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中国物理学会期刊

磁荷对中子星质量半径比的约束

CSTR: 32037.14.aps.62.160401

Magnetic charge constrained the mass-radius ratio of neutron star

CSTR: 32037.14.aps.62.160401
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  • 讨论了荷电(磁)质点的量子力学波方程及其解. 由磁场中解的奇异性讨论了磁单极的存在; 由Rubakov-Callan模型推知中子星可能含有大量磁单极. 然后采用中子星的结构方程, 讨论了磁荷对中子星质量半径比的约束, 分别得到了磁荷对中子星质量半径比上限的影响 和磁荷对中子星质量半径比下限的影响的数学表达式.

     

    In this paper, we use the wave equation of charged mass point to prove the existence of magnetic monopole. And according to Rubakov-Callan model there could be a lot of magnetic monopoles in neutron stars. Then using the structure equation of neutron stars we obtain upper limit and lower limit of mass-radius ratio for magnetic charged neutron star.

     

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