# Effects of hyperonic many-body force on $B_\Lambda$ values of   hypernuclei

**Authors:** M. Isaka, Y. Yamamoto, Th.A. Rijken

arXiv: 1703.03117 · 2017-04-12

## TL;DR

This paper investigates how strongly repulsive many-body forces, modeled via multi-pomeron exchange, influence the binding energies of hypernuclei and support a stiff equation of state consistent with massive neutron stars.

## Contribution

It introduces a model incorporating multi-pomeron exchange potentials to accurately reproduce hypernuclear binding energies and neutron star observations.

## Key findings

- MBE with strong MPP repulsion reproduces $B_\Lambda$ data across hypernuclei.
- The model supports a stiff EoS compatible with $2M_{\odot}$ neutron stars.
- Calculated $B_\Lambda$ values match experimental data within a few hundred keV.

## Abstract

The stiff equation of state (EoS) giving the neutron-star mass of $2M_{\odot}$ suggests the existence of strongly repulsive many-body effect (MBE) not only in nucleon channels but also in hyperonic ones. As a specific model for MBE, the repulsive multi-pomeron exchange potential (MPP) is added to the two-body interaction together with the phenomenological three-body attraction. For various versions of the Nijmegen interaction models, the MBE parts are determined so as to reproduce the observed data of $B_\Lambda$. The mass dependence of $B_\Lambda$ values is shown to be reproduced well by adding MBE with the strong MPP repulsion assuring the stiff EoS of hyperon-mixed neutron-star matter, when $P$-state components of the adopted interaction model lead to almost vanishing contributions. The nuclear matter $\Lambda\!N$ $G$-matrix interactions are derived and used in $\Lambda$ hypernuclei on the basis of the averaged-density approximation (ADA). The $B_\Lambda$ values of hypernuclei with $9 \le A \le 59$ are analyzed in the framework of Antisymmetrized Molecular Dynamics with use of the two types of $\Lambda\!N$ $G$-matrix interactions including strong and weak MPP repulsions. The calculated values of $B_\Lambda$ reproduce the experimental data finely within a few hundred keV. The values of $B_\Lambda$ in $p$-states also can be reproduced well, when ADA is modified to be suitable also to weakly-bound $\Lambda$ states.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1703.03117/full.md

## References

50 references — full list in the complete paper: https://tomesphere.com/paper/1703.03117/full.md

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Source: https://tomesphere.com/paper/1703.03117