Abstract
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 k B T = 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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