paper

New attractor mechanism for spherically symmetric extremal black holes

arXiv:0707.1933 · doi:10.1103/PhysRevD.76.104045

Abstract

We introduce a new attractor mechanism to find the entropy for spherically symmetric extremal black holes. The key ingredient is to find a two-dimensional (2D) dilaton gravity with the dilaton potential . The condition of an attractor is given by and and for a constant dilaton , these are also used to find the location of the degenerate horizon of an extremal black hole. As a nontrivial example, we consider an extremal regular black hole obtained from the coupled system of Einstein gravity and nonlinear electrodynamics. The desired Bekenstein-Hawking entropy is successfully recovered from the generalized entropy formula combined with the 2D dilaton gravity, while the entropy function approach does not work for obtaining this entropy.

20 pages, 4 figures, Accepted for publication in Physical Review D. This version includes revisions suggested by the referee

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