Crustal oscillations of slowly rotating relativistic stars

被引：0

作者：

Vavoulidis, M. ^{[1
]}

Kokkotas, K. D. ^{[1
,2
]}

Stavridis, A. ^{[1
]}

机构：

[1] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki 54124, Greece

[2] Univ Tubingen, D-72076 Tubingen, Germany

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2008年 / 384卷 / 04期

关键词：

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

D O I：

10.1111/j.1365-2966.2007.12835.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study low-amplitude crustal oscillations of slowly rotating relativistic stars consisting of a central fluid core and an outer thin solid crust. We estimate the effect of rotation on the torsional toroidal modes and on the interfacial and shear spheroidal modes. The results compared against the Newtonian ones for wide range of neutron star models and equations of state.

引用

页码：1711 / 1724

页数：14

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