Symmetric nuclear matter with chiral three-nucleon forces in the self-consistent Green's functions approach
arXiv:1307.1889 · doi:10.1103/PhysRevC.88.044302
Abstract
We present calculations for symmetric nuclear matter using chiral nuclear interactions within the Self-Consistent Green's Functions approach in the ladder approximation. Three-body forces are included via effective one-body and two-body interactions, computed from an uncorrelated average over a third particle. We discuss the effect of the three-body forces on the total energy, computed with an extended Galitskii-Migdal-Koltun sum-rule, as well as on single-particle properties. Saturation properties are substantially improved when three-body forces are included, but there is still some underlying dependence on the SRG evolution scale.
12 pages, 12 figures
References in corpus (14)
- Chiral effective field theory and nuclear forces
- Improved nuclear matter calculations from chiral low-momentum interactions
- Similarity Renormalization Group for Nucleon-Nucleon Interactions
- Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory
- Constraints on neutron star radii based on chiral effective field theory interactions
- Local three-nucleon interaction from chiral effective field theory
- Density dependence of the nuclear symmetry energy: a microscopic perspective
- Chiral three-nucleon interaction and the carbon-14 dating beta decay
- Momentum space evolution of chiral three-nucleon forces
- Hot neutron matter from a Self-Consistent Green's Functions approach
- In medium T-matrix for nuclear matter with three-body forces - binding energy and single particle properties
- Density-dependent nucleon-nucleon interaction from three-nucleon forces
- Thermodynamic properties of nuclear matter with three-body forces
- Neutron matter based on consistently evolved chiral three-nucleon interactions
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