中子星物理简览
核理论
2018-05-03 v1
摘要
本文中我们简要回顾中子星物理的若干方面。引言之后，我们给出中子星概念及其自 1930 年代中期至今理论与观测发展的简要历史概述。随后，我们回顾其观测的若干方面，特别讨论所用各类望远镜、这些天体的多种天体物理表现，以及质量、半径或引力波等若干可观测量。最后，我们简要总结其组成、结构方程、状态方程以及中微子发射与冷却等一些理论问题。
引用
@article{arxiv.1805.00837,
title = {A short walk through the physics of neutron stars},
author = {Isaac Vidana},
journal= {arXiv preprint arXiv:1805.00837},
year = {2018}
}
备注
Lecture given at the school "Rewriting Nuclear Physics Textbooks: Basic nuclear interactions and their applications to nuclear processes in the Cosmos and on Earth" held in Pisa during the last week of July 2017. To be published in the European Physical Journal Plus. 41 pages, 3 figures