dc.creatorAlvarado Marín,Rodrigo
dc.creatorAngulo Sibaja,Andrés A.
dc.creatorVargas Obando,Mauricio
dc.date2022-12-01
dc.date.accessioned2023-09-25T14:31:15Z
dc.date.available2023-09-25T14:31:15Z
dc.identifierhttp://www.scielo.sa.cr/scielo.php?script=sci_arttext&pid=S1409-24332022000200225
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8821480
dc.descriptionAbstract In this paper, two exact solutions of the Einstein's equations are obtained for an anisotropic and homogeneous symmetry of Petrov Type D, the difference between both solutions lies in how relevant is the expansión that is presented initially, either on an axis or on a perpendicular plane. Both solutions represent a mixture of two fluids with minimum interaction: dark energy (P = -µ) and radiation (P = µ/3). The singularities and the influence that these fluids have on this metric are studied; the Hubble parameters, the deceleration parameter and the role that these fluids representon them are determined and analyzed. Additionally, their temperatura and the role that both play on this magnitude are determined.
dc.formattext/html
dc.languageen
dc.publisherCentro de Investigaciones en Matemática Pura y Aplicada (CIMPA) y Escuela de Matemática, San José, Costa Rica.
dc.relation10.15517/rmta.v29i2.46390
dc.rightsinfo:eu-repo/semantics/openAccess
dc.sourceRevista de Matemática Teoría y Aplicaciones v.29 n.2 2022
dc.subjectcosmology
dc.subjectexact solution
dc.subjectEinstein
dc.subjecttemperature
dc.subjectHubble
dc.subjectdeceleration parameter
dc.subjectKretschmann
dc.subjectsingularity.
dc.titleCosmological exact solutions of Petrov type D. a mixture of two fluids: dark energy and radiation
dc.typeinfo:eu-repo/semantics/article


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