Foundations of a Theory of Gravity with a Constraint and its Canonical Quantization
Alexander P. Sobolev

TL;DR
This paper introduces a gravity theory with a physical constraint, unifying cosmological models without dark matter or energy, and explores its implications for the early Universe, including wave functions and initial conditions.
Contribution
It proposes a gravity theory with a physical constraint that generalizes GR and unimodular gravity, providing a new cosmological model consistent with observations.
Findings
Universe's maximum energy density was much lower than Planck scale
Entropy density exceeds GR predictions by 18 orders of magnitude
Wave function of the early Universe indicates a random origin
Abstract
The gravitational equations were derived in general relativity (GR) using the assumption of their covariance relative to arbitrary transformations of coordinates. It has been repeatedly expressed an opinion over the past century that such equality of all coordinate systems may not correspond to reality. Nevertheless, no actual verification of the necessity of this assumption has been made to date. The paper proposes a theory of gravity with a constraint, the degenerate variants of which are general relativity (GR) and the unimodular theory of gravity. This constraint is interpreted from a physical point of view as a sufficient condition for the adiabaticity of the process of the evolution of the space-time metric. The original equations of the theory of gravity with the constraint are formulated. On this basis, a unified model of the evolution of the modern, early, and very early…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Space Science and Extraterrestrial Life
