Stochastic background from extra-galactic double neutron stars

Details Stochastic background from extra-galactic double neutron stars Stochastic background from extra-galactic double neutron stars

2007-07-30

arxiv.org/abs/0707.4327v1

Class.Quant.Grav.24:S627-S638,2007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, 7 figures - proceeding of a talk given at the 11th GWDAW, to appear in CQG

Scientific paper

10.1088/0264-9381/24/19/S25

We present Monte Carlo simulations of the extra galactic population of inspiralling double neutron stars, and estimate its contribution to the astrophysical gravitational wave background, in the frequency range of ground based interferometers, corresponding to the last thousand seconds before the last stable orbit when more than 96 percent of the signal is released. We show that sources at redshift z>0.5 contribute to a truly continuous background which may be detected by correlating third generation interferometers.

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