Termodinamica del universo temprano desde una cosmolog\`Ia 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 , specific heat Cp and the fluid temperature gradient considered T 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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