On the maximum mass of differentially rotating neutron stars

被引：300

作者：

Baumgarte, TW ^{[1
]}

Shapiro, SL ^{[1
]}

Shibata, M ^{[1
]}

机构：

[1] Univ Illinois, Dept Astron, Urbana, IL 61801 USA

来源：

ASTROPHYSICAL JOURNAL | 2000年 / 528卷 / 01期

基金：

美国国家科学基金会;

关键词：

black hole physics; relativity; stars : neutron; stars : rotation;

D O I：

10.1086/312425

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We construct relativistic equilibrium models of differentially rotating neutron stars and show that they can support significantly more mass than their nonrotating or uniformly rotating counterparts. We dynamically evolve such "hypermassive" models in full general relativity and show that there do exist configurations that are dynamically stable against radial collapse and bar formation. Our results suggest that the remnant of binary neutron star coalescence may be temporarily stabilized by differential rotation, leading to delayed collapse and a delayed gravitational wave burst.

引用

页码：L29 / L32

页数：4

共 42 条

[1] Equation of state of nucleon matter and neutron star structure [J].