Abstract

Baryon density inhomogeneities in the early universe can give rise to a floor of heavy elements (up to A≈270A\approx 270) produced in a primordial r-process with fission cycling. A parameter study with variation of the global baryon to photon ratio ηη, and under inclusion of neutron diffusion effects was performed. New results concerning the dependence of the results on nuclear physics parameters are presented.

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