Special Purpose Pulsar Telescope for the Detection of Cosmic Gravitational Waves

Details Special Purpose Pulsar Telescope for the Detection of Cosmic Gravitational Waves Special Purpose Pulsar Telescope for the Detection of Cosmic Gravitational Waves

2002-12-09

arxiv.org/abs/astro-ph/0212191v1

Int.J.Mod.Phys.D11:1061-1065,2002

Astronomy and Astrophysics

Astrophysics

5 pages, no figure, Latex file

Scientific paper

10.1142/S0218271802002566

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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