Highly accurate calculation of rotating neutron stars

被引：38

作者：

Ansorg, M ^{[1
]}

Kleinwächter, A ^{[1
]}

Meinel, R ^{[1
]}

机构：

[1] Univ Jena, Inst Theoret Phys, D-07743 Jena, Germany

来源：

ASTRONOMY & ASTROPHYSICS | 2002年 / 381卷 / 03期

关键词：

stars : rotation; stars : neutron; gravitation; relativity; methods : numerical;

D O I：

10.1051/0004-6361:20011643

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A new spectral code for constructing general-relativistic models of rapidly rotating stars with an unprecedented accuracy is presented. As a first application, we reexamine uniformly rotating homogeneous stars and compare our results with those obtained by several previous codes. Moreover, representative relativistic examples corresponding to highly flattened rotating bodies are given.

引用

页码：L49 / L52

页数：4

共 40 条

[1]

[Anonymous], LECT NOTES PHYS

[2]

[Anonymous], 1885, CR HEBD ACAD SCI

[3] REEXAMINATION OF POST-NEWTONIAN MACLAURIN SPHEROIDS [J].