Rotating Relativistic Thin Disks as Sources of the Taub-NUT Solution

dc.creatorGonzález, Guillermo A.
dc.date2002-06-06
dc.date.accessioned2022-03-14T20:23:05Z
dc.date.available2022-03-14T20:23:05Z
dc.descriptionRotating disks with nonzero radial pressure and finite radius are studied. The models are based in the Taub-NUT metric and cons-tructed using the well-known "displace, cut and reflect" method. We find that the disks are made of perfect fluids with constant energy density and pressure. The energy density is negative, but the effective Newto-nian density is possitive as the strong energy condition requires. We also find that the disks are not stable under radial perturbations and that there are regions of the disks where the particles move with superluminal velocities.   es-ES
dc.formatapplication/pdf
dc.identifierhttps://revistas.uis.edu.co/index.php/revistaintegracion/article/view/732
dc.identifier.urihttps://noesis.uis.edu.co/handle/20.500.14071/7101
dc.languagespa
dc.publisherUniversidad Industrial de Santanderes-ES
dc.relationhttps://revistas.uis.edu.co/index.php/revistaintegracion/article/view/732/1021
dc.rights.accessrightsinfo:eu-repo/semantics/openAccess
dc.rights.coarhttp://purl.org/coar/access_right/c_abf2
dc.rights.creativecommonsAtribución-NoComercial-SinDerivadas 4.0 Internacional (CC BY-NC-ND 4.0)
dc.rights.licenseAttribution-NonCommercial 4.0 International (CC BY-NC 4.0)
dc.sourceRevista integración, temas de matemáticas; Vol. 20 Núm. 1 y 2 (2002): Revista Integración, temas de matemáticas; 13-17es-ES
dc.sourceREVISTA INTEGRACIÓN; v. 20 n. 1 y 2 (2002): Revista Integración, temas de matemáticas; 13-17pt-BR
dc.source2145-8472
dc.source0120-419X
dc.subjectTaub-NUT metrices-ES
dc.subjectNewotnian densityes-ES
dc.subjectgeneral relativityes-ES
dc.titleRotating Relativistic Thin Disks as Sources of the Taub-NUT Solutiones-ES
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion
dspace.entity.type
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