Effect of an Accretion Disk on the Gravitational Wave Signal from an Inspiralling Binary

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dc.creatorChakrabarti, Sandip K.
dc.date2000-12-29
dc.date.accessioned2026-07-07T01:57:12Z
dc.date.available2026-07-07T01:57:12Z
dc.descriptionSince black holes can only accrete sub-Keplerian matter, a companion black hole orbiting on a circular and instantaneously Keplerian orbit around a central, massive black hole in a galactic Centre will loss angular momentum and energy to the accreting matter. This loss could be a significant fraction of the loss due to gravitational wave (GW) emission. The corresponding GW signal would be modified. We discuss this effects in the light of the modern accretion disk theory.
dc.descriptionWorld Scientific Style (Two pages)
dc.identifierhttps://arxiv.org/abs/astro-ph/0012529
dc.identifierhttp://arxiv.org/abs/astro-ph/0012529
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2292
dc.subjectAstrophysics
dc.titleEffect of an Accretion Disk on the Gravitational Wave Signal from an Inspiralling Binary
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