Primordial chemistry: an overview

Details Primordial chemistry: an overview Primordial chemistry: an overview

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..476...83s&link_type=abstract

Conference on 3K cosmology. AIP Conference Proceedings, Volume 476, pp. 83-104 (1999).

Physics

Origin, Formation, And Abundances Of The Elements, Big Bang Nucleosynthesis

Scientific paper

In the standard Big Bang model, the light elements in the cosmos -hydrogen and helium but also deuterium and lithium- were created in the very early Universe. The main problem is to connect what we can actually observe to day with the standard Big Bang nucleosynthesis predictions essentially because of uncertainties in modeling their evolution since the Big Bang. After a brief review of the primordial nucleosynthesis -predictions and observations of the primordial abundances- we present the preliminary studies of the primordial chemistry: molecular formation and evolution in the early Universe.

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