Production of the light elements in primordial nucleosynthesis

Details Production of the light elements in primordial nucleosynthesis Production of the light elements in primordial nucleosynthesis

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...359..267k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 359, Aug. 20, 1990, p. 267-276.

Astronomy and Astrophysics

Astrophysics

124

Abundance, Beryllium, Boron, Cosmochemistry, Light Elements, Nuclear Fusion, Chemical Evolution, Cosmic Rays, Lithium, Universe

Scientific paper

The predicted yields of Be-9, B-10, and B-11 from primordial nucleosynthesis are investigated in both the standard model (SM) and the nonuniform density model (NDM). For SM, the study takes into account a wide range of Omega(B), the average baryonic density of the universe, and for NDM it takes into account a larger range of parameter space, including variations in Omega(B), the volume fraction of the high-density zones, and the ratio of baryon number density in high-density zones to that in low-density zones. The NDM is found for most of the possible parameter space to produce considerably more Be-9, B-10, and B-11 than does the SM.

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