Is the $(3+1)-d$ nature of the universe a thermodynamic necessity?
Julian Gonzalez-Ayala, F. Angulo-Brown

TL;DR
This paper proposes that the three spatial dimensions and the one time dimension of the universe emerged from thermodynamic principles, specifically entropy maximization and free energy minimization, within a higher-dimensional black body radiation framework.
Contribution
It introduces a thermodynamic explanation for the universe's dimensionality based on black body radiation in higher dimensions and principles like entropy increase and free energy minimization.
Findings
The universe's dimensions can be derived from thermodynamic selection principles.
The three spatial dimensions result from Helmholtz free energy minimization.
The arrow of time is linked to entropy increase in a closed system.
Abstract
It is well established that at early times, long before the time of radiation-matter equality, the universe could have been well described by a spatially flat, radiation only model. In this letter we consider the whole primeval universe as a black body radiation (BBR) system in an dimensional Euclidean space. We propose that the nature of the universe could be the result of a kind of thermodynamic selection principle stemming from the second law of thermodynamics. In regard the three spatial dimensions we suggest that they were chosen by means of the minimization of the Helmholtz free energy per hypervolume unit, while the time dimension, as it is well known was the result of the principle of increment of entropy for closed systems; that is, the so-called arrow of time.
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Taxonomy
TopicsCosmology and Gravitation Theories · Advanced Thermodynamics and Statistical Mechanics · Statistical Mechanics and Entropy
