Debye Layer Confinement of Nucleons in Nuclei for Heavy Nuclear Synthesis

Following the laser ablation studies Icading to a theory of nuclei confinement by a Debye layer mechanism, we presentlhere numerical evaluations for the known stable nuclei where the Coulomb repulsion is included as a rather minor componentespecially for lager nuclei. It is noticed that the well known empirical nuclear density of 2x I0^38 cm^-3 follows for anucleon number A 60 for iron. The crucial change of the Fermi energy into the relativistic branch for the nucleons resultsfor a density at 3x10^ 39 cm^-3 which density corresponds to the Debye layer equilibrium near uranium to curiumabove which the Fermi energy will not permit any equilibrium based nucleation. It is speculated whether the range betweenboth densities at the big bang expansion at temperatures offew 100 keY and at 200 seconds after the big bang isresulting in a nuclear-chemical Boltzmann equilibrium for the generation of the endothermic nuclear generation. Thequestion is then open, what additional nuclear expansion forces are acting in the elements between iron and uraniumduring these equilibrium reactions in nuclei such that the empirical nuclear density is produced.