Stochastic gravitational wave background from extragalactic binary stars and its angular properties

Details Stochastic gravitational wave background from extragalactic binary stars and its angular properties Stochastic gravitational wave background from extragalactic binary stars and its angular properties

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.489p&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We investigate statistical properties of extragalactic gravitational wave background formed by unresolved binary stars in galaxies with taking into account realistic distribution of matter according to Las Campanas Redshift Survey. We found that the power density of the GW energy density Omega^2(k) varies as k^{-0.5} (k is the wave number) at angular scales from 10 to 1 degrees. This is a distinctive feature of the background connected with a large scale distribution of matter as opposite to a stochastic background of cosmological origin.

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