GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS |
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Effect of Ultrastrong Magnetic Field on the Electron Capture in the Stellar Surroundings |
WANG Kun,LUO Zhi-Quan**,LI Ying-Lin |
Institute of Theoretical Physics, China West Normal University, Nanchong 637009 |
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Cite this article: |
WANG Kun, LUO Zhi-Quan, LI Ying-Lin 2012 Chin. Phys. Lett. 29 049701 |
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Abstract Using the nuclear shell model, we study the influence of ultra-strong magnetic field on the electron capture nuclei reactions 56,58Co→56,58Fe, 56,57Ni→56,57Co, 52,53Fe→52,53Mn and 57,60Cu→57,60Ni. The results show that the electron capture rates of most iron group nuclei are increased greatly in the ultrastrong magnetic field, and even exceed three orders of magnitude in the range from 5×1013 G to 2.5×1017 G.
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Received: 30 October 2011
Published: 04 April 2012
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PACS: |
97.60.-s
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(Late stages of stellar evolution (including black holes))
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95.85.Sz
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(Gravitational radiation, magnetic fields, and other observations)
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23.40.-s
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(β-decay;double β-decay; electron and muon capture)
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