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- W2027298238 abstract "We develop a new method for calculation of quasi-normal modes of black holes, when the effective potential, which governs black hole perturbations, is known only numerically in some region near the black hole. This method can be applied to perturbations of a wide class of numerical black hole solutions. We apply it to the black holes in the Einstein-Aether theory, a theory where general relativity is coupled to a unit time-like vector field, in order to observe local Lorentz symmetry violation. We found that in the non-reduced Einstein-Aether theory, real oscillation frequency and damping rate of quasi-normal modes are larger than those of Schwarzschild black holes in the Einstein theory." @default.
- W2027298238 created "2016-06-24" @default.
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- W2027298238 date "2007-01-01" @default.
- W2027298238 modified "2023-09-27" @default.
- W2027298238 title "Perturbations and quasi-normal modes of black holes in Einstein–Aether theory" @default.
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- W2027298238 doi "https://doi.org/10.1016/j.physletb.2006.11.036" @default.
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