Abstracts

Francisco Bulnes

Baryongenesis until dark matter: H-particles proliferation

A digression on the dark matter and dark energy considering the baryongenesis and their evolution until the actual Universe is realised. The factors of inflation and matter-energy production are analysed, likewise the hadrons as fundamental part in the dark matter production are considered. Some results on torsion in baryongenesis are used to complete the evidences as baryons acoustic oscillations, the effects due to the cosmic expansion, redshift, space-time distortions, and other inhomogeneous effects observed. Then is established a theorem in mathematical cosmology that affirms that the dark energy is given beyond of the fundamental interacting of the baryongenesis and arises with the proliferation of the H-particles in extended photon sources.