Constraints on the heavy elements production in inhomogeneous Big-Bang nucleosynthesis from light-element observations

Details Constraints on the heavy elements production in inhomogeneous Big-Bang nucleosynthesis from light-element observations Constraints on the heavy elements production in inhomogeneous Big-Bang nucleosynthesis from light-element observations

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..378n&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Computer Science

Nucleosynthesis, Cosmic Background Radiation, Star Formation, Origin, Formation, And Abundances Of The Elements, Background Radiations, Star Formation

Scientific paper

We investigate the nucleosynthesis that includes the production of heavy elements beyond 7Li in the inhomogeneous big-bang nucleosynthesis. We can get the parameter regions from light elements of 4He and D for the baryon-to-photon ratio obtained by CMB. In these allowed parameter region, we have confirmed that the heavy elements beyond Fe can be produced appreciably, where p- and/or r-elements are produced well compared to the solar system abundances.

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