Inhomogeneous cosmologic models with heat flow

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dc.contributor.authorBaysal H.
dc.date.accessioned2019-10-27T09:02:08Z
dc.date.available2019-10-27T09:02:08Z
dc.date.issued1992
dc.departmentEge Üniversitesien_US
dc.description.abstractWe obtain some cosmological models that are exact solutions of Einstein's equations. The metric utilized is the one of Szekeres's class II and the curvature source is a perfect fluid with heat flow. The pressure is assumed to have the form p=c(2 R/RR). © 1992 Kluwer Academic Publishers.en_US
dc.identifier.doi10.1007/BF00692898
dc.identifier.endpage349en_US
dc.identifier.issn0004640X
dc.identifier.issn0004-640Xen_US
dc.identifier.issue2en_US
dc.identifier.scopusqualityQ3en_US
dc.identifier.startpage345en_US
dc.identifier.urihttps://doi.org/10.1007/BF00692898
dc.identifier.urihttps://hdl.handle.net/11454/28327
dc.identifier.volume196en_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherKluwer Academic Publishersen_US
dc.relation.ispartofAstrophysics and Space Scienceen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titleInhomogeneous cosmologic models with heat flowen_US
dc.typeArticleen_US

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