Boundary conditions in first order gravity: Hamiltonian and ensemble

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dc.contributor.authorAros, R.
dc.date.accessioned2023-03-27T18:54:29Z
dc.date.available2023-03-27T18:54:29Z
dc.date.issued2006-01
dc.descriptionIndexación: Scopus.
dc.description.abstractIn this work two different boundary conditions for first order gravity, corresponding to a null and a negative cosmological constant, respectively, are studied. Both boundary conditions allow one to obtain the standard black hole thermodynamics. Furthermore, both boundary conditions define a canonical ensemble. Additionally the quasilocal energy definition is obtained for the null cosmological constant case.es
dc.description.urihttps://journals-aps-org.recursosbiblioteca.unab.cl/prd/abstract/10.1103/PhysRevD.73.024004
dc.identifier.citationPhysical Review D - Particles, Fields, Gravitation and Cosmology, Volume 73, Issue 215, January 2006, Article number 024004es
dc.identifier.doi10.1103/PhysRevD.73.024004
dc.identifier.issn1550-7998
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/47925
dc.language.isoenes
dc.publisherAmerican Physical Societyes
dc.rights.licenseAttribution 4.0 International (CC BY 4.0)
dc.rights.urihttps://journals-aps-org.recursosbiblioteca.unab.cl/prd/about
dc.subjectSupergravityes
dc.subjectGravitationes
dc.subjectBlack Holeses
dc.titleBoundary conditions in first order gravity: Hamiltonian and ensemblees
dc.typeArtículoes
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