标题： 轴向 anomalies 和大脉冲星速度变化 显示英文标题

标题： The Axial Anomaly and Large Pulsar Kicks

摘要： 拓扑矢量流最近引起了广泛关注，可能在RHIC通过电荷分离效应和手征磁效应得到验证。 大量工作已经致力于理解拓扑矢量流在天体物理学中的作用，特别是在中子星和夸克星内部的作用。 我们将讨论这项工作的近期一个方面，即脉冲星的喷射速度。 已知脉冲星群体中有很大比例的速度超过1000公里/秒，但这些速度的一个合适解释尚不存在。 我们将详细说明拓扑流可能是这些大喷射速度的原因，并讨论为什么该机制在其他机制失败时能够成功。 显示英文摘要

摘要： Topological vector currents have gained interest recently with their possible verification at RHIC through the Charge Separation Effect and the Chiral Magnetic Effect. Much work has been done in understanding the role of topological vector currents in astrophysics, specifically in the interiors of neutron stars and quark stars. We will discuss a recent aspect of this work regarding pulsar kicks. A significant percentage of the pulsar population is known to have velocities above 1000 km/s, but a suitable explanation for these velocities does not exist. We will detail how topological currents may be responsible for these large kicks and discuss why the mechanism is successful where others fail.