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Experimental, computational, and observational analysis of primordial nucleosynthesis

Smith, Michael S., Kawano, Lawrence H., Malaney, Robert A.·1993·The Astrophysical Journal Supplement Series

Abstract

We present a comprehensive evaluation of the current status of the standard theory of primordial nucleosynthesis, determining the 12 nuclear reactions most important for the production of the light elements and conducting a detailed study of their rates and uncertainties; these are incorporated into a Monte Carlo analysis to evaluate uncertainties in the computed elemental abundances. These predicted abundances are compared with primordial abundances deduced from astronomical observations of the light elements D, He-3, He-4, and Li-7; consistent agreement exists over a narrow range of the baryon-to-photon ratio n, thereby supporting the standard theory of big bang nucleosynthesis. This n range corresponds to a constraint on the baryon density parameter of 0.01-0.09, where the primordial D + He-3 abundance sets the lower bound and the He-4 abundance sets the upper bound. The new reaction rates cause an increase in the upper bound from Li-7 by 40 percent over that determined in previous studies.

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Metadata

Authors
Smith, M. S., Kawano, L. H., & Malaney, R. A.
Venue
The Astrophysical Journal Supplement Series
Published
1993-04
Volume
85
Pages
219
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W2097088502
Cited by
408
References
0
Type
conference abstract
Language
en
Open access
closed

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CoChat. (2026). Citation check: Experimental, computational, and observational analysis of primordial nucleosynthesis. https://app.cochat.ai/papers/10.1086/191763
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Smith, M. S., Kawano, L. H., & Malaney, R. A. (1993). Experimental, computational, and observational analysis of primordial nucleosynthesis. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/191763

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