Pulsars and Gravitational Waves

K. J. Lee; R. X. Xu; G. J. Qiao

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arXiv · 1109.0812

Pulsars and Gravitational Waves

K. J. Lee·R. X. Xu·G. J. Qiao

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Abstract

The relationship between pulsar-like compact stars and gravitational waves is briefly reviewed. Due to regular spins, pulsars could be useful tools for us to detect ~nano-Hz low-frequency gravitational waves by pulsar-timing array technique; besides, they would also be ~kilo-Hz high-frequency gravitational wave radiators because of their compactness. The wave strain of an isolate pulsar depends on the equation state of cold matter at supra-nuclear densities. Therefore, a real detection of gravitational wave should be very meaningful in gravity physics, micro-theory of elementary strong interaction, and astronomy.

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K. J. Lee, R. X. Xu, G. J. Qiao. 2011-09-05. Pulsars and Gravitational Waves. https://arxiv.org/abs/1109.0812

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