dc.creatorGutiérrez-Piñeres A.C.
dc.creatorLopez-Monsalvo C.S.
dc.creatorQuevedo H.
dc.date.accessioned2020-03-26T16:32:45Z
dc.date.accessioned2022-09-28T20:10:32Z
dc.date.available2020-03-26T16:32:45Z
dc.date.available2022-09-28T20:10:32Z
dc.date.created2020-03-26T16:32:45Z
dc.date.issued2015
dc.identifierGeneral Relativity and Gravitation; Vol. 47, Núm. 12; pp. 1-9
dc.identifier00017701
dc.identifierhttps://hdl.handle.net/20.500.12585/9010
dc.identifier10.1007/s10714-015-1972-7
dc.identifierUniversidad Tecnológica de Bolívar
dc.identifierRepositorio UTB
dc.identifier25225467000
dc.identifier56013682900
dc.identifier55989741100
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3721688
dc.description.abstractWe present a relativistic model describing a thin disk system composed of two fluids. The system is surrounded by a halo in the presence of a non-trivial electromagnetic field. We show that the model is compatible with the variational multifluid thermodynamics formalism, allowing us to determine all the thermodynamic variables associated with the matter content of the disk. The asymptotic behavior of these quantities indicates that the single fluid interpretation should be abandoned in favor of a two-fluid model. © 2015, Springer Science+Business Media New York.
dc.languageeng
dc.publisherSpringer New York LLC
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-s2.0-84946575429&doi=10.1007%2fs10714-015-1972-7&partnerID=40&md5=d4ef9b1f45f41ea5fa48a9871af153ea
dc.titleVariational thermodynamics of relativistic thin disks


Este ítem pertenece a la siguiente institución