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Quantum Gravity Effects in Rotating Black Holes

M. Reuter, E. Tuiran

hep-tharXiv:hep-th/0612037

Abstract

A set of features of the renormalization group improved Kerr spacetime taking into account the running of Newton's constant is presented. This set includes: Behavior of the critical surfaces and corrections to the mass and angular momentum of the Kerr black hole.

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