Neutron stars and quark phases in the Nambu-Jona-Lasinio model

被引：107

作者：

Schertler, K ^{[1
]}

Leupold, S

Schaffner-Bielich, J

机构：

[1] Univ Giessen, Inst Theoret Phys, D-35392 Giessen, Germany

[2] Brookhaven Natl Lab, RIKEN BNL Res Ctr, Upton, NY 11973 USA

来源：

PHYSICAL REVIEW C | 1999年 / 60卷 / 02期

关键词：

D O I：

10.1103/PhysRevC.60.025801

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 study the possible existence of deconfined quark matter in the interior of neutron stars using the Nambu-Jona-Lasinio model to describe the quark phase. We find that typical neutron stars with masses around 1.4 solar masses do not possess any deconfined quark matter in their center. This can be traced back to the property of the NJL model which suggests a large constituent strange quark mass over a wide range of densities. [S0556-2813(99)01008-0].

引用

页数：11

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