中子星的磁场会衰减吗

The evolution of X‐ray binaries Pub Date : 2008-05-12 DOI:10.1063/1.45968

F. Verbunt

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摘要

x射线双星中的中子星有很强的磁场，而那些在老双星中的中子星通常磁场较弱，但例外情况反驳了简单的解释。声称证明单个射电脉冲星自发场衰减的观测证据在更仔细的审查中被发现缺乏。描述了射电脉冲星z -分布的一些详细性质;这也许可以解释明显相似的人口综合研究的相互矛盾的结果。

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Do magnetic fields of neutron stars decay

Neutron stars in x‐ray binaries have strong magnetic fields, those in old binaries usually weak magnetic fields, but exceptions confute simple explanations. Observational evidence claimed to prove spontaneous field decay in single radio pulsars is found wanting on closer scrutiny. Some detailed properties of the z‐distributions of radio pulsars are described; these may explain the contradictory results of apparently similar population synthesis studies.

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The evolution of X‐ray binaries

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