Evolution of high-spin states in neutron-rich Au195–202 isotopes approaching the N=126 shell closure
Abstract
\textbf{Background: } The nuclear structure in the region southwest of the doubly magic 208Pb is important to benchmark theoretical models relevant for neutron-rich heavy element formation and for the origin of the A≈195 peak in the mass abundance distribution. Although neutron-rich Pb, Tl, and Hg (Z=80−82) isotopes are relatively well studied, experimental data for neutron-rich Au isotopes (Z=79) 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 N=126 shell closure and to characterize the underlying shell-model configurations, with a particular focus on the roles of the high-j unique-parity πh11/2 and νi13/2 orbitals. \textbf{Methods: } Neutron-rich 195−202Au isotopes were produced using multi-nucleon transfer reactions of 198Pt(136Xe, xI)yAu at a beam energy of 7 MeV/u. %between a 7 MeV/u 136Xe beam and a 198Pt target at GANIL. Prompt and delayed γ-ray spectroscopy of isotopically identified reaction products was performed with a unique experimental setup combining the VAMOS++ large acceptance magnetic spectrometer, the AGATA HPGe γ-ray tracking array, and the CATLIFE detection system.
Versions
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BibTeX
@article{cho2026evolution,
title = {{Evolution of high-spin states in neutron-rich Au195–202 isotopes approaching the N=126 shell closure}},
author = {Y Cho and Y.H Kim and A Navin and M Rejmund and A Lemasson and D Ramos and E Clément and C Yuan and M Liu and P van Isacker and A.N Andreyev and J Dudouet and S Choi and Y Son and A Mukherjee and D Ackermann and G de Angelis and S Bae and R Banik and S Bhattacharya and S Bhattacharyya and K Chae and F Didierjean and C Fougéres and G de France and G Fremont and J Goupil and G.M Gu and J Ha and K.I Hahn and Y Hirayama and S Jeong and D.T Kattikat Melcom and C.H Kim and M.J Kim and S.H Kim and W Korten and P Marini and H Miyatake and M Mukai and G Mukherjee and T Niwase and T Otsuka and J Park and R.M Pérez-Vidal and F Recchia and K Rezynkina and P Schury and J.C Thomas and I Tsekhanovich and A Utepov and Y.X Watanabe},
journal = {Phys.Rev.C},
year = {2026},
month = sep,
doi = {10.1103/nclr-tjv1},
eprint = {2610.07058},
archivePrefix = {arXiv},
url = {https://hal.science/hal-05759909v1},
note = {CC BY 4.0},
}
RIS
TY - JOUR
TI - Evolution of high-spin states in neutron-rich Au195–202 isotopes approaching the N=126 shell closure
AU - Y Cho
AU - Y.H Kim
AU - A Navin
AU - M Rejmund
AU - A Lemasson
AU - D Ramos
AU - E Clément
AU - C Yuan
AU - M Liu
AU - P van Isacker
AU - A.N Andreyev
AU - J Dudouet
AU - S Choi
AU - Y Son
AU - A Mukherjee
AU - D Ackermann
AU - G de Angelis
AU - S Bae
AU - R Banik
AU - S Bhattacharya
AU - S Bhattacharyya
AU - K Chae
AU - F Didierjean
AU - C Fougéres
AU - G de France
AU - G Fremont
AU - J Goupil
AU - G.M Gu
AU - J Ha
AU - K.I Hahn
AU - Y Hirayama
AU - S Jeong
AU - D.T Kattikat Melcom
AU - C.H Kim
AU - M.J Kim
AU - S.H Kim
AU - W Korten
AU - P Marini
AU - H Miyatake
AU - M Mukai
AU - G Mukherjee
AU - T Niwase
AU - T Otsuka
AU - J Park
AU - R.M Pérez-Vidal
AU - F Recchia
AU - K Rezynkina
AU - P Schury
AU - J.C Thomas
AU - I Tsekhanovich
AU - A Utepov
AU - Y.X Watanabe
PY - 2026
DA - 2026/09/23
JO - Phys.Rev.C
DO - 10.1103/nclr-tjv1
UR - https://hal.science/hal-05759909v1
AB - \textbf{Background: } The nuclear structure in the region southwest of the doubly magic ^208Pb is important to benchmark theoretical models relevant for neutron-rich heavy element formation and for the origin of the A≈195 peak in the mass abundance distribution. Although neutron-rich Pb, Tl, and Hg (Z=80−82) isotopes are relatively well studied, experimental data for neutron-rich Au isotopes (Z=79) 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 N=126 shell closure and to characterize the underlying shell-model configurations, with a particular focus on the roles of the high-j unique-parity πh_11/2 and νi_13/2 orbitals. \textbf{Methods: } Neutron-rich ^195−202Au isotopes were produced using multi-nucleon transfer reactions of ^198Pt(^136Xe, ^xI)^yAu at a beam energy of 7 MeV/u. %between a 7 MeV/u ^136Xe beam and a ^198Pt target at GANIL. Prompt and delayed γ-ray spectroscopy of isotopically identified reaction products was performed with a unique experimental setup combining the VAMOS++ large acceptance magnetic spectrometer, the AGATA HPGe γ-ray tracking array, and the CATLIFE detection system.
ER -