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Phys. Rev. C 57, 3447–3451 (1998)

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

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Norbert Fröhlich and Hans Baier
Institut für Radiumforschung und Kernphysik, University of Vienna, Boltzmanngasse 3, 1090 Vienna, Austria

Wolfgang Bentz
Department of Physics, Faculty of Science, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113, Japan

Received 12 January 1998; published in the issue dated June 1998

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.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.57.3447
DOI:
10.1103/PhysRevC.57.3447
PACS:
26.60.+c, 21.60.-n, 21.65.+f