Conformastatic disk-haloes in Einstein-Maxwell gravity

dc.creatorGutiérrez-Piñeres A.C.
dc.creatorGonzález G.A.
dc.creatorQuevedo H.
dc.date.accessioned2020-03-26T16:32:54Z
dc.date.accessioned2022-09-28T20:15:02Z
dc.date.available2020-03-26T16:32:54Z
dc.date.available2022-09-28T20:15:02Z
dc.date.created2020-03-26T16:32:54Z
dc.date.issued2013
dc.identifierPhysical Review D - Particles, Fields, Gravitation and Cosmology; Vol. 87, Núm. 4
dc.identifier15507998
dc.identifierhttps://hdl.handle.net/20.500.12585/9078
dc.identifier10.1103/PhysRevD.87.044010
dc.identifierUniversidad Tecnológica de Bolívar
dc.identifierRepositorio UTB
dc.identifier25225467000
dc.identifier7202571265
dc.identifier55989741100
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3723715
dc.description.abstractWe present a relativistic model describing a thin disk surrounded by a halo in the presence of an electromagnetic field. The model is obtained by solving the Einstein-Maxwell equations on a particular conformastatic spacetime background and by using the distributional approach for the energy-momentum tensor. A class of solutions is obtained in which the gravitational and electromagnetic potentials are completely determined by a harmonic function only. A particular solution is given that is asymptotically flat and singularity free, and satisfies all the energy conditions. © 2013 American Physical Society.
dc.languageeng
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.rightsAtribución-NoComercial 4.0 Internacional
dc.sourcehttps://www.scopus.com/inward/record.uri?eid=2-s2.0-84873578551&doi=10.1103%2fPhysRevD.87.044010&partnerID=40&md5=a403049746d91f3e2d43c08ac8e5e923
dc.titleConformastatic disk-haloes in Einstein-Maxwell gravity


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