arXiv · 1110.4056
Termodinamica del universo temprano desde una cosmologÌa newtoniana
Abstract
We study a model of fluent material universe from a modified Newtonian cosmology proposed by D'Inverno and Tawfik. From this perspective, it shows a list of space-time curvature k with energy E, density ρ, specific heat $C_{p}$ and the fluid temperature gradient considered $ΔT$ corresponding to standard thermodynamic variables. We determined the coupling constants accompanying the matter density for different values we can take k
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W. A. Rojas C. 2011-10-18. Termodinamica del universo temprano desde una cosmologÌa newtoniana. https://arxiv.org/abs/1110.4056
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