Computer Science – Numerical Analysis
Scientific paper
Sep 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...378..504e&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 378, Sept. 10, 1991, p. 504-518. Research supported by Keck Foundation and
Computer Science
Numerical Analysis
35
Abundance, Big Bang Cosmology, Nuclear Fusion, Analytic Functions, Baryons, Deuterium, Numerical Analysis
Scientific paper
Approximate results for the standard theory of big bang nucleosynthesis are derived analytically, i.e., without the use of the Wagoner code, using ideas of fixed points and freezeout. The element abundances follow quasi-static equilibrium and eventually freeze out near their final values. The calculations are relatively simple and provide a better understanding of the physics than is possible from a numerical code containing nearly 100 reactions.
Dimopoulos Savas
Esmailzadeh Rahim
Starkman Glenn D.
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