Building a linear equation of state for trapped gravitons from finite size effects and the Schwarzschild black hole case
Stefano Viaggiu

TL;DR
This paper investigates how finite size effects modify the spectrum of trapped gravitons, leading to a linear equation of state and potential implications for black hole entropy and dark energy formation.
Contribution
It introduces a model linking finite size effects to a linear graviton equation of state and explores its implications for black hole physics and dark energy.
Findings
Finite size effects can produce a linear equation of state for trapped gravitons.
Logarithmic corrections to black hole entropy naturally emerge from the model.
Constraints on the areal radius R depend on the equation of state parameter γ.
Abstract
In this paper we continue the investigations present in \cite{1} and \cite{2} concerning the spectrum of trapped gravitons in a spherical box, and in particular inside a Schwarzschild black hole (BH). We explore the possibility that, due to finite size effects, the frequency of the radiation made of trapped gravitons can be modified in such a way that a linear equation of state for the pressure and the internal energy arises. Firstly, we study the case with , where only fluids with are possible. If corrections are added to , for we found no limitation on the allowed value for the areal radius of the trapped sphere . Moreover, for we have a minimum allowed value for of the order of the Planck length . Conversely, a fluid with can be obtained but with a…
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