http://arxiv.org/abs/1906.00603
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.
A. Barrau, K. Martineau, J. Martinon, et. al.
Tue, 4 Jun 19
69/71
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