Quasinormal modes of black holes in a toy-model for cumulative quantum gravity
arXiv:1906.00603 · doi:10.1016/j.physletb.2019.06.033
Abstract
The idea that quantum gravity effects might leak outside the horizon of a black hole has recently been intensively considered. In this study, we calculate the quasinormal modes as a function of the location and amplitude of a generic metric perturbation distorting to the Schwarzschild spacetime. We conclude on the possible observability of quantum metric corrections by current and future gravitational wave experiments.
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