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Black Hole Entropy and the Dimensional Continuation of the Gauss-Bonnet Theorem

Abstract

The Euclidean black hole has topology 2×Sd2\Re^2 \times {\cal S}^{d-2}. It is shown that -in Einstein's theory- the deficit angle of a cusp at any point in 2\Re^2 and the area of the Sd2{\cal S}^{d-2} are canonical conjugates. The black hole entropy emerges as the Euler class of a small disk centered at the horizon multiplied by the area of the Sd2{\cal S}^{d-2} there.These results are obtained through dimensional continuation of the Gauss-Bonnet theorem. The extension to the most general action yielding second order field equations for the metric in any spacetime dimension is given.Comment: 7 pages, RevTe

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    Last time updated on 02/01/2020