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| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Kolassis, Charalampos A. | en |
| dc.date.accessioned | 2015-11-24T18:35:13Z | - |
| dc.date.available | 2015-11-24T18:35:13Z | - |
| dc.identifier.issn | 0375-9601 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/17064 | - |
| dc.rights | Default Licence | - |
| dc.title | Space-time symmetries and the gravitational-neutrino field equations in general relativity | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.primary | http://dx.doi.org/10.1016/0375-9601(83)90145-7 | - |
| heal.identifier.secondary | http://www.sciencedirect.com/science/article/pii/0375960183901457 | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 1983 | - |
| heal.abstract | We 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.journalName | Physics Letters A | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) - ΦΥΣ | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| kolassis-1983-Space-time symmetries and the gravitational-neutrino field equations in general relativity.pdf | 149.73 kB | Adobe PDF | View/Open Request a copy |
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