Motion in bimetric type theories of gravity

dc.AffiliationOctober University for modern sciences and Arts (MSA)
dc.contributor.authorKahil M.E.
dc.contributor.otherOctober University for Modern Sciences and Arts MSA
dc.date.accessioned2020-01-09T20:41:25Z
dc.date.available2020-01-09T20:41:25Z
dc.date.issued17-2-2015
dc.descriptionSJR 2025 0.438 Q3 H-Index 26 Subject Area and Category: Physics and Astronomy Astronomy and Astrophysics
dc.description.abstractThe 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.urihttps://www.scimagojr.com/journalsearch.php?q=17600155002&tip=sid&clean=0
dc.identifier.citationKahil, 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.doihttps://doi.org/10.1134/S0202289317010066
dc.identifier.issn2022893
dc.identifier.otherhttps://doi.org/10.1134/S0202289317010066
dc.identifier.urihttps://t.ly/7OGMJ
dc.language.isoEnglishen_US
dc.publisherPleiades Publishingen_US
dc.relation.ispartofseriesGravitation and Cosmology ; 23(1)
dc.subjectGeneral Relativity and Quantum Cosmology; High Energy Physics ; Theory
dc.titleMotion in bimetric type theories of gravityen_US
dc.typeArticleen_US
dcterms.sourceScopus

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