Equation of state of homogeneous nuclear matter and the symmetry coefficient

Details Equation of state of homogeneous nuclear matter and the symmetry coefficient Equation of state of homogeneous nuclear matter and the symmetry coefficient

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvc..50..460o&link_type=abstract

Physical Review C (Nuclear Physics), Volume 50, Issue 1, July 1994, pp.460-468

Physics

Nuclear Physics

14

Late Stages Of Stellar Evolution, Nuclear Matter, Binding Energies And Masses

Scientific paper

For different Skyrme-type forces we investigate the equation of state of homogeneous nuclear matter under the conditions appropriate to a collapsing star. We find that the stiffness of the equation of state increases significantly as the symmetry coefficient J of nuclear matter increases over the range of its experimental uncertainty. We present analytic expressions for the adiabatic index Γ permitting the elimination of all numerical derivatives.

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