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dc.contributor.authorMars, Marc
dc.contributor.authorPaetz, Tim-Torben
dc.contributor.authorMartín Senovilla, José María ORCID
dc.contributor.authorSimon, Walter
dc.date.accessioned2018-03-05T12:15:10Z
dc.date.available2018-03-05T12:15:10Z
dc.date.issued2016-08-04
dc.identifier.citationClassical and Quantum Gravityes_ES
dc.identifier.issn0264-9381
dc.identifier.issn1361-6382
dc.identifier.urihttp://hdl.handle.net/10810/25463
dc.description.abstractWe investigate solutions(M, g) to Einstein's vacuum field equations with positive cosmological constant. which admit a smooth past null infinity J(-) a la Penrose and a Killing vector field whose associated Mars-Simon tensor (MST) vanishes. The main purpose of this work is to provide a characterization of these spacetimes in terms of their Cauchy data on J(-). Along the way, we also study spacetimes for which the MST does not vanish. In that case there is an ambiguity in its definition which is captured by a scalar function Q. We analyze properties of the MST for different choices of Q. In doing so, we are led to a definition of 'asymptotically Kerr-de Sitter-like spacetimes', which we also characterize in terms of their asymptotic data on J(-).es_ES
dc.description.sponsorshipMM acknowledges financial support under the projects FIS2012-30926, FIS2015-65140-P (Spanish MINECO-fondos FEDER) and P09-FQM-4496 (J Andalucia-FEDER). TTP acknowledges financial support by the Austrian Science Fund (FWF): P 24170-N16. JMMS is supported under grant FIS2014-57956-P (Spanish MINECO-fondos FEDER), GIU12/15 (Gobierno Vasco), UFI 11/55 (UPV/EHU) and by project P09-FQM-4496 (J Andalucia-FEDER). The research of WS was funded by the Austrian Science Fund (FWF): P 23337-N16.es_ES
dc.language.isoenges_ES
dc.publisherIOP Publishinges_ES
dc.relationinfo:eu-repo/grantAgreement/MINECO/FIS2012-30926es_ES
dc.relationinfo:eu-repo/grantAgreement/MINECO/FIS2015-65140-Pes_ES
dc.relationinfo:eu-repo/grantAgreement/MINECO/FIS2014-57956-Pes_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectcharacterizationes_ES
dc.subjectKerr-de Sitter-likees_ES
dc.subjectcosmological constantes_ES
dc.subjectnull infinityes_ES
dc.subjectMars-Simon tensores_ES
dc.subjectsymmetric hyperbolic systemses_ES
dc.subjectfield-equationses_ES
dc.subjectEinsteines_ES
dc.subjectuniquenesses_ES
dc.subjectexistencees_ES
dc.subjectsmoothes_ES
dc.titleCharacterization of (asymptotically) Kerr–de Sitter-like spacetimes at null infinity*es_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holderOriginal content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.es_ES
dc.rights.holderAtribución 3.0 España*
dc.relation.publisherversionhttp://iopscience.iop.org/article/10.1088/0264-9381/33/15/155001/metaes_ES
dc.identifier.doi10.1088/0264-9381/33/15/155001
dc.departamentoesFísica teórica e historia de la cienciaes_ES
dc.departamentoeuFisika teorikoa eta zientziaren historiaes_ES


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Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
Except where otherwise noted, this item's license is described as Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.