Model equation of state to investigate the structure and evolution of superdense stars with a phase transition

被引：0
|
作者：
A. V. Yudin
T. L. Razinkova
D. K. Nadyozhin
机构：
[1] Institute for Theoretical and Experimental Physics,
[2] Novosibirsk State University,undefined
[3] “Kurchatov Institute” National Research Center,undefined
来源：
Astronomy Letters | 2013年 / 39卷
关键词：
phase transition; quark matter; quark stars; equation of state;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
A model equation of state that describes the phase transition to quark matter is proposed. This equation of state is used to construct hydrostatically equilibrium stellar models for various values of the entropy and the negative bag constant B added to the pressure of quarkmatter. Parameters of the calculated models and conditions for their stability are discussed.
引用
收藏
页码：161 / 170
页数：9
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