Thermodynamics of rotating solutions in (n+1)-dimensional Einstein-Maxwell-dilaton gravity

Simple item page
dc.creatorSheykhi, A.
dc.creatorDehghani, M. H.
dc.creatorRiazi, N.
dc.creatorPakravan, J.
dc.date2006-06-25
dc.date2006-07-01
dc.date.accessioned2026-07-07T11:06:44Z
dc.date.available2026-07-07T11:06:44Z
dc.descriptionWe construct a class of charged, rotating solutions of (n+1)-dimensional Einstein-Maxwell-dilaton gravity with Liouville-type potentials and investigate their properties. These solutions are neither asymptotically flat nor (anti)-de Sitter. We find that these solutions can represent black brane, with two inner and outer event horizons, an extreme black brane or a naked singularity provided the parameters of the solutions are chosen suitably. We also compute temperature, entropy, charge, electric potential, mass and angular momentum of the black brane solutions, and find that these quantities satisfy the first law of thermodynamics. We find a Smarr-type formula and perform a stability analysis by computing the heat capacity in the canonical ensemble. We find that the system is thermally stable for alpha <1, while for alpha >1 the system has an unstable phase. This is incommensurate with the fact that there is no Hawking-Page phase transition for black objects with zero curvature horizon.
dc.description15 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/hep-th/0606237
dc.identifierhttp://arxiv.org/abs/hep-th/0606237
dc.identifierPhys.Rev.D74:084016,2006
dc.identifierdoi:10.1103/PhysRevD.74.084016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/189619
dc.subjectHigh Energy Physics - Theory
dc.titleThermodynamics of rotating solutions in (n+1)-dimensional Einstein-Maxwell-dilaton gravity
dc.typetext

Files

Collections

arXiv