Gravitating macroscopic media in general relativity
Giovanni Montani (ICRA, University of Rome), Remo Ruffini (ICRA,, University of Roma), Roustam Zalaletdinov (ICRA, Univeristy of Rome and, Institute of Nuclear Physics, Tashkent)

TL;DR
This paper develops a macroscopic gravity model in general relativity, addressing the construction of continuous matter models from microscopic distributions and analyzing the limitations of existing approaches.
Contribution
It introduces a second-order perturbation theory approach to derive macroscopic gravitational field equations incorporating polarization effects.
Findings
Identifies inconsistencies in Szekeres' linearized approach.
Proposes a set of material relations linking polarization tensors and energy-momentum.
Derives a system of macroscopic field equations including polarization effects.
Abstract
The problem of construction of a continuous (macroscopic) matter model for a given point-like (microscopic) matter distribution in general relativity is formulated. The existing approaches are briefly reviewed and a physical analogy with the similar problem in classical macroscopic electrodynamics is pointed out. The procedure by Szekeres in the linearized general relativity on Minkowski background to construct a tensor of gravitational quadruple polarization by applying Kaufman's method of molecular moments for derivation of the polarization tensor in macroscopic electrodynamics and to derive an averaged field operator by utilizing an analogy between the linearized Bianchi identities and Maxwell equations, is analyzed. It is shown that the procedure has some inconsistencies, in particular, (1) it has only provided the terms linear in perturbations for the averaged field operator which…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Black Holes and Theoretical Physics
