Citation
Vb. Ignatiev et al., Gravitational wave background from coalescing compact stars in eccentric orbits, M NOT R AST, 327(2), 2001, pp. 531-537
Citations number
23
Categorie Soggetti
Space Sciences
Journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN journal
00358711
→ ACNP
Volume
327
Issue
2
Year of publication
2001
Pages
531 - 537
Database
ISI
SICI code
0035-8711(20011021)327:2<531:GWBFCC>2.0.ZU;2-D
Abstract
Stochastic gravitational wave background produced by a stationary coalescin
g population of binary neutron stars in the Galaxy is calculated. This back
ground is found to constitute a confusion limit within the LISA frequency b
and up to a limiting frequency of nu (lim) similar to to 10(-3) HZ, leaving
the frequency window similar to 10(-3)-10(-2) Hz open for the potential de
tection of cosmological stochastic GWs and of signals involving massive bla
ck holes out to cosmological distances.