuclei within the finite temperature quasiparticle random phase approximation framework journal August 2017
Electron Capture Rates on Nuclei and Implications for Stellar Core Collapse journal June 2003
Supernova mechanisms journal October 1990
Colloquium : Perspectives on core-collapse supernova theory journal February 2013
Elucidating the finite temperature quasiparticle random phase approximation journal February 2025
Physics of Core-Collapse Supernovae in Three Dimensions: A Sneak Preview journal October 2016
Heating in Magnetar Crusts from Electron Captures journal June 2021
The Sensitivity of Core-Collapse Supernovae to Nuclear Electron Capture journal December 2015
ELECTRON-CAPTURE AND β -DECAY RATES FOR sd -SHELL NUCLEI IN STELLAR ENVIRONMENTS RELEVANT TO HIGH-DENSITY O–NE–MG CORES journal January 2016
Evolution of ONeMg Core in Super-AGB Stars toward Electron-capture Supernovae: Effects of Updated Electron-capture Rate journal November 2019