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Special Purpose Pulsar Telescope for the Detection of Cosmic Gravitational Waves

Shou-Guan Wang·Zong-Hong Zhu·Zhen-Long Zou·Yuan-Zhong Zhang
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Abstract

Pulsars can be used to search for stochastic backgrounds of gravitational waves of cosmological origin within the very low frequency band (VLF), $10^{-7}$ to $10^{-9}$ Hz. We propose to construct a special 50 m radio telescope. Regular timing measurements of about 10 strong millisecond pulsars will perhaps allow the detection of gravitational waves within VLF or at least will give a more stringent upper limits.

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Shou-Guan Wang, Zong-Hong Zhu, Zhen-Long Zou, Yuan-Zhong Zhang. 2002-12-09. Special Purpose Pulsar Telescope for the Detection of Cosmic Gravitational Waves. https://doi.org/10.1142/s0218271802002566

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