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| DC Field | Value | Language |
|---|---|---|
| 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.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.secondary | http://stacks.iop.org/0305-4470/16/i=4/a=013 | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 1983 | - |
| 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.journalName | Journal of Physics A: Mathematical and General | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| kolassis-1983-On the stationary axially symmetric Einstein-Weyl field equations.pdf | 713.57 kB | Adobe PDF | View/Open Request a copy |
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