Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/16074
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dc.contributor.authorKanti, P.en
dc.contributor.authorVayonakis, C. E.en
dc.date.accessioned2015-11-24T18:27:41Z-
dc.date.available2015-11-24T18:27:41Z-
dc.identifier.issn0556-2821-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16074-
dc.rightsDefault Licence-
dc.subjecthomogeneous space-timesen
dc.titleGodel-type universes in string-inspired charged gravityen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://000083862300024-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1999-
heal.abstractWe consider a string-inspired, gravitational theory of scalar and electromagnetic fields and eve investigate the existence of axially symmetric, Godel-type cosmological solutions. The neutral ease is studied first and an "extreme" Godel-type rotating solution, which respects the causality, is determined. The charged case is considered next and two new configurations, minimally coupled to gravity, are presented, for the electromagnetic field. Another configuration motivated by the expected distribution of currents and charges in a rotating universe is studied and shown to lead to a Godel-type solution for a space-dependent coupling function. Finally, we investigate the existence of Godel-type cosmological solutions in the framework of the one-loop corrected superstring effective action and we determine the sole configuration of the electromagnetic field that leads to such a solution. It turns out that, in all the charged cases considered, closed timelike curves do appear and the causality is always violated. [S0556-2821(99)06920-9].en
heal.journalNamePhysical Review Den
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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