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Isospin symmetry holds beyond the proton drip line: First observation of excited states in 55Cu
Letter/Communication   Open access

Isospin symmetry holds beyond the proton drip line: First observation of excited states in 55Cu

Jeffrey Allan Tostevin, S. Pigliapoco, M.L. Cortés, F. Recchia, P. Doornenbal, S. M. Lenzi and M. A. Bentley
Physics Letters B, 140564
20/05/2026

Abstract

Isospin symmetry Proton-drip line Mirror nuclei In-beam í µí»¾-ray spectroscopy
Isospin symmetry, combined with shell-model description, has long been successful in reproducing nuclear structure and predicting mirror energy differences. However, these descriptions have been primarily limited to mirror nuclei with well-bound ground states. As one approaches the proton drip line, coupling to the continuum becomes important. Despite this, little is known about medium-mass nuclei at the drip line. Here we report the measurement of the excitation energies of several unbound states in a nucleus beyond the proton drip line, 55Cu, performed via γ-ray spectroscopy at the Radioactive Isotope Beam Factory (RIKEN). Several low-lying yrast states are observed to decay predominantly by γ-ray emission. In contrast, the state–predicted to be strongly populated in the one-proton knockout reaction–is notably absent, suggesting that it decays primarily via prompt proton emission. We show that even for such an unbound system, shell-model calculations based on a harmonic oscillator potential reproduce the observed mirror energy differences remarkably well in all the observed states. Based on this result, we propose that a general pattern might emerge where, in medium-mass systems at the proton drip line, the stronger Coulomb barrier together with the centrifugal barrier effectively confines the wave functions, so that the shell model is able to describe low-lying states, enabling accurate predictions of mirror energy differences between isobaric analogue states.
url
https://doi.org/10.1016/j.physletb.2026.140564View
Published (Version of record) Open CC BY V4.0

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