Short-range correlations in isospin symmetric and asymmetric nuclear matter: a microscopic perspective
arXiv:1409.3999 · doi:10.1103/PhysRevC.90.064312
Abstract
Short-range correlations in nuclear and neutron matter are examined through the properties of the correlated wave function obtained by solving the Bethe-Goldstone equation. Tensor correlations are explored through the dominant tensor-driven transition and central correlations through the singlet and triplet S waves. Predictions from a popular meson-theoretic nucleon-nucleon potential employed in the Dirac-Brueckner-Hartree-Fock approach are compared with those from two- and three-body high-quality chiral interactions in Brueckner G-matrix calculations. Short-range correlations in symmetric matter are remarkably stronger than in neutron matter. It is found that short-range correlations are very model dependent and have a large impact on the symmetry energy above normal density.
10 pages, 6 figures; revised version, in press with Physical Review C
References in corpus (4)
Cited by in corpus (3)
- Relativistic Effects and Three-Nucleon Forces in Nuclear Matter and Nuclei
- Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter
- An overview of symmetric nuclear matter properties from chiral interactions up to fourth order of the chiral expansion