Chemical origins: Nuclear chemistry in the early universe

Research output: Chapter in Book/Report/Conference proceedingConference contribution

3 Scopus citations

Abstract

Big bang nucleosynthesis (BBN), describes the production of the light elements in the early universe. The theoretical prediction for the abundances of D, 3He, 4He, and 7Li is discussed and compared with their observational determination. The spectrum of anisotropies in the cosmic microwave background (CMB) now independently measures the baryon density to high precision. As a result, the CMB data test BBN. One finds that the CMB along with D and 4He observations paint a consistent picture. This concordance stands as a major success of the hot big bang. On the other hand, 7Li remains discrepant with the CMB-preferred baryon density; possible explanations are reviewed.

Original languageEnglish (US)
Title of host publicationChemical Evolution Across Space and Time
Subtitle of host publicationFrom the Big Bang to Prebiotic Chemistry
PublisherAmerican Chemical Society
Pages16-38
Number of pages23
ISBN (Print)9780841274310
DOIs
StatePublished - Feb 15 2008

Publication series

NameACS Symposium Series
Volume981
ISSN (Print)0097-6156
ISSN (Electronic)1947-5918

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