Quantum fluctuations of geometry in hot Universe
Iwo Bialynicki-Birula

TL;DR
This paper investigates quantum fluctuations of spacetime geometry at finite temperature using linearized gravity, revealing foam-like configurations and energy expressions consistent with graviton treatment, and highlighting differences from electromagnetic fluctuations.
Contribution
It introduces a novel analysis of gravitational field fluctuations at finite temperature using the Wigner functional and linearized Riemann-Weyl tensor, showing foam-like structures and energy consistency.
Findings
Fluctuations have a foam-like structure with large geometric changes.
Total energy expression matches graviton-based calculations.
Infrared divergence at zero temperature distinguishes gravitational from electromagnetic fluctuations.
Abstract
The fluctuations of spacetime geometries at finite temperature are evaluated within the linearized theory of gravity. These fluctuations are described by the probability distribution of various configurations of the gravitational field. The field configurations are described by the linearized Riemann-Weyl tensor without any reference to the metric. The probability distribution of various configurations is described by the Wigner functional of the gravitational field. It has a foam-like structure, dominant configurations are those with large changes of geometry at nearby points. In the high-temperature limit one obtains the Bolzmann distribution that enables one to identify the expression for the total energy of the gravitational field. The appearance of the same expression for the total energy when the gravitational field is treated as a collection of gravitons and as the…
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