Thermodynamics of rotating black branes in $(n+1)$-dimensional Einstein-Born-Infeld gravity
| dc.creator | Dehghani, M. H. | |
| dc.creator | Sedehi, H. R. Rastegar | |
| dc.date | 2006-10-23 | |
| dc.date.accessioned | 2026-07-07T11:28:04Z | |
| dc.date.available | 2026-07-07T11:28:04Z | |
| dc.description | We construct a new class of charged rotating solutions of $(n+1)$-dimensional Einstein-Born-Infeld gravity with cylindrical or toroidal horizons in the presence of cosmological constant and investigate their properties. These solutions are asymptotically (anti)-de Sitter and reduce to the solutions of Einstein-Maxwell gravity as the Born-Infeld parameters goes to infinity. We find that these solutions can represent black branes, with inner and outer event horizons, an extreme black brane or a naked singularity provided the parameters of the solutions are chosen suitably. We compute temperature, mass, angular momentum, entropy, charge and electric potential of the black brane solutions. We obtain a Smarr-type formula and show that these quantities satisfy the first law of thermodynamics. We also perform a stability analysis by computing the heat capacity and the determinant of Hessian matrix of mass with respect to its thermodynamic variables in both the canonical and the grand-canonical ensembles, and show that the system is thermally stable in the whole phase space. | |
| dc.description | 12 pages, one figure | |
| dc.identifier | https://arxiv.org/abs/hep-th/0610239 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0610239 | |
| dc.identifier | Phys.Rev.D74:124018,2006 | |
| dc.identifier | doi:10.1103/PhysRevD.74.124018 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/196325 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Thermodynamics of rotating black branes in $(n+1)$-dimensional Einstein-Born-Infeld gravity | |
| dc.type | text |