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We study a model of fluent material universe from a modified Newtoniancosmology proposed by D'Inverno and Tawfik. From this perspective, it shows alist of space-time curvature k with energy E, density \rho, specific heat$C_{p}$ and the fluid temperature gradient considered $\Delta T$ correspondingto standard thermodynamic variables. We determined the coupling constantsaccompanying the matter density for different values we can take k

Termodinamica del universo temprano desde una cosmolog\`Ia newtoniana