Spectroscopy of deeply bound orbitals in neutron-rich Ca isotopes

TL;DR

This study measures unbound states in neutron-rich calcium isotopes to understand their shell structure and single-particle strength, providing new experimental data that supports shell-model predictions and reveals detailed orbital configurations.

Contribution

First experimental measurement of unbound states in $^{53}$Ca and $^{55}$Ca, elucidating their orbital structure and supporting shell-model calculations.

Findings

Identification of unbound states at specific excitation energies.

Evidence for $ u 0f_{7/2}$ single-particle strength in neutron-rich Ca.

Good agreement with shell-model and extit{ab initio} predictions.

Abstract

The calcium isotopes are an ideal system to investigate the evolution of shell structure and magic numbers. Although the properties of surface nucleons in calcium have been well studied, probing the structure of deeply bound nucleons remains a challenge. Here, we report on the first measurement of unbound states in $^{53}$Ca and $^{55}$Ca, populated from \ts{54,56}Ca($p,pn$) reactions at a beam energy of around 216 MeV/nucleon at the RIKEN Radioactive Isotopes Beam Factory. The resonance properties, partial cross sections, and momentum distributions of these unbound states were analyzed. Orbital angular momentum $l$ assignments were extracted from momentum distributions based on calculations using the distorted wave impulse approximation (DWIA) reaction model. The resonances at excitation energies of 5516(41)\,keV in $^{53}$Ca and 6000(250)\,keV in $^{55}$Ca indicate a significant $l$\, =\,3 component, providing the first experimental evidence for the $\nu 0f_{7/2}$ single-particle strength of unbound hole states in the neutron-rich Ca isotopes. The observed excitation energies and cross-sections point towards extremely localized and well separated strength distributions, with some fragmentation for the $\nu 0f_{7/2}$ orbital in $^{55}$Ca. These results are in good agreement with predictions from shell-model calculations using the effective GXPF1Bs interaction and \textit{ab initio} calculations and diverge markedly from the experimental distributions in the nickel isotones at $Z=28$.