A Hamiltonian approach to quantum gravity

dc.creatorStefanovich, Eugene V.
dc.date2006-12-03
dc.date2008-04-02
dc.date.accessioned2026-07-07T09:29:45Z
dc.date.available2026-07-07T09:29:45Z
dc.descriptionWe explore the idea that gravitational interaction can be described by instantaneous inter-particle potentials. This idea is in full accord with relativistic quantum theory. In particular, it resembles the ``dressed particle'' approach to quantum electrodynamics. Although the complete non-perturbative of this theory is yet unknown, one can reasonably guess its form in low perturbation orders and in the (1/c)^2 approximation. We suggest a relativistic energy operator, which in the classical limit reduces to the Einstein-Infeld-Hoffmann Hamiltonian for massive particles and correctly describes the effects of gravity on photons, including the light bending, the Shapiro delay, the gravitational time dilation and the red shift. The causality of this approach is briefly discussed.
dc.description9 pages, 1 figure; v2 and v3 - improved discussion of the principle of equivalence and the gravitational time dilation; v4 - added footnote and a reference; v5 - added discussion of optical clocks; v6 - discussion of the equivalence principle is rewritten; v7 - improved discussion of gravitational time dilation; v8 - multiple improvements; v9 - major revision;
dc.identifierhttps://arxiv.org/abs/physics/0612019
dc.identifierhttp://arxiv.org/abs/physics/0612019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/157902
dc.subjectGeneral Physics
dc.titleA Hamiltonian approach to quantum gravity
dc.typetext

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