出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：Light clusters (up to A=4) in nuclear matter at subsaturation densities are treated in a quantum statistical approach. Self-energy, Pauli-blocking, and effects of continuum correlations are taken into account to calculate the quasiparticle properties and abundances of light elements [1]. Results are compared with experiments from Heavy Ion Collisions [2]. Consequences for the Equation of State [3] and nuclear structure are given [4]. The appearence of light clusters in core-collapse supernovae at post-bounce stage may modify the neutrino emission and absorption processes and, thereby, influence the supernova mechanism [5].
