论文标题
关于脉冲星故障的角动量转移机制的挑战
On the challenges of Angular Momentum Transfer Mechanism of Pulsar Glitches
论文作者
论文摘要
脉冲星故障的角动量转移机制已有四十年了，现在是独立的理论，说明了小故障大小和吉利奇间的时间间隔。但是，最近的分析和统计分析正处于抑制理论的边缘。在本文中，我们概述了超流体理论，以强调角动量过程的功效，并强调了理论和观察证据，这些证据无法通过涉及角动量转移的过程来解释。
The angular momentum transfer mechanism of pulsar glitches for over four decades now stands as standalone theory with regards to glitch sizes and inter-glitch time intervals. However, recent analyses both analytic and statistical are on the verge of suppressing the theory. In this paper, we overviewed the superfluid theory to highlight the efficacy of the angular momentum process and highlighted the theoretical and observational evidences that could not be explained by processes involving transfer of angular momentum.
