QMC and the nature of dense matter: written in the stars?

被引：2

作者：

Carroll, J. D. ^{[1
]}

机构：

[1] Univ Adelaide, Dept Phys, Ctr Subat Struct Matter CSSM, Adelaide, SA 5005, Australia

来源：

ACHIEVEMENTS AND NEW DIRECTIONS IN SUBATOMIC PHYSICS: FESTSCHRIFT IN HONOUR OF TONY THOMAS 60TH BIRTHDAY | 2010年 / 1261卷

关键词：

QMC EOS; dense matter; neutron stars; hybrid stars; MIT NJL; MESON-COUPLING MODEL; NEUTRON-STAR;

D O I：

10.1063/1.3479349

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

We discuss the recent progress in calculating the properties of hybrid stars (stellar objects similar to neutron stars classified by the incorporation of non-nucleonic degrees of freedom including but not limited to hyperons and/or a quark matter core) using the octet baryon Quark-Meson Coupling (QMC) model The version of QMC used is a recent improvement which includes the in medium modification of the quark quark hyperfine interaction

引用

页码：226 / 231

页数：6

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