低质量 X 射线二元星系的引力波：现状报告
天体物理学
2009-10-31 v1 广义相对论与量子宇宙学
摘要
We summarize the observations of the spin periods of rapidly accreting neutron stars. If gravitational radiation is responsible for balancing the accretion torque at the observed spin frequencies of ~300 Hz, then the brightest of these systems make excellent gravitational wave sources for LIGO-II and beyond. We review the recent theoretical progress on two mechanisms for gravitational wave emission: mass quadrupole radiation from deformed neutron star crusts and current quadrupole radiation from r-mode pulsations in neutron star cores.
关键词
引用
@article{arxiv.astro-ph/0001129,
title = {Gravitational Waves from Low-Mass X-ray Binaries: a Status Report},
author = {Greg Ushomirsky and Lars Bildsten and Curt Cutler},
journal= {arXiv preprint arXiv:astro-ph/0001129},
year = {2009}
}
备注
10 pages, 5 figures, 3rd Edoardo Amaldi Conference on Gravitational Waves