Relations between three-particle interactions in nuclear matter to observable quantities
Wolfgang Bentz, Ian C. Cloët
TL;DR
The paper addresses how three-particle interactions in nuclear matter influence observable bulk quantities by deriving model-independent relations between the slope parameters of the symmetry energy and incompressibility, $L$ and $J$, and the $ extit{ell}=0$ moments of in-medium three-nucleon forward scattering amplitudes. It uses the Landau-Migdal Fermi liquid framework to express these slopes in terms of dimensionless three-body parameters $H_\ell$ and $H'_\ell$, and then analyzes the physical content of the three-particle amplitude, decomposing it into retardation terms and a three-body kernel $K^{(3)}$, with a BBG-inspired ladder expansion up to third order revealing both two-body and higher-order three-body contributions. Semi-quantitative assessments with empirical inputs suggest $H_0>1$ (isoscalar) and $H'_0<0$ (isovector) with $|H'_0|<1$, while $H_1$ is subleading; the results imply that three-body cluster terms may be needed to account for the symmetry energy slope $L$. The work highlights the emergence of medium-induced four-body-like effects in the in-medium three-particle amplitude and establishes a concrete link between microscopic three-body dynamics and macroscopic nuclear observables, with implications for nuclei and neutron-star structure.
Abstract
In the first part of this paper, we use the framework of the Fermi liquid theory to derive model-independent relations between the slope parameters of the symmetry energy and of the incompressibility in nuclear matter to three-particle interaction parameters. Based on these relations, we present simple estimates and compare with the empirical information. In the second part, we discuss the general structure of the three-particle scattering amplitude in nuclear matter, and use methods similar to the Bethe-Brueckner-Goldstone theory to show how three-particle cluster diagrams emerge naturally in the Fermi liquid theory.
