Short range correlations in relativistic nuclear matter models
arXiv:nucl-th/0602059 · doi:10.1103/PhysRevC.73.035805
Abstract
Short range correlations are introduced using unitary correlation method in a relativistic approach to the equation of state of the infinite nuclear matter in the framework of the Hartree-Fock approximation. It is shown that the correlations give rise to an extra node in the ground-state wave-function in the nucleons, contrary to what happens in non-relativistic calculations with a hard core. The effect of the correlations in the ground state properties of the nuclear matter and neutron matter is studied. The nucleon effective mass and equation of state (EOS) are very sensitive to short range correlations. In particular, if the pion contact term is neglected a softening of the EOS is predicted. Correlations have also an important effect on the neutron matter EOS which presents no binding but only a very shallow minimum contrary to the Walecka model.
8pages, 4 figures
References in corpus (4)
Cited by in corpus (5)
- Non-rotating and rotating neutron stars in the extended field theoretical model
- Density matrix expansion for the MDI interaction
- Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter
- Neutron stars within relativistic central variational method
- Relativistic model for the nonmesonic weak decay of single-lambda hypernuclei