摘要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.
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.
(β-decay;double β-decay; electron and muon capture)
引用本文:
WANG Kun,LUO Zhi-Quan**,LI Ying-Lin. Effect of Ultrastrong Magnetic Field on the Electron Capture in the Stellar Surroundings[J]. 中国物理快报, 2012, 29(4): 49701-049701.
WANG Kun,LUO Zhi-Quan**,LI Ying-Lin. Effect of Ultrastrong Magnetic Field on the Electron Capture in the Stellar Surroundings. Chin. Phys. Lett., 2012, 29(4): 49701-049701.
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2012, Vol. 29 
