COMPACT STARS IN HADRON AND QUARK-HADRON MODELS

被引：1

作者：

Schramm, S. ^{[1
]}

Dexheimer, V. A. ^{[2
]}

机构：

[1] Goethe Univ Frankfurt, FIAS, D-60438 Frankfurt, Germany

[2] Gettysburg Coll, Dept Phys, Gettysburg, PA 17325 USA

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2010年 / 19卷 / 8-10期

关键词：

Chiral symmetry; neutron star; quark star; NEUTRON-STARS; NUCLEI;

D O I：

10.1142/S0218271810017810

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We investigate strongly interacting dense matter and neutron stars using a flavor-SU(3) approach based on a nonlinear realization of chiral symmetry. We study chiral symmetry restoration and the equation of state of stellar matter and determine neutron star properties using different sets of degrees of freedom. Finally, we include quarks in the model approach. We show the resulting phase diagram as well as hybrid star solutions for this model.

引用

页码：1455 / 1462

页数：8

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