Gravitational spectrum of black holes in the Einstein-Aether theory

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dc.creatorKonoplya, R. A.
dc.creatorZhidenko, A.
dc.date2006-11-21
dc.date2007-01-15
dc.date.accessioned2026-07-07T11:02:59Z
dc.date.available2026-07-07T11:02:59Z
dc.descriptionEvolution of gravitational perturbations, both in time and frequency domains, is considered for a spherically symmetric black hole in the non-reduced Einstein-Aether theory. It is shown that real oscillation frequency and damping rate are larger for the Einstein-Aether black hole than for the Schwarzschild black hole. This may provide an opportunity to observe aether in the forthcoming experiments with new generation of gravitational antennas.
dc.description4 pages, RevTex, to be published in Phys. Lett. B
dc.identifierhttps://arxiv.org/abs/hep-th/0611226
dc.identifierhttp://arxiv.org/abs/hep-th/0611226
dc.identifierPhys.Lett.B648:236-239,2007
dc.identifierdoi:10.1016/j.physletb.2007.03.018
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188440
dc.subjectHigh Energy Physics - Theory
dc.titleGravitational spectrum of black holes in the Einstein-Aether theory
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