Motion in bimetric type theories of gravity
| dc.Affiliation | October University for modern sciences and Arts (MSA) | |
| dc.contributor.author | Kahil M.E. | |
| dc.contributor.other | October University for Modern Sciences and Arts | |
| dc.contributor.other | Giza | |
| dc.contributor.other | Egypt; Egyptian Relativity Group | |
| dc.contributor.other | Cairo | |
| dc.contributor.other | Egypt | |
| dc.date.accessioned | 2020-01-09T20:41:25Z | |
| dc.date.available | 2020-01-09T20:41:25Z | |
| dc.date.issued | 2017 | |
| dc.description | Scopus | |
| dc.description.abstract | The problem of motion of different test particles, charged and spinning objects with a constant spin tensor in different versions of the bimetric theory of gravity is considered by deriving their corresponding path and path deviation equations using a modified Bazanski Lagrangian. Such a Lagrangian, as in the framework of Riemannian geometry, has a capability to obtain path and path deviations of any object simultaneously. This method enables us to derive the path and path deviation equations of different objects orbiting in very strong gravitational fields. 2017, Pleiades Publishing, Ltd. | en_US |
| dc.description.uri | https://www.scimagojr.com/journalsearch.php?q=17600155002&tip=sid&clean=0 | |
| dc.identifier.doi | https://doi.org/10.1134/S0202289317010066 | |
| dc.identifier.doi | PubMed ID : | |
| dc.identifier.issn | 2022893 | |
| dc.identifier.other | https://doi.org/10.1134/S0202289317010066 | |
| dc.identifier.other | PubMed ID : | |
| dc.identifier.uri | https://t.ly/7OGMJ | |
| dc.language.iso | English | en_US |
| dc.publisher | Maik Nauka Publishing / Springer SBM | en_US |
| dc.relation.ispartofseries | Gravitation and Cosmology | |
| dc.relation.ispartofseries | 23 | |
| dc.title | Motion in bimetric type theories of gravity | en_US |
| dc.type | Article | en_US |
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| dcterms.source | Scopus |