Evolution of high-spin states in neutron-rich Au isotopes approaching the shell closure
Y. Cho · Y. H. Kim · A. Navin · M. Rejmund · A. Lemasson · D. Ramos · E. Clement · C. Yuan · M. Liu · P. van Isacker · A. N. Andreyev · J. Dudouet and 39 other authors
\textbf{Background: } The nuclear structure in the region southwest of the doubly magic Pb is important to benchmark theoretical models relevant for neutron-rich heavy element formation and for the origin of the peak in the mass abundance distribution. Although neutron-rich Pb, Tl, and Hg () isotopes are relatively well studied, experimental data for neutron-rich Au isotopes () remain largely limited due to experimental challenges. \textbf{Purpose: } The purpose of this work is to investigate the evolution of the high-spin structure in neutron-rich Au isotopes near the shell closure and to characterize the underlying shell-model configurations, with a particular focus on the roles of the high- unique-parity and orbitals. \textbf{Methods: } Neutron-rich Au isotopes were produced using multi-nucleon transfer reactions of Pt(Xe, I)Au at a beam energy of 7 MeV/u. %between a 7 MeV/u Xe beam and a Pt target at GANIL. Prompt and delayed -ray spectroscopy of isotopically identified reaction products was performed with a unique experimental setup combining the VAMOS++ large acceptance magnetic spectrometer, the AGATA HPGe -ray tracking array, and the CATLIFE detection system.