dc.creatorUjevic, M
dc.creatorLetelier, PS
dc.date2007
dc.dateSEP
dc.date2014-11-18T01:24:01Z
dc.date2015-11-26T16:48:46Z
dc.date2014-11-18T01:24:01Z
dc.date2015-11-26T16:48:46Z
dc.date.accessioned2018-03-28T23:35:16Z
dc.date.available2018-03-28T23:35:16Z
dc.identifierGeneral Relativity And Gravitation. Springer/plenum Publishers, v. 39, n. 9, n. 1345, n. 1365, 2007.
dc.identifier0001-7701
dc.identifierWOS:000248810500004
dc.identifier10.1007/s10714-007-0438-y
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/74487
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/74487
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/74487
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1275242
dc.descriptionWe study the stability of general relativistic static thick disks. As an application we consider the thick disk generated by applying the "displace, cut, fill and reflect" method, usually known as the image method, to the Schwarzschild metric in isotropic coordinates. The isotropic Schwarzschild thick disk obtained from this method is the simplest model to describe, in the context of General Relativity, real thick galaxies. Stability under a general first order perturbation of the disk energy momentum tensor is investigated. The first order perturbation, when applied to the conservation equations, leads to a set of differential equations that have fewer equations than unknowns. In this article we search for perturbations in which the perturbation of the four velocity in a certain direction leads to a pressure perturbation in the same direction. We found that, in general, the isotropic Schwarzschild thick disk is stable under these kinds of perturbations.
dc.description39
dc.description9
dc.description1345
dc.description1365
dc.languageen
dc.publisherSpringer/plenum Publishers
dc.publisherNew York
dc.publisherEUA
dc.relationGeneral Relativity And Gravitation
dc.relationGen. Relativ. Gravit.
dc.rightsfechado
dc.rightshttp://www.springer.com/open+access/authors+rights?SGWID=0-176704-12-683201-0
dc.sourceWeb of Science
dc.subjectBlack-hole
dc.subjectGravitational-field
dc.subjectDust
dc.subjectStationary
dc.subjectModels
dc.subjectMetrics
dc.titleStability of general relativistic static thick disks: the isotropic Schwarzschild thick disk
dc.typeArtículos de revistas


Este ítem pertenece a la siguiente institución