arXiv · 1309.0121
The effects of intense magnetic fields on Landau levels in a neutron star
Abstract
In this paper, an approximate method of calculating the Fermi energy of electrons ($E_{F}(e)$) in a high-intensity magnetic field, based on the analysis of the distribution of a neutron star magnetic field, has been proposed. In the interior of a Neutron star, different forms of intense magnetic field could exist simultaneously and a high electron Fermi energy could be generated by the release of magnetic field energy. The calculation results show that: $E_{F}(e)$ is related to density $ρ$, the mean electron number per baryon $Y_{e}$ and magnetic field strength $B$.
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Z. F. Gao, N. Wang, D. L. Song, J. P. Yuan, C. K. Chou. 2013-08-31. The effects of intense magnetic fields on Landau levels in a neutron star. https://doi.org/10.1007/s10509-011-0733-7
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