Quasinormal Modes of Maximally Charged RN Black Holes and the Search for a Quantum Theory of Gravity
نویسنده
چکیده
In the context of searching for a quantum theory of gravity, the quasinormal modes of black holes has become a promising area of study that may link a quantum theory of gravity with classical general relativity. Of special interest are the asymptotic real values of the quasinormal frequencies, which have recently been shown to converge to an analytically predicted value. In this paper, we will review the development of the analytical formula for the Schwarzchild case, and then show how that formula fails to agree with numerical results in the case of maximally charged Reissner-Nordström black holes. We conclude with an outlook on possible results of further study.
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