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An new estimate of electron capture of nuclides Co-55 and Ni-56 in magnetars

机译:磁星中Co-55和Ni-56核素电子俘获的新估计

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摘要

Basing on the theory of relativity in ultrastrong magnetic fields (UMFs) and Random Phase Approximation (RPA), by using the Shell-Model Monte Carlo (SMMC) method, the influence of UMFS on electron capture (EC) and the rates of electron fraction change (REFC) of nuclides Co-55 and Ni-56 are investigated in magnetars. Basing on the Dirac delta-function and Pauli exclusion principle, we also discuss the influence on electron Fermi energy by UMFs in magnetars. The results show that the EC rates are increased greatly and even exceed five orders of magnitude by UMFs. The REFC is decreased even more than six orders of magnitude due to UMFs.
机译:基于超强磁场(UMFs)和随机相位近似(RPA)的相对论,通过壳模型蒙特卡洛(SMMC)方法,研究了UMFS对电子俘获(EC)和电子分数速率的影响在磁星中研究了Co-55和Ni-56核素的变化(REFC)。基于狄拉克δ函数和保利排斥原理,我们还讨论了UMF在磁星中对电子费米能量的影响。结果表明,UMF使EC率大大提高,甚至超过了五个数量级。由于UMF,REFC降低了六个数量级以上。

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