Quasiparticle interaction in nuclear matter with chiral three-nucleon forces
J. W. Holt, N. Kaiser, W. Weise

TL;DR
This paper derives the effective quasiparticle interaction in symmetric nuclear matter from chiral three-nucleon forces, revealing their significant impact on nuclear matter stability, the compression modulus, and spin-isospin response, with implications for nuclear models.
Contribution
It provides a first-order calculation of the Landau parameters including chiral three-nucleon forces, highlighting their effects on nuclear matter properties and stability.
Findings
Three-nucleon forces induce substantial repulsion in F_0, stabilizing nuclear matter.
Uncertainty in the compression modulus is large due to the low-energy constant c_3.
Three-nucleon forces cause small corrections to the nucleon effective mass and symmetry energy.
Abstract
We derive the effective interaction between two quasiparticles in symmetric nuclear matter resulting from the leading-order chiral three-nucleon force. We restrict our study to the L=0,1 Landau parameters of the central quasiparticle interaction computed to first order. We find that the three-nucleon force provides substantial repulsion in the isotropic spin- and isospin-independent component F_0 of the interaction. This repulsion acts to stabilize nuclear matter against isoscalar density oscillations, a feature which is absent in calculations employing low-momentum two-nucleon interactions only. We find a rather large uncertainty for the nuclear compression modulus due to a sensitive dependence on the low-energy constant c_3. The effective nucleon mass on the Fermi surface, as well as the nuclear symmetry energy, receive only small corrections from the leading-order chiral three-body…
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