Topological Roots of Black Hole Entropy

Simple item page
dc.creatorTeitelboim, C.
dc.date1994-05-31
dc.date.accessioned2026-07-07T04:20:14Z
dc.date.available2026-07-07T04:20:14Z
dc.descriptionWe review the insights into black hole entropy that arise from the formulation of gravitation theory in terms of dimensional continuation. The role of the horizon area and the deficit angle of a conical singularity at the horizon as canonically conjugate dynamical variables is analyzed. The path integral and the extension of the Wheeler-De Witt equation for black holes are discussed.
dc.description11 pages, no figures, use latex, IASSNS-HEP 93/35
dc.identifierhttps://arxiv.org/abs/hep-th/9405199
dc.identifierhttp://arxiv.org/abs/hep-th/9405199
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53882
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTopological Roots of Black Hole Entropy
dc.typetext

Files

Collections

arXiv