Comparative study of three-nucleon potentials in nuclear matter
arXiv:1109.5489 · doi:10.1103/PhysRevC.85.024003
Abstract
A new generation of local three-body potentials providing an excellent description of the properties of light nuclei, as well as of the neutron-deuteron doublet scattering length, has been recently derived. We have performed a comparative analysis of the equations of state of both pure neutron matter and symmetric nuclear matter obtained using these models of three-nucleon forces. None of the considered potentials simultaneously explains the empirical equilibrium density and binding energy of symmetric nuclear matter. However, two of them provide reasonable values of the saturation density. The ambiguity concerning the treatment of the contact term of the chiral inspired potentials is discussed.
14 pages, 8 figures
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- Three-Nucleon Forces: Implementation and Applications to Atomic Nuclei and Dense Matter
- Self-consistent Green's functions formalism with three-body interactions
- Symmetric nuclear matter with chiral three-nucleon forces in the self-consistent Green's functions approach
- Quantum Monte Carlo Methods in Nuclear Physics: Recent Advances
- Correlated density-dependent chiral forces for infinite matter calculations within the Green's function approach
- Auxiliary-Field Quantum Monte Carlo Simulations of Neutron Matter in Chiral Effective Field Theory
- Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactions
- Linear response of homogeneous nuclear matter with energy density functionals
- Regulator Artifacts in Uniform Matter for Chiral Interactions
- Analyzing the Fierz Rearrangement Freedom for Local Chiral Two-Nucleon Potentials
- Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials
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- Short-range correlation effects on the nuclear matrix element of neutrinoless double- decay
- Applying the Density Matrix Expansion with Coordinate-Space Chiral Interactions
- Quantum Monte Carlo formalism for dynamical pions and nucleons
- Exact restoration of Galilei invariance in density functional calculations with quantum Monte Carlo
- Effective interaction approach to the Fermi hard-sphere system
- Comparison of nuclear hamiltonians using spectral function sum rules
- Self-consistent Green's functions with three-body forces
- Modeling Neutron Star Matter in the Age of Multimessenger Astrophysics
- Neutron star calculations with the phenomenological three-nucleon force
- Nuclear matter calculations with the phenomenological three-nucleon interaction
- Ab initio calculations on nuclear matter properties including the effects of three-nucleons interaction
- The hard-sphere model of strongly interacting fermion systems