Numerical nucleosynthesis results for Bianchi type-V cosmological models

Details Numerical nucleosynthesis results for Bianchi type-V cosmological models Numerical nucleosynthesis results for Bianchi type-V cosmological models

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.123..411m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 123, no. 2, June 1986, p. 411-414.

Statistics

Computation

2

Abundance, Cosmology, Deuterium, Helium Isotopes, Nuclear Fusion, Astronomical Models, Computational Astrophysics

Scientific paper

Results of numerical calculations of helium-4 and deuterium abundances
in a wide range of Bianchi type-V locally rotationally-symmetric
cosmolgical models are presented. The tabulated element abundances show
that these models generically yield helium fractions which are
unacceptably large compared with the available observational data.

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