Regularity of core coupled high-spin structure in neutron-rich ${}^{196-202}$Au isotopes approaching N $=126$

Abstract

Excited states built upon long-lived high-spin isomers in hard-to-reach neutron-rich Au ($Z=79$) isotopes were populated using multi-nucleon transfer reactions between ${}^{136}$Xe and ${}^{198}$Pt at 7 MeV/u. These states in ${}^{196,198-202}$Au were identified for the first time using the powerful combination of the VAMOS++ spectrometer, the CATLIFE detection system, and the AGATA $\gamma$-ray tracking array. Their measured energies exhibit remarkable regularity as a function of neutron number and are seen to be inherited from the energies of yrast-band members in the corresponding Hg ($Z=80$) isotope. Large-scale shell-model calculations reproduce the observed regularity and show that these states arise from the unique-parity orbitals $\pi 0h_{11/2}$ and $\nu 0i_{13/2}$ coupled to the Hg core. This regularity is due to the dominant proton configurations of the Hg and Au isotopes, where the level energies are almost independent of different neutron-orbital occupancies. The calculated Au wave functions show significant higher-spin components of the corresponding Hg core, unlike what is expected in the conventional interpretation in terms of the weak-coupling/decoupling limits of the particle-core coupling model.

References in corpus (7)

• Nuclear magic numbers: new features far from stability
• AGATA - Advanced Gamma Tracking Array
• Evolution of shell structure in exotic nuclei
• Dual Position Sensitive MWPC for tracking reaction products at VAMOS++
• Production of new neutron-rich heavy nuclei with $Z=56-80$ in the multinucleon transfer reactions of ${}^{136}$Xe+${}^{198}$Pt
• Nuclear structure properties of ${}^{193-200}$Hg isotopes within large-scale shell model calculations
• Particle Identification at VAMOS++ with Machine Learning Techniques

Cited by in corpus (1)

• Evolution of high-spin states in neutron-rich ${}^{195-202}$Au isotopes approaching the $N=126$ shell closure