Potential Sources of Gravitational Wave Emission and Laser Beam Interferometers

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dc.creatorPacheco, J. A. de Freitas
dc.date2000-12-06
dc.date.accessioned2026-07-07T01:56:53Z
dc.date.available2026-07-07T01:56:53Z
dc.descriptionThe properties of potential gravitational wave sources like neutron stars, black holes and binary systems are reviewed, as well as the different contributions (stochastic and continuous) to the gravitational wave background. The detectability of these sources by the present generation of laser beam interferometers, which will be fully operational around 2002, is also considered.
dc.descriptionPaper presented at the 6$^{th}$ International Workshop on Relativistic Aspects of Nuclear Physics - Tabatinga - Brazil - October 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0012128
dc.identifierhttp://arxiv.org/abs/astro-ph/0012128
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2170
dc.subjectAstrophysics
dc.titlePotential Sources of Gravitational Wave Emission and Laser Beam Interferometers
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