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dc.contributor.advisorVera Jiménez, Raül ORCID
dc.contributor.authorBorchers Pascual, Ángela
dc.contributor.otherF. CIENCIA Y TECNOLOGIA
dc.contributor.otherZIENTZIA ETA TEKNOLOGIA F.
dc.date.accessioned2020-01-16T18:03:15Z
dc.date.available2020-01-16T18:03:15Z
dc.date.issued2020-01-16
dc.identifier.urihttp://hdl.handle.net/10810/38528
dc.description.abstract[EN] In General Relativity, the causal structure of spherically symmetric spacetime solutions can be studied by the so-called Penrose diagrams. Based on conformal transformations, this technique is used to compactify spacetime manifolds, in order to make its causal relationships more evident. In this work, we review several solutions to Einstein’s equation of gravity, constructing in each case the associated conformal diagram. Different black hole solutions are studied, together with the de Sitter spacetime, a vacuum solution that considers a positive cosmological constant. Eventually, we give an account of the global properties of charged black holes with positive cosmological constant.es_ES
dc.language.isoenges_ES
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/es/
dc.subjectPenrose diagram
dc.subjectSitter spacetime
dc.subjectvacuum solution
dc.subjectblack hole
dc.subjectagujero negro
dc.subjectSitter
dc.subjectPenrose
dc.subjectsolución de vacío
dc.titleGlobal properties of charged black holes with cosmological constantes_ES
dc.typeinfo:eu-repo/semantics/bachelorThesis
dc.date.updated2019-07-19T10:25:12Z
dc.language.rfc3066es
dc.rights.holderAtribución-NoComercial-CompartirIgual (cc by-nc-sa)
dc.identifier.gaurregister98908-796336-11
dc.identifier.gaurassign79820-796336


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