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关于脉冲星物理相关的坐标系

On coordinate frames relevant for pulsar physics

Jyotijwal Debnath, Manjari Bagchi

arXiv 2608.18501首次发表:更新:

AI 中文总结

本短篇综述针对脉冲星物理相关的坐标系,呈现了大量坐标系及其间的关系,以满足脉冲星相关理论模型及多物理过程研究的需求。

AI 中文摘要

脉冲星可分为孤立系统或双星(甚至三星)系统,其观测特征被用于探究基础物理的多个方面,包括辐射机制、引力物理等。各类现象的理论模型需要不同的坐标系,不同物理过程常相互影响,需使用多个坐标系及它们之间的关系。本短篇综述呈现了大量坐标系及这些坐标系间的关系。

英文摘要

Pulsars can be either isolated or binary (or even in triple) systems. Observational features of pulsars are used to probe various aspects of fundamental physics, including emission mechanism, gravitational physics, etc. Theoretical models of various phenomena need different coordinate frames. Often different physical processes affect each other and we need to use multiple coordinate frames and relations between those. This short review presents an extensive set of coordinate frames and relations between those.

CommentsShort review. Comments are welcome

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