Quantum Gravity Effects in Rotating Black Holes
arXiv: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.
4 pages, 1 figure, to appear in the proceedings of the 11th Marcel Grossmann Meeting (Berlin 2006), latex