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dc.contributor.authorAdami, H.
dc.contributor.authorConcha Aguilera, Patrick
dc.contributor.authorRodriguez, E.
dc.contributor.authorSafari, H. R.
dc.date.accessioned2021-08-17T23:52:39Z
dc.date.available2021-08-17T23:52:39Z
dc.date.issued2020-10-19
dc.identifier.citationThe European Physical Journal C, Volume 80, Issue 10es_CL
dc.identifier.issn1434-6052
dc.identifier.urihttp://repositoriodigital.ucsc.cl/handle/25022009/2351
dc.descriptionArtículo de publicación ISIes_CL
dc.description.abstractWe present a three-dimensional Chern–Simons gravity based on a deformation of the Maxwell algebra. This symmetry allows introduction of a non-vanishing torsion to the Maxwell Chern–Simons theory, whose action recovers the Mielke–Baekler model for particular values of the coupling constants. By considering suitable boundary conditions, we show that the asymptotic symmetry is given by the bmsˆ3⊕vir algebra with three independent central charges.es_CL
dc.language.isoenes_CL
dc.publisherThe European Physical Journal Ces_CL
dc.source.urihttps://doi.org/10.1140/epjc/s10052-020-08537-z
dc.subjectGeneral relativityes_CL
dc.subjectBlack-holees_CL
dc.subject3Des_CL
dc.subjectGravityes_CL
dc.subjectSupergravityes_CL
dc.subjectFieldes_CL
dc.subjectFomulationes_CL
dc.subjectExtensiones_CL
dc.subjectParticleses_CL
dc.subjectChargeses_CL
dc.subjectLimites_CL
dc.titleAsymptotic symmetries of Maxwell Chern–Simons gravity with torsiones_CL
dc.typeArticlees_CL
dc.identifier.doi/10.1140/epjc/s10052-020-08537-z


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