Modified Brink-Axel hypothesis for astrophysical Gamow-Teller transitions
Abstract
Weak interaction charged current transition strengths from highly excited nuclear states are fundamental ingredients for accurate modeling of compact object composition and dynamics, but are difficult to obtain either from experiment or theory. For lack of alternatives, calculations have often fallen back upon a generalized Brink-Axel hypothesis, that is, assuming the strength function (transition probability) is independent of the initial nuclear state but depends only upon the transition energy and the weak interaction properties of the parent nucleus ground state. Here we present numerical evidence for a modified “local” Brink-Axel hypothesis for Gamow-Teller transitions for pf-shell nuclei relevant to astrophysical applications. Specifically, while the original Brink-Axel hypothesis does not hold globally, strength functions from initial states nearby in energy are similar within statistical fluctuations. This agrees with previous work on strength function moments. Using this modified hypothesis, we can tackle strength functions at previously intractable initial energies, using semiconverged initial states at arbitrary excitation energy. Our work provides a well-founded method for computing accurate thermal weak transition rates for medium-mass nuclei at temperatures occurring in stellar cores near collapse. We finish by comparing results to previous calculations of astrophysical rates.
- Authors:
-
- Univ. of California, San Diego, CA (United States)
- San Diego State Univ., CA (United States)
- Publication Date:
- Research Org.:
- San Diego State Univ., CA (United States); Oak Ridge Associated Universities (ORAU), Oak Ridge, TN (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Office of Workforce Development for Teachers & Scientists (WDTS); National Science Foundation (NSF); Simons Foundation
- OSTI Identifier:
- 1979857
- Grant/Contract Number:
- FG02-03ER41272; SC0014664; ACI-1548562; PHY-170054; PHY-1914242; PHY-2020275; 2017-228
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. C
- Additional Journal Information:
- Journal Volume: 105; Journal Issue: 1; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; Physics; electroweak interactions in nuclear physics; nuclear astrophysics; nuclear physics of explosive environments; nuclear structure & decays; thermal & statistical models
Citation Formats
Herrera, Raúl A., Johnson, Calvin W., and Fuller, George M. Modified Brink-Axel hypothesis for astrophysical Gamow-Teller transitions. United States: N. p., 2022.
Web. doi:10.1103/physrevc.105.015801.
Herrera, Raúl A., Johnson, Calvin W., & Fuller, George M. Modified Brink-Axel hypothesis for astrophysical Gamow-Teller transitions. United States. https://doi.org/10.1103/physrevc.105.015801
Herrera, Raúl A., Johnson, Calvin W., and Fuller, George M. Mon .
"Modified Brink-Axel hypothesis for astrophysical Gamow-Teller transitions". United States. https://doi.org/10.1103/physrevc.105.015801. https://www.osti.gov/servlets/purl/1979857.
@article{osti_1979857,
title = {Modified Brink-Axel hypothesis for astrophysical Gamow-Teller transitions},
author = {Herrera, Raúl A. and Johnson, Calvin W. and Fuller, George M.},
abstractNote = {Weak interaction charged current transition strengths from highly excited nuclear states are fundamental ingredients for accurate modeling of compact object composition and dynamics, but are difficult to obtain either from experiment or theory. For lack of alternatives, calculations have often fallen back upon a generalized Brink-Axel hypothesis, that is, assuming the strength function (transition probability) is independent of the initial nuclear state but depends only upon the transition energy and the weak interaction properties of the parent nucleus ground state. Here we present numerical evidence for a modified “local” Brink-Axel hypothesis for Gamow-Teller transitions for pf-shell nuclei relevant to astrophysical applications. Specifically, while the original Brink-Axel hypothesis does not hold globally, strength functions from initial states nearby in energy are similar within statistical fluctuations. This agrees with previous work on strength function moments. Using this modified hypothesis, we can tackle strength functions at previously intractable initial energies, using semiconverged initial states at arbitrary excitation energy. Our work provides a well-founded method for computing accurate thermal weak transition rates for medium-mass nuclei at temperatures occurring in stellar cores near collapse. We finish by comparing results to previous calculations of astrophysical rates.},
doi = {10.1103/physrevc.105.015801},
journal = {Physical Review. C},
number = 1,
volume = 105,
place = {United States},
year = {Mon Jan 03 00:00:00 EST 2022},
month = {Mon Jan 03 00:00:00 EST 2022}
}
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