中子星的自旋演变

IF 3.2 Q2 ASTRONOMY & ASTROPHYSICS

Galaxies Pub Date : 2024-02-06 DOI:10.3390/galaxies12010007

Pavel Abolmasov, Anton Biryukov, Sergei B. Popov

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引用次数: 0

摘要

在本文中，我们回顾了中子星磁旋转特性的基本原理，重点是不同演化阶段的自旋上升/自旋下降行为。主要目的是提供各种状态（射电脉冲星、推进器、吸积器等）下的自旋频率变化方程。由于目前中子星在各个阶段的自旋行为仍然存在许多不确定性，我们回顾了多年来文献中提出的不同建议。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Spin Evolution of Neutron Stars

In this paper we review the basics of magneto-rotational properties of neutron stars focusing on spin-up/spin-down behavior at different evolutionary stages. The main goal is to provide equations for the spin frequency changes in various regimes (radio pulsar, propeller, accretor, etc.). Since presently the spin behavior of neutron stars at all stages remains a subject of many uncertainties, we review different suggestions made over the years in the literature.

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来源期刊

Galaxies Physics and Astronomy-Astronomy and Astrophysics

CiteScore

4.90

自引率

12.00%

发文量

100

审稿时长

11 weeks

期刊介绍： Es una revista internacional de acceso abierto revisada por pares que proporciona un foro avanzado para estudios relacionados con astronomía, astrofísica y cosmología. Areas temáticas Astronomía Astrofísica Cosmología Astronomía observacional: radio, infrarrojo, óptico, rayos X, neutrino, etc. Ciencia planetaria Equipos y tecnologías de astronomía. Ingeniería Aeroespacial Análisis de datos astronómicos. Astroquímica y Astrobiología. Arqueoastronomía Historia de la astronomía y cosmología. Problemas filosóficos en cosmología.