大学物理 ›› 2025, Vol. 44 ›› Issue (8): 8-.doi: 10.16854/j.cnki.1000-0712.250103

• 专家视点 • 上一篇    下一篇

天文教育II:迈向奇点的致密星

刘荷蕾, 徐仁新
  

  1. 1. 新疆大学物理科学与技术学院,乌鲁木齐新疆 830046;2. 北京大学物理学院天文系;3. 核物理与核技术全国重点实验室,北京100871
  • 收稿日期:2025-03-03 修回日期:2025-03-12 出版日期:2025-11-03 发布日期:2025-11-11
  • 通讯作者: 徐仁新,E-mail: r.x.xu@pku.edu.cn
  • 作者简介:刘荷蕾(1987—),女,河南南阳人,新疆大学物理科学与技术学院教授,博士,主要从事致密星、I型X射线暴等研究工作.
  • 基金资助:
    新疆维吾尔自治区自然科学基金项目(2024D01C52),新疆维吾尔自治区重大科技专项子课题(2022A03013-3),国家自然科学基金项目(12263006)资助

Astronomy education II: compact stars going towards the singularity

LIU HeLei1, Xu Renxin2,3   

  1. 1.School of physical science and technology, Xinjiang University, Urumuqi, Xinjiang 830046, China; 
    2. Department of astronomy, Peking University, Beijing 100871, China; 
    3. State Key Laboratory of Nuclear Physics and Technology, Beijing 100871, China
  • Received:2025-03-03 Revised:2025-03-12 Online:2025-11-03 Published:2025-11-11

Abstract:  It is clear from the singularity theorem that the formation of black holes is inevitable in the Universe, but the path from massive stars to black holes cannot be “smooth” under their own gravity. By analyzing the balance between the internal and gravitational energy of stars, the process from main sequence star to compact star (white dwarf, neutron star and black hole) is discussed in general, and the semi-quantitative relationship between the accumulated internal energy per baryon (ε) and the stellar radius (R) is also presented. During a stars journey towards the singularity (R→0), there are three stages that prevent it from gravitational collapse, corresponding to the internal energy per baryon of ε ~keV(main-sequence stars), ~MeV (white dwarfs) and ~100 MeV (neutron stars). For black holes,R→0, ε→∞. Finally, the basic physical properties of compact stars and their impact on the modern astrophysics, as well as the education of stellar astronomy, are briefly reviewed.

Key words:  astronomy education, star, compact star, gravity