Spinning and spinning deviation equations of bi-metric type theories

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dc.AffiliationOctober University for modern sciences and Arts (MSA)
dc.contributor.authorKahil, Magd E
dc.date.accessioned2020-07-20T14:58:29Z
dc.date.available2020-07-20T14:58:29Z
dc.date.issued7/15/2020
dc.descriptionSCOPUSen_US
dc.description.abstractSpinning equations of bi-metric type theories of gravity, the counterpart of the Papapetrou equations of motion are derived as well as their corresponding spinning deviation equations, by means of introducing different types of bi-metric theories. The influence of different curvatures based on different connections is illustrated. A specific Lagrangian function for each type theory is proposed, in order to derive the set of spinning motion and their corresponding spinning deviation equations.en_US
dc.description.urihttps://www.scimagojr.com/journalsearch.php?q=145208&tip=sid&clean=0
dc.identifier.issnhttps://doi.org/10.1007/s12648-020-01793-5
dc.identifier.urihttps://t.ly/vvqo
dc.language.isoen_USen_US
dc.publisherSpringeren_US
dc.relation.ispartofseriesIndian Journal of Physics;2020
dc.subjectSpinning deviationen_US
dc.subjectSpinning equationsen_US
dc.subjectGeodesic deviationen_US
dc.subjectBi-metricen_US
dc.subjectGeodesicen_US
dc.titleSpinning and spinning deviation equations of bi-metric type theoriesen_US
dc.typeArticleen_US

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