The matter-energy intensity distribution in a quantum gravitational system
V. E. Kuzmichev, V. V. Kuzmichev (Bogolyubov Institute for Theoretical, Physics)

TL;DR
This paper investigates the quantum matter-energy distribution in a maximally symmetric quantum gravitational system using constraint quantization, analyzing wave equations, and calculating intensity distributions for specific models.
Contribution
It introduces a normalized wave function framework for quantum gravitational systems and extends wave equations to negative scale factors, providing new insights into quantum cosmology.
Findings
Derived normalized wave functions for QGS
Calculated matter intensity distributions for specific models
Drawn analogies with optical diffraction phenomena
Abstract
In the framework of the method of constraint system quantization, a quantum gravitational system (QGS) with the maximally symmetric geometry is studied. The state vector of the QGS satisfies the set of wave equations which describes the time evolution of a quantum system in the space of quantum fields. It is shown that this state vector can be normalized to unity. The generalization of the wave equations to the domain of negative values of the cosmic scale factor is made. For the arrow of time from past to future, the state vector describes the QGS contracting for the negative values of the scale factor and expanding for its positive values. The intensity distributions of matter are calculated for two exactly solvable models of spatially closed and flat QGSs formed by dust and radiation. The analogies with the motion in time of minimum wave packet for spatially closed QGS and with the…
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