The effects of intense magnetic fields on Landau levels in a neutron star
The effects of intense magnetic fields on Landau levels in a neutron star
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DOI：
10.1007/s10509-011-0733-7
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发表时间：
2011-06
影响因子：
1.9
通讯作者：
Z. F. Gao;N. Wang;D. Song;J. Yuan;C. Chou
中科院分区：
文献类型：
--
作者：
Z. F. Gao;N. Wang;D. Song;J. Yuan;C. Chou
本文基于对中子星磁场分布的分析，提出了一种计算高强度磁场中电子费米能（EF(e)）的近似方法。中子星内部可以同时存在不同形式的强磁场，通过磁场能量的释放可以产生高电子费米能。计算结果表明：EF(e)与密度ρ、每重子平均电子数Ye和磁场强度B有关。
In this paper, an approximate method of calculating the Fermi energy of electrons (EF(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:EF(e) is related to densityρ, the mean electron number per baryonYeand magnetic field strengthB.