Properties of dense nuclear and neutron matter with relativistic nucleon-nucleon interactions

Journal Article · Mon Jun 01 00:00:00 EDT 1992 · Physical Review, C (Nuclear Physics); (United States)

DOI:https://doi.org/10.1103/PhysRevC.45.2782· OSTI ID:7286921

Li, G Q; Machleidt, R ^[1]; Brockmann, R ^[2]

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1. Department of Physics, University of Idaho, Moscow, Idaho 83843 (United States)
2. Department of Physics, University of Mainz, D-6500 Mainz (Germany)

Within the framework of the Dirac-Brueckner (DB) approach, the properties of dense nuclear and neutron matter are investigated using realistic nucleon-nucleon ({ital NN}) interactions which are derived from relativistic meson-field theory and describe the two-nucleon system quantitatively. Single-particle potentials, equations of state, nucleon effective masses, Landau parameters, and speeds of sound are calculated and analyzed as functions of density, for both nuclear and neutron matter. In the DB approach, the equation of state comes out stiffer than in the most sophisticated nonrelativistic calculation, but softer than in the Walecka model. Possible extensions of the present approach to nucleon-nucleus scattering and nucleus-nucleus collisions are also discussed.

• OSTI ID: 7286921
• Journal Information: Physical Review, C (Nuclear Physics); (United States), Vol. 45:6; ISSN 0556-2813
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
NUCLEAR MATTER
BRUECKNER MODEL
DIRAC EQUATION
EFFECTIVE MASS
EQUATIONS OF STATE
NEUTRON STARS
NUCLEON-NUCLEON INTERACTIONS
RELATIVISTIC RANGE
BARYON-BARYON INTERACTIONS
DIFFERENTIAL EQUATIONS
ENERGY RANGE
EQUATIONS
HADRON-HADRON INTERACTIONS
INTERACTIONS
MASS
MATHEMATICAL MODELS
MATTER
NUCLEAR MODELS
PARTIAL DIFFERENTIAL EQUATIONS
PARTICLE INTERACTIONS
STARS
WAVE EQUATIONS
663110* - General & Average Properties of Nuclei & Nuclear Energy Levels- (1992-)