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Observation of a new isomer in 185Au

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【作者】 付翔宇刘忠A.N.Andreyev焦长峰董润妍张文强黄浩孙武陈启博张双全李健国周小红余兴汉曾全波D.SeweryniakB.AndelS.AntalicA.E.BarzakhM.BlockA.BronisM.P.CarpenterP.CoppJ.G.CubissD.T.DohertyP.Van DuppenZ.FavierF.GiacoppoB.KindlerF.G.KondevT.LauritsenB.LommelM.Al MontheryP.MosatC.RaisonW.ReviolG.SavardS.StolzeG.L.Wilson丁兵郭松郭成宇余永博吴迎峰

【Author】 X.Y.Fu;Z.Liu;A.N.Andreyev;C.F.Jiao;R.Y.Dong;W.Q.Zhang;H.Huang;W.Sun;Q.B.Chen;S.Q.Zhang;J.G.Li;X.H.Zhou;X.H.Yu;Q.B.Zeng;D.Seweryniak;B.Andel;S.Antalic;A.E.Barzakh;M.Block;A.Bronis;M.P.Carpenter;P.Copp;J.G.Cubiss;D.T.Doherty;P.Van Duppen;Z.Favier;F.Giacoppo;B.Kindler;F.G.Kondev;T.Lauritsen;B.Lommel;M.Al Monthery;P.Mosat;C.Raison;W.Reviol;G.Savard;S.Stolze;G.L.Wilson;B.Ding;S.Guo;C.Y.Guo;Y.B.Yu;Y.F.Wu;Institute of Modern Physics,Chinese Academy of Sciences;University of Chinese Academy of Sciences;School of Physics,Engineering and Technology,University of York;Advanced Science Research Center (ASRC),Japan Atomic Energy Agency;School of Physics and Astronomy,SUN YAT-SEN University;School of Physics,SUN YAT-SEN University;Department of Physics,East China Normal University;State Key Laboratory of Nuclear Physics and Technology,School of Physics,Peking University;Physics Division,Argonne National Laboratory;Department of Nuclear Physics and Biophysics,Comenius University in Bratislava;KU Leuven,Instituut voor Kern-en Stralingsfysica;Petersburg Nuclear Physics Institute,NRC Kurchatov Institute;Helmholtz-Institut Mainz;GSI Helmholtzzentrum für Schwerionenforschung Darmstadt;Johannes-Gutenberg Universit?t;School of Physics and Astronomy,University of Edinburgh;Department of Physics,University of Surrey;Irfu,CEA,Université Paris-Saclay;Department of Physics and Astronomy,Louisiana State University;

【机构】 Institute of Modern Physics,Chinese Academy of SciencesUniversity of Chinese Academy of SciencesSchool of Physics,Engineering and Technology,University of YorkAdvanced Science Research Center (ASRC),Japan Atomic Energy AgencySchool of Physics and Astronomy,SUN YAT-SEN UniversitySchool of Physics,SUN YAT-SEN UniversityDepartment of Physics,East China Normal UniversityState Key Laboratory of Nuclear Physics and Technology,School of Physics,Peking UniversityPhysics Division,Argonne National LaboratoryDepartment of Nuclear Physics and Biophysics,Comenius University in BratislavaKU Leuven,Instituut voor Kern-en StralingsfysicaPetersburg Nuclear Physics Institute,NRC Kurchatov InstituteHelmholtz-Institut MainzGSI Helmholtzzentrum für Schwerionenforschung DarmstadtJohannes-Gutenberg Universit?tSchool of Physics and Astronomy,University of EdinburghDepartment of Physics,University of SurreyIrfu,CEA,Université Paris-SaclayDepartment of Physics and Astronomy,Louisiana State University

【摘要】 Delayed γ-ray spectroscopy of 185Au was studied at the Argonne Gas-Filled Analyzer.A new isomer at an excitation energy of 1504.2(4) keV with a half-life of 630(80) ns was identified via γ-γ coincidence analysis,decaying via a 294.8(3) keV transition.Based on Weisskopf estimates,the multipolarity of the 295 keV transition is assigned to be E1,M1,E2,or M2.Possible configurations for this new isomer are discussed based on configurationconstrained potential energy surface calculations.

【Abstract】 Delayed γ-ray spectroscopy of 185Au was studied at the Argonne Gas-Filled Analyzer.A new isomer at an excitation energy of 1504.2(4) keV with a half-life of 630(80) ns was identified via γ-γ coincidence analysis,decaying via a 294.8(3) keV transition.Based on Weisskopf estimates,the multipolarity of the 295 keV transition is assigned to be E1,M1,E2,or M2.Possible configurations for this new isomer are discussed based on configurationconstrained potential energy surface calculations.

【基金】 Supported by the National Natural Science Foundation of China (12405140, 12135004, 11961141004, U2032138, 12275369);the Natural Science Foundation of Gansu Province, China (24JRRA033);financial support from the STFC;funded by the Chinese Academy of Sciences President’s International Fellowship Initiative (2020VMA0017);Supported by the U.S. Department of Energy, Office of Nuclear Physics, (DE-AC02-06CH11357, DE-FG02-94ER41041 (UNC), DE-FG02-97ER41033 (TUNL));supported by the Slovak Research and Development Agency (APVV-22-0282);Slovak Grant Agency VEGA (1/0019/25)
  • 【文献出处】 Chinese Physics C ,中国物理C(英文) , 编辑部邮箱 ,2025年08期
  • 【分类号】O571
  • 【下载频次】1
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