On the stochastic gravitational radiation background produced by an ensemble of single neutron stars.

Details On the stochastic gravitational radiation background produced by an ensemble of single neutron stars. On the stochastic gravitational radiation background produced by an ensemble of single neutron stars.

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...327..428p&link_type=abstract

Astronomy and Astrophysics, v.327, p.428-431

Astronomy and Astrophysics

Astrophysics

3

Gravitational Waves, Stars: Neutron

Scientific paper

The possible stochastic background produced by single galactic neutron star is studied. The upper limit to this background independent of the NS ellipticities is derived. If ~0.1 of old neutron star population have a low surface magnetic field (<10^7^G from the beginning or due to field decay), this background may be detected by the advanced LIGO/VIRGO interferometers with a sensitivity of ~10^-25^ at 100Hz during 1-year integration.

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