Review of Big Bang Nucleosynthesis and Primordial Abundances

Details Review of Big Bang Nucleosynthesis and Primordial Abundances Review of Big Bang Nucleosynthesis and Primordial Abundances

2000-01-18

arxiv.org/abs/astro-ph/0001318v1

Phys.Scripta T85 (2000) 12

Astronomy and Astrophysics

Astrophysics

61 pages, to appear in Physica Scripta

Scientific paper

10.1238/Physica.Topical.085a0001

Big Bang Nucleosynthesis (BBN) is the synthesis of the light nuclei, Deuterium, He3, He4 and Li7, during the first few minutes of the universe. This review concentrates on recent improvements in the measurement of the primordial (after BBN, and prior to modification) abundances of these nuclei. We mention improvement in the standard theory, and the non-standard extensions which are limited by the data. (abridged)

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