论文标题
Pulsar故障：评论
Pulsar Glitches: A Review
论文作者
论文摘要
已经观察到所有已知脉冲星的$ \ sim 6 \％$ $ $ $ $ $ $ $ $ $ $ $ $ $ $ $ $。五十多年来，这些现象在帮助了解Pulsar（Astro）物理学方面发挥了重要作用。基于对Pulsar Glitches搜索方法的综述，近年来观察结果的进展总结了，包括中国望远镜获得的成就。小故障脉冲星表现出大量的行为，可以将其分为四类：正常的故障，缓慢的故障，延迟旋转的故障和抗纤毛。审查了已提出的故障的主要模型，并在我们当前的理解方面对其对中子星结构的影响进行了严格的研究。此外，还详细介绍和讨论了磁层状态变化与脉冲星 - 内部过程相关的磁层状态变化之间的相关性，这表明磁层状态变化与脉冲星的相关性有关。
$\sim 6\%$ of all known pulsars have been observed to exhibit sudden spin-up events, known as glitches. For more than fifty years, these phenomena have played an important role in helping to understand pulsar (astro)physics. Based on the review of pulsar glitches search method, the progress made in observations in recent years is summarized, including the achievements obtained by Chinese telescopes. Glitching pulsars demonstrate great diversity of behaviours, which can be broadly classified into four categories: normal glitches, slow glitches, glitches with delayed spin-ups, and anti-glitches. The main models of glitches that have been proposed are reviewed and their implications for neutron star structure are critically examined regarding our current understanding. Furthermore, the correlations between glitches and emission changes, which suggest that magnetospheric state-change is linked to the pulsar-intrinsic processes, are also described and discussed in some detail.
