Hypernuclear constraints on $\Lambda N$ and $\Lambda NN$ interactions

TL;DR

This paper reviews how density-dependent $\Lambda$-nuclear optical potentials can accurately model $\Lambda$ hypernuclear binding energies across a wide mass range, highlighting the roles of $\Lambda N$ and $\Lambda NN$ interactions.

Contribution

It introduces a simplified two-parameter interaction model that fits all known $\Lambda$ binding energies and addresses the hyperon puzzle.

Findings

The $\Lambda N$ interaction alone overbinds hypernuclei.

Two interaction parameters effectively fit experimental data.

The $\Lambda NN$ interaction strength aligns with resolving the hyperon puzzle.

Abstract

Recent work on using density dependent $\Lambda$-nuclear optical potentials in calculations of $\Lambda$-hypernuclear binding energies is reviewed. It is found that all known $\Lambda$ binding energies in the mass range $16 \leq A \leq 208$ are well fitted in terms of two interaction parameters: one, attractive, for the spin-averaged $\Lambda N$ interaction and another one, repulsive, for the $\Lambda NN$ interaction. The $\Lambda N$ interaction term by itself overbinds $\Lambda$ hypernuclei, in quantitative agreement with recent findings obtained in EFT and Femtoscopy studies. The strength of the $\Lambda NN$ interaction term is compatible with values required to resolve the hyperon puzzle.