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

dc.creatorBañados, Máximo
dc.creatorTeitelboim, Claudio
dc.creatorZanelli, Jorge
dc.date1993-09-25
dc.date.accessioned2026-07-07T12:33:13Z
dc.date.available2026-07-07T12:33:13Z
dc.descriptionThe Euclidean black hole has topology $\Re^2 \times {\cal S}^{d-2}$. It is shown that -in Einstein's theory- the deficit angle of a cusp at any point in $\Re^2$ and the area of the ${\cal S}^{d-2}$ 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 ${\cal S}^{d-2}$ 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.
dc.description7 pages, RevTex
dc.identifierhttps://arxiv.org/abs/gr-qc/9309026
dc.identifierhttp://arxiv.org/abs/gr-qc/9309026
dc.identifierPhys.Rev.Lett.72:957-960,1994
dc.identifierdoi:10.1103/PhysRevLett.72.957
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/217049
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack Hole Entropy and the Dimensional Continuation of the Gauss-Bonnet Theorem
dc.typetext

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