Charged Black Hole in a Canonical Ensemble

dc.creatorLundgren, Andrew P.
dc.date2006-12-19
dc.date.accessioned2026-07-07T11:21:36Z
dc.date.available2026-07-07T11:21:36Z
dc.descriptionWe consider the thermodynamics of a charged black hole enclosed in a cavity. The charge in the cavity and the temperature at the walls are fixed so that we have a canonical ensemble. We derive the phase structure and stability of black hole equilibrium states. We compare our results to that of other work which uses asymptotically anti-de Sitter boundary conditions to define the thermodynamics. The thermodynamic properties have extensive similarities which suggest that the idea of AdS holography is more dependent on the existence of the boundary than on the exact details of asymptotically AdS metrics.
dc.description9 pages; 4 multipart figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0612119
dc.identifierhttp://arxiv.org/abs/gr-qc/0612119
dc.identifierPhys.Rev.D77:044014,2008
dc.identifierdoi:10.1103/PhysRevD.77.044014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194312
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCharged Black Hole in a Canonical Ensemble
dc.typetext

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