Special Purpose Pulsar Telescope for the Detection of Cosmic Gravitational Waves

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dc.creatorWang, Shou-Guan
dc.creatorZhu, Zong-Hong
dc.creatorZou, Zhen-Long
dc.creatorZhang, Yuan-Zhong
dc.date2002-12-09
dc.date.accessioned2026-07-07T10:47:31Z
dc.date.available2026-07-07T10:47:31Z
dc.descriptionPulsars 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.
dc.description5 pages, no figure, Latex file
dc.identifierhttps://arxiv.org/abs/astro-ph/0212191
dc.identifierhttp://arxiv.org/abs/astro-ph/0212191
dc.identifierInt.J.Mod.Phys.D11:1061-1065,2002
dc.identifierdoi:10.1142/S0218271802002566
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183561
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSpecial Purpose Pulsar Telescope for the Detection of Cosmic Gravitational Waves
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