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 MSA | |
| dc.date.accessioned | 2020-01-09T20:41:25Z | |
| dc.date.available | 2020-01-09T20:41:25Z | |
| dc.date.issued | 17-2-2015 | |
| dc.description | SJR 2025 0.438 Q3 H-Index 26 Subject Area and Category: Physics and Astronomy Astronomy and Astrophysics | |
| 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. | en_US |
| dc.description.uri | https://www.scimagojr.com/journalsearch.php?q=17600155002&tip=sid&clean=0 | |
| dc.identifier.citation | Kahil, M. E. (2017). Motion in bimetric type theories of gravity. Gravitation and Cosmology, 23(1), 70–79. https://doi.org/10.1134/s0202289317010066 | |
| dc.identifier.doi | https://doi.org/10.1134/S0202289317010066 | |
| dc.identifier.issn | 2022893 | |
| dc.identifier.other | https://doi.org/10.1134/S0202289317010066 | |
| dc.identifier.uri | https://t.ly/7OGMJ | |
| dc.language.iso | English | en_US |
| dc.publisher | Pleiades Publishing | en_US |
| dc.relation.ispartofseries | Gravitation and Cosmology ; 23(1) | |
| dc.subject | General Relativity and Quantum Cosmology; High Energy Physics ; Theory | |
| dc.title | Motion in bimetric type theories of gravity | en_US |
| dc.type | Article | en_US |
| dcterms.source | Scopus |
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