Hot nuclear and neutron matter with a density-dependent interaction

Physics – Nuclear Physics

Scientific paper

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Nuclear Matter, Neutron Stars

Scientific paper

The temperature dependence of the different thermodynamic quantities like entropy, equation of state, free energy, internal energy, effective mass, chemical potential, etc. are calculated for nuclear and neutron matter within a fully self-consistent model and compared with the results obtained by others. An effective interaction consisting of Sussex interaction plus an empirical density-dependent interaction is taken in the calculation. The latter is added so as to correctly reproduce the saturation property of nuclear matter. The calculated entropy is in excellent agreement with experiment.

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