Constraints on particle physics from cosmology

Details Constraints on particle physics from cosmology Constraints on particle physics from cosmology

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nyasa.461..431s&link_type=abstract

(Aspen Center for Physics, DOE, NSF, et al., Aspen Winter Physics Conference, 1st, Aspen, CO, Jan. 6-19, 1985) New York Academy

Physics

Cosmology, Elementary Particle Interactions, Particle Theory, Baryons, Dark Matter, Grand Unified Theory, Gravitation Theory, Nuclear Fusion, Quantum Theory

Scientific paper

Cosmological models and their implications for theoretical and experimental particle physics are examined, reviewing the results of recent investigations. Consideration is given to quantum gravity, the search for a GUT, quark-lepton soup, weak freeze-out, nucleosynthesis, electricity and magnetism freeze-out, and dark matter. Topics discussed include cosmological limits on the baryon/photon ratio n(b)/n(gamma) = (3-10) x 10 to the -10th and on the number of neutrino flavors (best fit = 3, upper limit = 4), inflation theory and the early universe, the scale-free large-scale structure of the universe, and the nonbaryonic nature of the bulk of the matter in the universe.

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