Exact calculation of three-body contact interaction to second order
arXiv:1203.6283 · doi:10.1140/epja/i2012-12058-9
Abstract
For a system of fermions with a three-body contact interaction the second-order contributions to the energy per particle are calculated exactly. The three-particle scattering amplitude in the medium is derived in closed analytical form from the corresponding two-loop rescattering diagram. We compare the (genuine) second-order three-body contribution to with the second-order term due to the density-dependent effective two-body interaction, and find that the latter term dominates. The results of the present study are of interest for nuclear many-body calculations where chiral three-nucleon forces are treated beyond leading order via a density-dependent effective two-body interaction.
9 pages, 6 figures, to be published in European Journal A
References in corpus (4)
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- Subleading contributions to the chiral three-nucleon force I: long-range terms
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Cited by in corpus (14)
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- Chiral Effective Field Theory and the High-Density Nuclear Equation of State
- Equation of state of nuclear and neutron matter at third-order in perturbation theory from chiral EFT
- Symmetric nuclear matter with chiral three-nucleon forces in the self-consistent Green's functions approach
- Towards order-by-order calculations of the nuclear and neutron matter equations of state in chiral effective field theory
- Nuclear chiral dynamics and thermodynamics
- Towards grounding nuclear physics in QCD
- Regulator Artifacts in Uniform Matter for Chiral Interactions
- Density-dependent effective baryon-baryon interaction from chiral three-baryon forces
- Microscopically constrained mean field models from chiral nuclear thermodynamics
- Implementing chiral three-body forces in terms of medium-dependent two-body forces
- Exact solution of the Brueckner-Bethe-Goldstone equation with three-body forces in nuclear matter
- Estimates and power counting in uniform matter with softened interactions
- Partial restoration of chiral symmetry in hot and dense neutron matter