Electron capture of iron group nuclei in magnetars

Abstract

Using the theory of relativity in superstrong magnetic fields (SMFs) and nuclear shell model, we carry out estimation for electron capture (EC) rates on iron group nuclei in SMFs. The rates of change of electronic abundance (RCEA) due to EC are also investigated in SMFs. It is concluded that the EC rates of most iron group nuclides are increased greatly by SMFs and even exceeded by nine orders of magnitude. On the other hand, RCEA is influenced greatly by SMFs and even reduced by more than eight orders of magnitude in the EC reaction.We also compare our results with those of Fuller et al.(FFN) and Aufderheide et al.(AUFD) in the case with and without SMFs. The results show that our results are in good agreement with AUFD's, but the rates of FFN's are about close to one order of magnitude bigger than ours in the case without SMFs. On the contrary, our calculated rates for most nuclides in SMFs are increased and even exceeded as much as for nine and eight orders of magnitude of compared to FFN's and AUFD's results, which is in the case without SMFs, respectively.

8 pages, 13 figures, accepted by MNRAS

References in corpus (3)

• The physics of strong magnetic fields in neutron stars
• Electron capture of strongly screening nuclides ${}^{56}$Fe, ${}^{56}$Co, ${}^{56}$Ni , ${}^{56}$Mn ,${}^{56}$Cr and ${}^{56}$V in presupernova
• Landau level-superfluid modified factor and effective X/$\gamma$-ray coefficient of a magnetar

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