Evidence for a possible common origin of baryonic and non-baryonic dark matter

Details Evidence for a possible common origin of baryonic and non-baryonic dark matter Evidence for a possible common origin of baryonic and non-baryonic dark matter

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aipc..336..513s&link_type=abstract

Dark matter. AIP Conference Proceedings, Volume 336, pp. 513-516 (1995).

Mathematics

Logic

Dark Matter, Particle-Theory And Field-Theory Models Of The Early Universe

Scientific paper

A single ``positronium'' or integrally charged ``quarkonium''-like model for matter originally developed for the spin 0 neutral pion is shown to explain the nature of cold dark matter in the early Universe when in a highly excited spin 1 vector boson state, as well as the properties of baryonic matter following a phase transition to form a three-component nucleon structure in its final step of decay to the ground-state accompanied by a large release of energy that represents the Big Bang. The model gives the masses and sizes of cosmological structures, resolves the problem of nucleosynthesis at the high present baryon density, and explains the origin of dark baryonic halos as well as the rising mass-luminosity ratio with distance.

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