The Ambiguity in the Definition and Behavior of the Gravitational and Cosmological `Coupling Constants' in the Theory of Induced Gravity
Farkhat Zaripov

TL;DR
This paper extends a modified theory of induced gravity, exploring how effective gravitational and cosmological constants fluctuate and relate to dark energy and dark matter, revealing potential deviations from classical gravity at large distances.
Contribution
It introduces a new model (MTIG) with symmetric quadratic potentials, analyzing solutions that connect scalar fields to effective constants and uncovering novel large-distance gravitational effects.
Findings
Effective constants fluctuate near mean values in solutions.
Model matches observational data related to dark energy and dark matter.
New solutions suggest deviations from classical gravity at large scales.
Abstract
This work is the extension of author`s research, where the modified theory of induced gravity (MTIG) is proposed. The theory describes two systems (stages): Einstein (ES) and "restructuring" (RS). We consider equations with quadratic potential that are symmetric with respect to scale transformations. The solutions of the equations obtained for the case of spaces defined by the Friedman-Robertson-Walker metric, as well as for a centrally symmetric space are investigated. In our model arise effective gravitational and cosmological "constants", which are defined by the "mean square" of the scalar fields. In obtained solutions the values of such parameters as "Hubble parameter", gravitational and cosmological "constants" in the RS stage fluctuate near monotonically evolving mean values. These parameters are matched with observational data, described as phenomena of dark energy and dark…
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