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dc.contributor.authorGrammenos, T.en
dc.contributor.authorKolassis, C.en
dc.date.accessioned2015-11-24T18:33:03Z-
dc.date.available2015-11-24T18:33:03Z-
dc.identifier.issn0375-9601-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16681-
dc.rightsDefault Licence-
dc.titleAn Analytic Model of Radiating Spherical Gravitational Collapseen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://A1992JN19900002-
heal.identifier.secondaryhttp://ac.els-cdn.com/037596019290796O/1-s2.0-037596019290796O-main.pdf?_tid=7fe61f6de5dd580996257e2c1d995cf1&acdnat=1334228593_488242b77f1f6a73abe511b3baff3673-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1992-
heal.abstractThe gravitational collapse of a radiating sphere consisting of a heat-conducting fluid with shear-free and radial motion is considered. In the exterior of the sphere we assume Vaidya's outgoing metric, while in the interior we have a neutrino flux described by a pure radiation term in the energy-momentum tensor. At first, a brief review including some new considerations of a similar, previously studied model, is given. Then, a new model is presented, in which the space-time interior to the collapsing sphere is conformally flat.en
heal.journalNamePhysics Letters Aen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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