# The contribution of chiral three-body forces to the monopole component   of the effective shell-model Hamiltonian

**Authors:** Y. Z. Ma, L. Coraggio, L. De Angelis, T. Fukui, A. Gargano, N. Itaco,, and F. R. Xu

arXiv: 1812.03284 · 2019-10-02

## TL;DR

This paper investigates how realistic three-body forces derived from chiral perturbation theory influence the monopole component of the shell-model Hamiltonian, crucial for accurately describing shell evolution in nuclei.

## Contribution

It demonstrates that including three-body forces is essential for reproducing experimental shell evolution in fp-shell nuclei, advancing shell-model Hamiltonian accuracy.

## Key findings

- Three-body forces significantly improve shell evolution predictions.
- Including three-body forces reproduces experimental shell closures.
- Shell-model calculations with three-body forces match observed data.

## Abstract

We present a study of the role played by realistic three-body forces in providing a reliable monopole component of the effective shell-model Hamiltonian. To this end, starting from a nuclear potential built up within the chiral perturbation theory, we derive effective shell-model Hamiltonians with and without the contribution of the three-body potential and compare the results of shell-model calculations with a set of observables that evidence shell-evolution properties. The testing ground of our investigation are nuclei belonging to fp shell, since the shell evolution towards shell closures in 48Ca and 56Ni provides a paradigm for shell-model Hamiltonians. Our analysis shows that only by including contributions of the three-body force the monopole component of the effective shell-model Hamiltonian is then able to reproduce the experimental shell evolution towards and beyond the closure at N=28.

## Full text

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## Figures

22 figures with captions in the complete paper: https://tomesphere.com/paper/1812.03284/full.md

## References

53 references — full list in the complete paper: https://tomesphere.com/paper/1812.03284/full.md

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Source: https://tomesphere.com/paper/1812.03284