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β Decay of V61 and its Role in Cooling Accreted Neutron Star Crusts

  • Published:2020-12-28 Issue:26 Volume:125 Page:
  • ISSN:0031-9007
  • Container-title:Physical Review Letters
  • language:en
  • Short-container-title:Phys. Rev. Lett.

Author:

Ong W.-J.,Brown E. F.ORCID,Browne J.,Ahn S.ORCID,Childers K.,Crider B. P.,Dombos A. C.,Gupta S. S.,Hitt G. W.ORCID,Langer C.,Lewis R.,Liddick S. N.,Lyons S.,Meisel Z.,Möller P.,Montes F.,Naqvi F.,Pereira J.,Prokop C.,Richman D.,Schatz H.,Schmidt K.,Spyrou A.

Funder

Michigan State University

National Science Foundation

U.S. Department of Energy

National Nuclear Security Administration

Lawrence Livermore National Laboratory

Nuclear Science and Security Consortium

Publisher

American Physical Society (APS)

Subject

General Physics and Astronomy

Cited by 10 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. β -delayed neutron emission of Mn64, Cr62 , and Fe65;Physical Review C;2024-08-27

2. Shell-model study of weak β-decays relevant to astrophysical processes;Frontiers in Physics;2024-08-09

3. β -decay feeding intensity distribution of Mn64;Physical Review C;2024-04-05

4. Shell-Model Study of Nuclear Weak Rates relevant to Astrophysical Processes in Stars;Journal of Physics: Conference Series;2023-03-01

5. Roles of Spin-dependent Transitions in Nuclei on Astrophysical Processes in Stars;Proceedings of the 24th International Spin Symposium (SPIN2021);2022-12-26
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