Hot and dense asymmetric nuclear matter

Details Hot and dense asymmetric nuclear matter Hot and dense asymmetric nuclear matter

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvc..48.1056d&link_type=abstract

Physical Review C (Nuclear Physics), Volume 48, Issue 3, September 1993, pp.1056-1061

Physics

Nuclear Physics

9

Nuclear Matter, Neutron Stars

Scientific paper

The temperature dependence of different thermodynamic quantities such as the free energy, chemical potential, symmetry energy, single particle potential, equation of state, etc., is studied for asymmetric nuclear matter within a fully self-consistent model with an effective interaction. The equation of state is found to be quite soft in agreement with supernova calculations. The critical temperature for the occurrence of a liquid gas phase transition is found to decrease with the proton to neutron ratio γ and finally vanishes for pure neutron matter. The possibility of π- condensation has also been studied.

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