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dc.contributor.authorKolassis, C.en
dc.contributor.authorGriffiths, J. B.en
dc.date.accessioned2015-11-24T18:39:13Z-
dc.date.available2015-11-24T18:39:13Z-
dc.identifier.issn0001-7701-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17404-
dc.rightsDefault Licence-
dc.subjectsimilar cosmological modelsen
dc.subjectqualitative-analysisen
dc.subjecttetraden
dc.titlePerfect fluid space-times with a two-dimensional orthogonally transitive group of homothetic motionsen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://A1996UW01400003-
heal.identifier.secondaryhttp://www.springerlink.com/content/r548k57542481405/fulltext.pdf-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1996-
heal.abstractWe use the GHP formalism to obtain perfect fluid space-times with a two-dimensional and orthogonally transitive group of proper homothetic motions H-2, with the additional condition that the four-velocity of the fluid either lies on the group orbits or is orthogonal to them. In the first case the orbits of the H-2 are timelike and all possible solutions are explicitly given. They comprise (i) space-times of Petrov type I that admit a group H-3 containing two hypersurface orthogonal and commuting Killing vectors (when the H-2 is abelian, the fluid has a stiff equation of state and the space-time is of type D), and (ii) a class of type D static space-times with a maximal H-2 in which the two-spaces orthogonal to the group orbits have constant curvature. When the orbits of the H-2 are spacelike, the fluid is necessarily stiff and different classes of solutions admitting maximal H-2 and H-3 are identified.en
heal.journalNameGeneral Relativity and Gravitationen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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