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Evolution of rotating isolated compact stars
Xia Zhou1,2; Zhi-Yong Liu1,2; Na Wang1,2
2013
会议名称3rd Galileo - Xu Guangqi Meeting
会议日期11-15 Oct. 2011
通讯作者邮箱zhouxia@xao.ac.cn
会议地点Beijing, China
关键词Dense matter stars: neutron stars: evolution
卷号23
页码304-308
通讯作者Xia Zhou
英文摘要Differential rotation is an important feature of nonlinear r-modes. We investigate the role of differential rotation in the evolution of compact stars, including its cooling and spin evolution. Both normal neutron stars and strange stars are discussed. The heating effects due to viscous dissipation of the r-mode delay the cooling and spin evolution of compact stars. Especially, slight spin-up and a long time temperature plateaus in the cooling curves of normal neutron stars are found in case of differential rotation. We suggest the spin and cooling evolution should be taken into account synthetically, for the rotation of the star is a possible huge energy source for the thermal evolution of the star.
收录类别其他
会议录International Journal of Modern Physics: Conference Series
会议录出版者World Scientific Publishing Co. Pte. Ltd., Singapore
语种英语
ISSN号2010-1945
内容类型会议论文
源URL[http://ir.xao.ac.cn/handle/45760611-7/943]  
专题脉冲星研究团组
新疆天文台_射电天文研究室
新疆天文台_其它
作者单位1.Xinjiang Astronomical Observatory, CAS, 150, Science 1-Street Urumqi 830011, P. R. China
2.Key Laboratory of Radio Astronomy CAS, Urumqi 830011, P. R. China
推荐引用方式
GB/T 7714
Xia Zhou,Zhi-Yong Liu,Na Wang. Evolution of rotating isolated compact stars[C]. 见:3rd Galileo - Xu Guangqi Meeting. Beijing, China. 11-15 Oct. 2011.
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