Gravitational radiation of a differentially rotating superfluid neutron star

被引：0
|
作者：
Hayrapetyan, M. V. [1 ]
机构：
[1] Erevan State Univ, Yerevan, Armenia
来源：
ASTROPHYSICS | 2008年 / 51卷 / 04期
关键词：
stars:; neutron:; rotation;
D O I：
10.1007/s10511-008-9034-4
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The gravitational radiation of a neutron star with a weakly coupled superfluid component is considered. It is assumed that regions can exist in the star's core which rotate at substantially higher angular velocities than the observed angular velocities of pulsars. A star of this sort has a quadrupole moment on the order of the maximum value for the neutron star configurations that have been discussed, so it could be a powerful source of gravitational radiation for the planned Advanced LIGO detector.
引用
收藏
页码：559 / 564
页数：6
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