ON THE MAXIMUM MASS OF NEUTRON STARS

被引：46

作者：

Chamel, N. ^{[1
]}

Haensel, P. ^{[2
]}

Zdunik, J. L. ^{[2
]}

Fantina, A. F. ^{[1
]}

机构：

[1] Univ Libre Bruxelles, Inst Astron & Astrophys, B-1050 Brussels, Belgium

[2] Polish Acad Sci, Ctr Astron, PL-00716 Warsaw, Poland

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS E | 2013年 / 22卷 / 07期

关键词：

Neutron stars; maximum mass; equation of state; dense matter; EQUATION-OF-STATE; QUARK MATTER; MILLISECOND PULSAR; GENERAL-RELATIVITY; NUCLEAR-EQUATION; PSR J1903+0327; ROTATION; CAUSALITY; COMPANION; DENSITY;

D O I：

10.1142/S021830131330018X

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：

One of the most intriguing questions about neutron stars concerns their maximum mass. The answer is intimately related to the properties of matter at densities far beyond that found in heavy atomic nuclei. The current view on the internal constitution of neutron stars and on their maximum mass, both from theoretical and observational studies, are briefly reviewed.

引用

页数：25

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