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2012

Quasinormal modes of regular black holes

Flachi, Antonino, Lemos, José P. S.

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Black hole quasinormal frequencies are complex numbers that encode information on how a black hole relaxes after it has been perturbed and depend on the features of the geometry and on the type of perturbations.

On the one hand, the examples studied so far in the literature focused on the case of black hole geometries with singularities in their interior.
On the other hand, it is expected that quantum or classical modifications of general relativity may correct the pathological singular behavior of classical black hole solutions.
Despite the fact that we do not have at hand a complete theory of quantum gravity, regular black hole solutions can be constructed by coupling gravity to an external form of matter, sometimes modeled by one form or another of nonlinear electrodynamics.

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