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R-mode instability in compact stars
Zhu, Cui1; Wang, Yu-Bin1; Zhou, Xia1,2
2012
Conference NameXiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy
Source PublicationAIP Proceedings of the Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy
Volume2127
Issue1
Pages020012
Conference Date JAN 03-07, 2019
Conference PlaceXiamen, PEOPLES R CHINA
CountryPEOPLES R CHINA
Contribution Rank1
AbstractR-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.
DOI10.1063/1.5117802
URL查看原文
Indexed ByCPCI
Language英语
ISBN978-0-7354-1869-1
ISSN0094-243X
WOS IDWOS:000507575500012
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/4167
Collection射电天文研究室_脉冲星研究团组
Corresponding AuthorZhou, Xia
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, 830011, China;
2.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing, 210008, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhu, Cui,Wang, Yu-Bin,Zhou, Xia. R-mode instability in compact stars[C],2012:020012.
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