On the stationary axially symmetric Einstein-Weyl field equations

dc.contributor.author	Kolassis, C. A.	en
dc.date.accessioned	2015-11-24T18:39:25Z
dc.date.available	2015-11-24T18:39:25Z
dc.identifier.issn	0305-4470	-
dc.identifier.uri	https://olympias.lib.uoi.gr/jspui/handle/123456789/17440
dc.rights	Default Licence	-
dc.title	On the stationary axially symmetric Einstein-Weyl field equations	en
heal.abstract	The combined gravitational-neutrino field equations in general relativity are solved under the following two assumptions: (i) space-time is stationary axially symmetric and the line element of the metric can be put into a canonical form, (ii) the energy flow vector of the neutrino field is time-like or null for all observers. The resulting metric is uniquely determined and asymptotically non-flat; the Weyl tensor is of Petrov type D, and the Ricci tensor belongs to the class (2T-2S) 2 in the Plebanski classification.	en
heal.access	campus	-
heal.fullTextAvailability	TRUE	-
heal.identifier.secondary	http://stacks.iop.org/0305-4470/16/i=4/a=013	-
heal.journalName	Journal of Physics A: Mathematical and General	en
heal.journalType	peer reviewed	-
heal.publicationDate	1983	-
heal.recordProvider	Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών	el
heal.type	journalArticle	-
heal.type.el	Άρθρο Περιοδικού	el
heal.type.en	Journal article	en

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