Space-time symmetries and the gravitational-neutrino field equations in general relativity

dc.contributor.authorKolassis, Charalampos A.en
dc.date.accessioned2015-11-24T18:35:13Z
dc.date.available2015-11-24T18:35:13Z
dc.identifier.issn0375-9601-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17064
dc.rightsDefault Licence-
dc.titleSpace-time symmetries and the gravitational-neutrino field equations in general relativityen
heal.abstractWe consider a neutrino field with geodesic rays in interaction with a gravitational field admitting a Killing vector field nμ. It is found that for solutions of the Einstein-Weyl field equations the neutrino field ξA and the neutrino flux vector lμ are restricted by the equations: LnξA = ?12 is ξA and Lnlμ = 0, whereas s is a real constant. In the case of pure radiation neutrino fields these equations become: LξA = case12(p ? is)ξA, Lnlμ = plμ, where p and s are in general real functions of the coordinates.en
heal.accesscampus-
heal.fullTextAvailabilityTRUE-
heal.identifier.primaryhttp://dx.doi.org/10.1016/0375-9601(83)90145-7-
heal.identifier.secondaryhttp://www.sciencedirect.com/science/article/pii/0375960183901457-
heal.journalNamePhysics Letters Aen
heal.journalTypepeer reviewed-
heal.publicationDate1983-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.typejournalArticle-
heal.type.elΆρθρο Περιοδικούel
heal.type.enJournal articleen

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