  For the first time, a reliable estimation for the equations of state (EoS),
bulk viscosity, and relaxation time, at temperatures ranging from a few MeV up
to TeV or energy density up to $10^{16}~$GeV/fm$^3$. This genuine study covers
both strong and electroweak epochs of the early Universe. Non--perturbation
(up, down, strange, charm, and bottom quark flavor) and perturbative
calculations (up, down, strange, charm, bottom, and top quark flavors), are
phenomenologically combined, at vanishing baryon--chemical potential. In these
results, calculations from Polyakov linear--sigma model (PLSM) of the vacuum
and thermal condensations of the gluons and the quarks (up, down, strange, and
charm flavors) are also integrated. Furthermore, additional degrees of freedom
(photons, neutrinos, charged leptons, electroweak particles, and scalar Higgs
boson) are found significant along the entire range of temperatures. As never
done before, the present study brings the standard model of elementary
particles closer to the standard model for cosmology.

High Energy Physics - Phenomenology;General Relativity and Quantum Cosmology