Gravitational wave background from a sample of 330 + 4 pulsars

Details Gravitational wave background from a sample of 330 + 4 pulsars Gravitational wave background from a sample of 330 + 4 pulsars

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...203..322b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 203, no. 2, Sept. 1988, p. 322-328. Research sponsored by Ministero della Pubb

Statistics

Computation

9

Computational Astrophysics, Gravitational Waves, Pulsars, Abundance, Amplitude Modulation, Continuous Radiation, Phase Modulation

Scientific paper

The gross features of gravitational radiation bathing the earth from a set of 330 + 4 pulsars have been computed. Particular attention has been paid in evaluating the lower and upper bounds of the gravitational-wave (GW) background, in view of planning GW detection experiments in the frequency range 0.1-1000 Hz. The analysis seems to indicate that strain sensitivities of the order of 10 to the -26th would allow the detection of several sparse pulsar sources.

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