Gravitational spectrum of black holes in the Einstein-Aether theory

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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4 pages, RevTex, to be published in Phys. Lett. B

Scientific paper

10.1016/j.physletb.2007.03.018

Evolution 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.

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