Testing the big bang: Light elements, neutrinos, dark matter, and large-scale structure

Details Testing the big bang: Light elements, neutrinos, dark matter, and large-scale structure Testing the big bang: Light elements, neutrinos, dark matter, and large-scale structure

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991stin...9133040s&link_type=abstract

Presented at the 2nd Winter School of Physics, San Juan (Puerto Rico), 28 Mar. - 5 Apr. 1991

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Big Bang Cosmology, Dark Matter, Galactic Evolution, Light Elements, Neutrinos, Nuclear Fusion, Abundance, Astrophysics

Scientific paper

In this series of lectures, several experimental and observational tests of the standard cosmological model are examined. In particular, detailed discussion is presented regarding: (1) nucleosynthesis, the light element abundances, and neutrino counting; (2) the dark matter problems; and (3) the formation of galaxies and large-scale structure. Comments will also be made on the possible implications of the recent solar neutrino experimental results for cosmology. An appendix briefly discusses the 17 keV thing and the cosmological and astrophysical constraints on it.

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