Element abundances in hot nuclear matter

Details Element abundances in hot nuclear matter Element abundances in hot nuclear matter

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phlb..185..281r&link_type=abstract

Physics Letters B, Volume 185, Issue 3-4, p. 281-286.

Physics

3

Scientific paper

The abundances of clusters in hot dense matter can become strongly influenced by in-medium effects such as Pauli quenching and Coulomb correlations. Model calculations are performed at the parameter values temperature kBT = 5 MeV, baryon density ϱ = 0.016 fm-3. The medium effect on element abundances may be of interest not only in heavy ion collisions but also in primordial nucleosynthesis.

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