Nuclear <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>β</mml:mi></mml:math> spectrum from the projected shell model: Allowed one-to-one transition-Reference-Cited by-同舟云学术

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Nuclear β spectrum from the projected shell model: Allowed one-to-one transition

Published:2023-11-27 Issue:5 Volume:108 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Gao Fan,Chen Zi-Rui,Wang Long-Jun^ORCID

Funder

Fundamental Research Funds for the Central Universities

National Natural Science Foundation of China

China Institute of Atomic Energy

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.108.054313/fulltext

Reference52 articles.

1. Strong neutrino cooling by cycles of electron capture and β− decay in neutron star crusts

2. Urca Cooling in Neutron Star Crusts and Oceans: Effects of Nuclear Excitations

3. Nuclear weak-interaction processes in stars

4. Origin of the heaviest elements: The rapid neutron-capture process

5. rp-process nucleosynthesis at extreme temperature and density conditions

Cited by 2 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. Stellar β -decay rate of the s -process branching-point Tl204 : Forbidden transitions;Physical Review C;2024-07-23

2. First-forbidden transition of nuclear β decay by projected shell model;Physics Letters B;2024-03

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