On Gravitational Stefan-Boltzmann Law and Casimir Effect in FRW Universe
A. F. Santos, S. C. Ulhoa, E. P. Spaniol, Faqir C. Khanna

TL;DR
This paper investigates gravitational thermodynamic effects in a flat FRW universe using Thermo Field Dynamics and Teleparallel Gravity, providing insights into the cosmological constant and universe's deceleration.
Contribution
It introduces a novel calculation of Stefan-Boltzmann and Casimir effects within the FRW universe using TFD and TEGR frameworks, linking thermodynamics to cosmological parameters.
Findings
Predicted a minimum deceleration parameter range.
Estimated a very small magnitude for the cosmological constant.
Aligned effects with observed cosmological phenomena.
Abstract
Both Stefan-Boltzmann law and the Casimir effect, in a universe described by the FRW metric with zero curvature, are calculated. These effects are described by Thermo Field Dynamics (TFD). The gravitational energy-momentum tensor is defined in the context of Teleparallel Equivalent to General Relativity (TEGR). Each of the two effects gives a consistent prediction with what is observed on a cosmological scale. One of the effect establishes a minimum range for the deceleration parameter. While another leads to the conclusion that a possible cosmological constant has a very small order of magnitude.
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