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Gravitational wave background from coalescing compact stars in eccentric orbits | | V.B. Ignatiev
; A.G.Kuranov
; K.A. Postnov
; M.E. Prokhorov
; | | Date: |
18 Jun 2001 | | Journal: | Mon.Not.Roy.Astron.Soc. 327 (2001) 531 | | Subject: | astro-ph gr-qc | | Affiliation: | Faculty of Physics, Moscow State University), A.G.Kuranov (Sternberg Astronomical Institute, Moscow, Russia), K.A. Postnov (Faculty of Physics, Moscow State University, Max-Planck Institut für Astrophysik, Garching, Germany), M.E. Prokhorov (Stern | | Abstract: | Stochastic gravitational wave background produced by a stationary coalescing population of binary neutron stars in the Galaxy is calculated. This background is found to constitute a confusion limit within the LISA frequency band up to a limiting frequency $NUlim{}sim 10^{-3}$ Hz, leaving the frequency window $sim 10^{-3}$--$10^{-2}$ Hz open for the potential detection of cosmological stochastic gravitational waves and of signals involving massive black holes out to cosmological distances. | | Source: | arXiv, astro-ph/0106299 | | Services: | Forum | Review | PDF | Favorites | |
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