Two-flavor hybrid stars with the Dyson-Schwinger quark model

作     者：魏金标 陈欢 H.-J.Schulze 

作者机构：School of Mathematics and PhysicsChina University of Geosciences INFN Sezione di CataniaDipartimento di FisicaUniversitá di Catania 

出 版 物：《Chinese Physics C》 (中国物理C（英文版）)

年 卷 期：2017年第41卷第11期

页      面：110-116页

核心收录：

学科分类：0709[理学-地质学] 07[理学] 0708[理学-地球物理学] 0804[工学-仪器科学与技术] 070401[理学-天体物理] 0827[工学-核科学与技术] 0703[理学-化学] 0704[理学-天文学] 070202[理学-粒子物理与原子核物理] 0702[理学-物理学] 

基　　金：Supported by NSFC(11305144,11475149,11303023) Central Universities(CUGL 140609)in China "NewCompStar,"COST Action MP1304 

主　　题：hybrid stars quark matter equation of state Dyson-Schwinger equations 

摘      要：We study the properties of two-flavor quark matter in the Dyson-Schwinger model and investigate the possible consequences for hybrid neutron stars,with particular regard to the two-solar-mass *** find that with some extreme values of the model parameters,the mass fraction of two-flavor quark matter in heavy neutron stars can be as high as 30 percent and the possible energy release during the conversion from nucleonic neutron stars to hybrid stars can reach 1052 erg.