J4 ›› 2010, Vol. 48 ›› Issue (1): 109-112.

• 物理 • 上一篇    下一篇

中子星中强子-|夸克的相变

刘军胜1, 韦明2| 张宇2, 朱明枫2   

  1. 1. 北华大学 物理学院, 吉林 吉林 132013|2. 吉林大学 物理学院, 长春 130021
  • 收稿日期:2009-01-26 出版日期:2010-01-26 发布日期:2010-01-27
  • 通讯作者: 刘军胜 E-mail:liujunshenglxy@sohu.com

Hadron-Quark Phase Transition in Neutron Stars

LIU Jun-sheng1, WEI Ming2, ZHANG Yu2, ZHU Ming-feng |2   

  1. 1. College of Physics, Beihua University, Jilin 132013, Jilin Province, China|2. College |of Physics, Jilin University, Changchun 130021, China
  • Received:2009-01-26 Online:2010-01-26 Published:2010-01-27
  • Contact: LIU Jun-sheng E-mail:liujunshenglxy@sohu.com

摘要:

给出一个研究由强子相到夸克相相变的简单模型, 并定性分析了奇异星与混合星的基本性质, 计算结果在观测范围内. 

关键词: 中子星, 奇异星, 混合星, 相变

Abstract:

The authors presented a simple mode to investigate the hadron-quark phase transition. In this way, the properties of strange and hybrid stars are described qualitatively. The calculation results are within the observational range. 

Key words: neutron star, strange star, hybrid star, phase transition

中图分类号: 

  • O571.2