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中国物理学会期刊

超强磁场对中子星外壳层核素56Fe,56Co,56Ni,56Mn和56Cr电子俘获过程中微子能量损失的影响

CSTR: 32037.14.aps.59.5169

Effect of superstrong magnetic field on neutrino energy loss of the nuclide 56Fe, 56Co, 56Ni, 56Mn and 56Cr by electron capture in the crust of neutron stars

CSTR: 32037.14.aps.59.5169
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  • 研究了超强磁场对中子星外壳层核素56Fe,56Co,56Ni,56Mn和56Cr电子俘获过程中微子能量损失的影响.结果表明,就大部分中子星表面的磁场B13G,超强磁场对中微子能量损失率的影响很小.对于一些磁场范围为1013—1015G的超磁星,超强磁场可使中微子能量损失率大大降低,甚至超过5个数量级.

     

    We investigated the neutrino energy loss by electron capture of the nuclide 56Fe, 56Co, 56Ni, 56Mn and 56Cr in superstrong magnetic field at the crusts of neutron stars. The results showed that the superstrong magnetic field has only a slight effect on the neutrino energy loss rates when B13 G on surfaces of most neutron stars. Whereas for some magnetars, the range of the magnetic field is 1013—1015 G, the neutrino energy loss rates would be lowered greatly and may be even decreased more than five orders of magnitude by superstrong magnetic field.

     

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