R-mode instability in compact stars

被引：3

作者：

Zhu, Cui ^{[1
]}

Wang, Yu-bin ^{[1
]}

Zhou, Xia ^{[1
,2
]}

机构：

[1] Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China

[2] Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China

来源：

XIAMEN-CUSTIPEN WORKSHOP ON THE EQUATION OF STATE OF DENSE NEUTRON-RICH MATTER IN THE ERA OF GRAVITATIONAL WAVE ASTRONOMY | 2019年 / 2127卷

基金：

中国国家自然科学基金;

关键词：

NEUTRON-STARS; X-RAY; DIFFERENTIAL ROTATION; STRANGE STARS; OSCILLATIONS; RADIATION; RUNAWAY;

D O I：

10.1063/1.5117802

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

R-mode oscillations occurring in compact stars have been identified as viable and promising targets for continuous gravitational wave searches. The interesting fact about the r-modes is that they allow us to probe the interior structure and composition of compact stars directly. As well as emitting gravitational wave, r-modes would strongly affect the thermal and spin evolution of compact stars. We are going to review the theory about the gravitational wave driven r-mode instability in a rapidly rotating compact star in this paper. In particular, we will focus on r-mode instability window, r-mode evolution and delectability of r-mode.

引用

页数：9

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