A timing signature of gravitational radiation from LMXB neutron stars

被引：0
作者：
Wagoner, RV [1 ]
机构：
[1] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
来源：
X-RAY TIMING 2003: ROSSI AND BEYOND | 2004年 / 714卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The coupled evolution of the spin frequency, core temperature, and r-mode amplitude of an accreting neutron star is calculated. We focus on those conditions that can produce persistent gravitational radiation from the r-mode. During X-ray quiescent phases of transient LMXBs, one may be able to identify the constant contribution of the gravitational wave emission to the spindown rate. Another signature is the r-mode contribution to the heating.
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页码：224 / 227
页数：4
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