The importance of the mixed phase in hybrid stars built with the Nambu-Jona-Lasinio model

被引：28

作者：

Paoli, M. G. ^{[1
]}

Menezes, D. P. ^{[1
]}

机构：

[1] Univ Fed Santa Catarina, CFM, Dept Fis, BR-88040900 Florianopolis, SC, Brazil

来源：

EUROPEAN PHYSICAL JOURNAL A | 2010年 / 46卷 / 03期

关键词：

NEUTRON-STAR; QUARK MATTER; DYNAMICAL MODEL; HADRON; SUPERCONDUCTIVITY; TRANSITIONS; EQUATIONS; ANALOGY;

D O I：

10.1140/epja/i2010-11059-0

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 investigate the structure of hybrid stars based on two different constructions: one is based on the Gibbs condition for phase coexistence and considers the existence of a mixed phase (MP), and the other is based on the Maxwell construction and no mixed phase is obtained. The hadron phase is described by the non-linear Walecka model (NLW) and the quark phase by the Nambu-Jona-Lasinio model (NJL). We conclude that the masses and radii obtained are model dependent but not significantly different for both constructions.

引用

页码：413 / 420

页数：8

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