Nuclear symmetry energy

C.-H. Lee, T. T. S. Kuo, G. Q. Li, and G. E. Brown
Phys. Rev. C 57, 3488 – Published 1 June 1998
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Abstract

To study the nuclear symmetry energy, we extend the Dirac-Brueckner approach with a Bonn one-boson-exchange nucleon-nucleon interaction to the general case of asymmetric nuclear matter. We extract the symmetry energy coefficient at the saturation to be about 31 MeV, which is in good agreement with the empirical value of 30±4MeV. The symmetry energy is found to increase almost linearly with the density, which differs considerably from the results of nonrelativistic approaches. This finding also supports the linear parametrization of Prakash, Ainsworth, and Lattimer. We find, furthermore, that the higher-order dependence of the nuclear equation of state on the asymmetry parameter is unimportant.

  • Received 22 December 1997

DOI:https://doi.org/10.1103/PhysRevC.57.3488

©1998 American Physical Society

Authors & Affiliations

C.-H. Lee, T. T. S. Kuo, G. Q. Li, and G. E. Brown

  • Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York 11794

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Issue

Vol. 57, Iss. 6 — June 1998

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