Relativistic generalization of the inertial and gravitational masses equivalence principle

dc.creatorMitskievich, Nikolai V.
dc.date2006-11-03
dc.date.accessioned2026-07-07T07:31:54Z
dc.date.available2026-07-07T07:31:54Z
dc.descriptionThe Newtonian approximation for the gravitational field equation should not necessarily involve admission of non-relativistic properties of the source terms in Einstein's equations: it is sufficient to merely consider the weak-field condition for gravitational field. When a source has electromagnetic nature, one simply {\em cannot} ignore its intrinsically relativistic properties, since there cannot be invented any non-relativistic approximation which would describe electromagnetic stress-energy tensor adequately, even at large distances where the fields become naturally weak. But the test particle on which gravitational field is acting, should be treated as non-relativistic (this premise is required for introduction of the Newtonian potential $Φ_{\rm N}$ from the geodesic equation).
dc.description5 pages, a talk delivered at the 11th Marcel Grossmann Meeting (Session GT4), Berlin, 2006
dc.identifierhttps://arxiv.org/abs/gr-qc/0611017
dc.identifierhttp://arxiv.org/abs/gr-qc/0611017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118919
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRelativistic generalization of the inertial and gravitational masses equivalence principle
dc.typetext

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