Thermodynamics of black holes in $(n+1)$-dimensional Einstein-Born-Infeld dilaton gravity

Simple item page
dc.creatorSheykhi, A.
dc.creatorRiazi, N.
dc.date2006-10-08
dc.date.accessioned2026-07-07T10:26:06Z
dc.date.available2026-07-07T10:26:06Z
dc.descriptionWe construct a new class of $(n+1)$-dimensional $(n\geq3)$ black hole solutions in Einstein-Born-Infeld-dilaton gravity with Liouville-type potential for the dilaton field and investigate their properties. These solutions are neither asymptotically flat nor (anti)-de Sitter. We find that these solutions can represent black holes, with inner and outer event horizons, an extreme black hole or a naked singularity provided the parameters of the solutions are chosen suitably. We compute the thermodynamic quantities of the black hole solutions and find that these quantities satisfy the first law of thermodynamics. We also perform stability analysis and investigate the effect of dilaton on the stability of the solutions.
dc.description18 pages, 15 figures
dc.identifierhttps://arxiv.org/abs/hep-th/0610085
dc.identifierhttp://arxiv.org/abs/hep-th/0610085
dc.identifierPhys.Rev.D75:024021,2007
dc.identifierdoi:10.1103/PhysRevD.75.024021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176762
dc.subjectHigh Energy Physics - Theory
dc.titleThermodynamics of black holes in $(n+1)$-dimensional Einstein-Born-Infeld dilaton gravity
dc.typetext

Files

Collections

arXiv