Equation of state of isospin asymmetric nuclear matter including relativistic random-phase approximation-type correlations

Details Equation of state of isospin asymmetric nuclear matter including relativistic random-phase approximation-type correlations Equation of state of isospin asymmetric nuclear matter including relativistic random-phase approximation-type correlations

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phrvc..57.3447f&link_type=abstract

Physical Review C (Nuclear Physics), Volume 57, Issue 6, June 1998, pp.3447-3451

Physics

Nuclear Physics

2

Nuclear Matter Aspects Of Neutron Stars, Nuclear Structure Models And Methods, Nuclear Matter

Scientific paper

The equation of state of asymmetric matter including the relativistic exchange and correlation parts is calculated in the σ-ω model. The results are discussed in comparison with empirical informations and phenomenological approaches. Neutron star matter in β equilibrium and the resulting neutron star masses are also discussed.

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