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Description of light clusters in relativistic nuclear models
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Description of light clusters in relativistic nuclear models
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Light clusters are included in the equation of state of nuclear matter within the relativistic mean field theory. The effect of the cluster-meson coupling constants on the dissolution density is discussed. Theoretical and experimental constraints are used to fix the cluster-meson couplings. The relative light cluster fractions are calculated for asymmetric matter in chemical equilibrium at finite temperature. It is found that above T = 5 MeV deuterons and tritons are the clusters in larger abundances. The results do not depend strongly on the relativistic mean field interaction chosen.
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Cited by 1 Pith paper
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Medium effects on light clusters from heavy-ion collisions within a relativistic mean-field description
Bayesian fits to Xe+Sn light-cluster yields show in-medium cluster couplings are temperature dependent, but cannot distinguish scalar-attraction from vector-repulsion pictures.
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