Quasi-Normal Modes and Gravitational Wave Astronomy

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dc.creatorFerrari, V.
dc.creatorGualtieri, L.
dc.date2007-09-05
dc.date2008-01-11
dc.date.accessioned2026-07-07T11:19:07Z
dc.date.available2026-07-07T11:19:07Z
dc.descriptionWe review the main results obtained in the literature on quasi-normal modes of compact stars and black holes, in the light of recent exciting developments of gravitational wave detectors. Quasi-normal modes are a fundamental feature of the gravitational signal emitted by compact objects in many astrophysical processes; we will show that their eigenfrequencies encode interesting information on the nature and on the inner structure of the emitting source and we will discuss whether we are ready for a gravitational wave asteroseismology.
dc.description25 pages, 7 figures, to appear on Gen. Rel. Grav
dc.identifierhttps://arxiv.org/abs/0709.0657
dc.identifierhttp://arxiv.org/abs/0709.0657
dc.identifierGen.Rel.Grav.40:945-970,2008
dc.identifierdoi:10.1007/s10714-007-0585-1
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193572
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleQuasi-Normal Modes and Gravitational Wave Astronomy
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