Vacuum solutions with nontrivial boundaries for the Einstein-Gauss-Bonnet theory

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dc.creatorDotti, Gustavo
dc.creatorOliva, Julio
dc.creatorTroncoso, Ricardo
dc.date2008-09-25
dc.date2008-09-30
dc.date.accessioned2026-07-07T13:07:34Z
dc.date.available2026-07-07T13:07:34Z
dc.descriptionThe classification of certain class of static solutions for the Einstein-Gauss-Bonnet theory in vacuum is presented. The spacelike section of the class of metrics under consideration is a warped product of the real line with a nontrivial base manifold. For arbitrary values of the Gauss-Bonnet coupling, the base manifold must be Einstein with an additional scalar restriction. The geometry of the boundary can be relaxed only when the Gauss-Bonnet coupling is related with the cosmological and Newton constants, so that the theory admits a unique maximally symmetric solution. This additional freedom in the boundary metric allows the existence of three main branches of geometries in the bulk, containing new black holes and wormholes in vacuum.
dc.descriptionPrepared for the proceedings of the 7th Alexander Friedmann International Seminar on Gravitation and Cosmology, July 2008, Joao Pessoa, Brasil. 4 pages, References added
dc.identifierhttps://arxiv.org/abs/0809.4378
dc.identifierhttp://arxiv.org/abs/0809.4378
dc.identifierInt.J.Mod.Phys.A24:1690-1694,2009
dc.identifierdoi:10.1142/S0217751X09045248
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/228133
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleVacuum solutions with nontrivial boundaries for the Einstein-Gauss-Bonnet theory
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