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arxiv: 1603.01898 · v2 · pith:ZASCGBSJnew · submitted 2016-03-07 · 🌌 astro-ph.HE · astro-ph.SR· nucl-th

A new insight into neutrino energy loss by electron capture of iron group nuclei in magnetars surface

classification 🌌 astro-ph.HE astro-ph.SRnucl-th
keywords energyelectroncapturegroupironlossmagnetarsneutrino
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Based on the relativistic mean-field effective interactions theory, and Lai dong model \citep{b37, b38, b39}, we discuss the influences of superstrong magnetic fields (SMFs) on electron Fermi energy, nuclear blinding energy, and single-particle level structure in magnetars surface. By using the method of Shell-Model Monte Carlo (SMMC), and the Random Phase Approximation (RPA) theory, we detailed analyze the neutrino energy loss rates(NELRs) by electron capture (EC) for iron group nuclei in SMFs.

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