Beta-decay rates of FP shell nuclei with A greater than 60 in massive stars at the presupernova stage
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 46 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Indispensability of cross-shell contributions in neutron resonance spacing;Journal of Physics G: Nuclear and Particle Physics;2024-03-07
2. Validity of Brink-Axel Hypothesis for calculations of allowed stellar weak rates of heavy nuclei;Physica Scripta;2023-07-26
3. Statistical nuclear spectroscopy with q-normal and bivariate q-normal distributions and q-hermite polynomials;Annals of Physics;2022-11
4. Comparisons of the electron capture of iron group nuclei from two strongly screening models in presupernova;Journal of Astrophysics and Astronomy;2022-09-30
5. How effective is the Brink–Axel hypothesis for astrophysical weak rates?;Journal of Physics G: Nuclear and Particle Physics;2022-04-21
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