Gravitational waves from r-modes

被引：0
|
作者：
Paulo M. Sá
Brigitte Tomé
机构：
[1] Universidade do Algarve,Centro Multidisciplinar de Astrofísica – CENTRA, Departamento de Física, Faculdade de Ciências e Tecnologia
来源：
Astrophysics and Space Science | 2007年 / 308卷
关键词：
Neutron stars; Stellar pulsation; Gravitational waves; 97.60.Jd; 97.10.Sj; 04.30.Db;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Detectability of gravitational waves emitted by newly born, hot, rapidly rotating neutron stars as they spin down due to the r-mode instability is discussed. It is shown that differential rotation induced by r-modes plays a fundamental role in the evolution of the mode’s instability, making it more difficult to detect these gravitational waves.
引用
收藏
页码：557 / 561
页数：4
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