Reduced regulator dependence of neutron-matter predictions with chiral interactions
arXiv:1209.5537 · doi:10.1103/PhysRevC.87.014322
Abstract
We calculate the energy per particle in infinite neutron matter perturbatively using chiral N3LO two-body potentials plus N2LO three-body forces. The cutoff dependence of the predictions is investigated by employing chiral interactions with different regulators. We find that the inclusion of three-nucleon forces, which are consistent with the applied two-nucleon interaction, leads to a strongly reduced regulator dependence of the results.
7 pages, 8 figures, 1 table, to be published in Physical Review C
References in corpus (5)
- Chiral effective field theory and nuclear forces
- Chiral three-nucleon interaction and the carbon-14 dating beta decay
- Low Momentum Nucleon-Nucleon Interactions and Shell-Model Calculations
- Spectra of Open-Shell Nuclei with Padé-Resummed Degenerate Perturbation Theory
- Study of the ground-state energy of 40Ca with the CD-Bonn nucleon-nucleon potential
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