Background gravitational waves as signature of the adiabatic expansion of a black body that represents the dark universe
Cl\'audio Nassif Cruz, A. C. Amaro de Faria Jr

TL;DR
This paper introduces a toy model of the dark universe as an expanding black-body sphere composed of exotic dark gas, deriving gravitational laws and predicting a very low-frequency background gravitational wave signature.
Contribution
It proposes a novel conceptual model linking dark energy, vacuum fluctuations, and gravitational waves through an expanding black-body analogy.
Findings
Estimates the cosmological constant's magnitude.
Predicts a background gravitational wave at ~10^{-17} Hz.
Derives a law of universal gravitation from the model.
Abstract
We propose a toy model of a spherical universe made up of an exotic dark gas with temperature in thermal equilibrium with a black-body in adiabatic expansion. Each particle of this exotic gas mimics a kind of particle of dark energy represented by the vacuum energy, being quantized into virtual particles with extremely small masses that form such gas representng the own tissue of the expanding space-time governed by a negative pressure whose origin is the equation of state (EOS) of vacuum, i.e., , where is the vacuum energy density. So, each vacuum particle occupies a tiny area of space so-called Planck area , which represents the minimum area of the whole space-time given by the spherical surface with area , where is the Hubble radius. We realize that such spherical surface is the surface of the black-body for representing the dark…
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