中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Isochronous mass measurements of T-z =-1 f p-shell nuclei from projectile fragmentation of Ni-58

文献类型:期刊论文

作者Zhang, Y. H.2,3,4; Zhang, P.1,2,3; Zhou, X. H.2,3,4; Wang, M.2,3,4; Litvinov, Yu A.2,3,5; Xu, H. S.2,3,4; Xu, X.2,3; Shuai, P.2,3; Lam, Y. H.2,3; Chen, R. J.2,3,5
刊名PHYSICAL REVIEW C
出版日期2018-07-18
卷号98期号:1页码:16
ISSN号2469-9985
DOI10.1103/PhysRevC.98.014319
英文摘要Atomic masses of seven T-z = -1, fp-shell nuclei from V-44 to Cu-56 and two low-lying isomers, V-44m (J(Pi) = 6(+)) and Co-52m (J(Pi) = 2(+)), have been measured with relative precisions of 1-4 x 10(-7 )with isochronous mass spectrometry (IMS) at the Cooler Storage Ring (CSRe), Lanzhou. The masses of Cu-56, Co-52g,Co-52m, and V-44m were measured for the first time in this experiment. The mass excesses (ME's) of V-44, Mn-48, Fe-50, and Ni-54 are determined with an order of magnitude improved precision compared to the literature values. Co-52g,Co-52m and Cu-56 are found to be 370 and 400 keV more bound, respectively, while V-44g,V-44m are similar to 300 KeV less bound than the extrapolations in the Atomic-Mass Evaluation 2012 (AME'12). The masses of the four T-z = -1/2 nuclei (45) V, Cr-47, Mn-49, and (51) Fe are re-determined to be in agreement, within the experimental errors, with the recent JYFLTRAP (University of Jyvaskyla, Finland) measurements or with the previous IMS measurements in CSRe. Details of the measurements and data analysis are described, and the impact of the new ME values on different aspects in nuclear structure are investigated and discussed.
WOS关键词PROTON-RICH NUCLEI ; FRS-ESR-FACILITY ; EXPERIMENTAL STORAGE-RING ; COULOMB ENERGIES ; EXOTIC NUCLEI ; HIRFL-CSR ; SPECTROMETRY ; IONS ; STATES ; DECAY
资助项目National Key R&D Program of China[2018YFA0404401] ; National Key R&D Program of China[2016YFA0400504] ; Key Research Program of Frontier Sciences of CAS[QYZDJ-SSW-SLH005] ; NSFC[U1232208] ; NSFC[U1432125] ; NSFC[11605248] ; NSFC[11605249] ; NSFC[11605252] ; NSFC[11605267] ; NSFC[11575112] ; NSFC[11575007] ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program[ERCCG 682841] ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; CAS[2009J2-23] ; CAS External Cooperation Program[GJHZ1305] ; HGF-CAS joint research group[HCJRG-108] ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Max Planck Society through the Max-Planck Partner Group
WOS研究方向Physics
语种英语
出版者AMER PHYSICAL SOC
WOS记录号WOS:000439059400002
资助机构National Key R&D Program of China ; National Key R&D Program of China ; Key Research Program of Frontier Sciences of CAS ; Key Research Program of Frontier Sciences of CAS ; NSFC ; NSFC ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; CAS ; CAS ; CAS External Cooperation Program ; CAS External Cooperation Program ; HGF-CAS joint research group ; HGF-CAS joint research group ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Max Planck Society through the Max-Planck Partner Group ; Max Planck Society through the Max-Planck Partner Group ; National Key R&D Program of China ; National Key R&D Program of China ; Key Research Program of Frontier Sciences of CAS ; Key Research Program of Frontier Sciences of CAS ; NSFC ; NSFC ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; CAS ; CAS ; CAS External Cooperation Program ; CAS External Cooperation Program ; HGF-CAS joint research group ; HGF-CAS joint research group ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Max Planck Society through the Max-Planck Partner Group ; Max Planck Society through the Max-Planck Partner Group ; National Key R&D Program of China ; National Key R&D Program of China ; Key Research Program of Frontier Sciences of CAS ; Key Research Program of Frontier Sciences of CAS ; NSFC ; NSFC ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; CAS ; CAS ; CAS External Cooperation Program ; CAS External Cooperation Program ; HGF-CAS joint research group ; HGF-CAS joint research group ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Max Planck Society through the Max-Planck Partner Group ; Max Planck Society through the Max-Planck Partner Group ; National Key R&D Program of China ; National Key R&D Program of China ; Key Research Program of Frontier Sciences of CAS ; Key Research Program of Frontier Sciences of CAS ; NSFC ; NSFC ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program ; European Research Council (ERC CG) under the EU Horizon 2020 research and innovation program ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum fur Schwerionenforschung, Darmstadt, Germany ; CAS ; CAS ; CAS External Cooperation Program ; CAS External Cooperation Program ; HGF-CAS joint research group ; HGF-CAS joint research group ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association ; Max Planck Society through the Max-Planck Partner Group ; Max Planck Society through the Max-Planck Partner Group
源URL[http://ir.bao.ac.cn/handle/114a11/20867]  
专题中国科学院国家天文台
通讯作者Zhou, X. H.; Wang, M.; Litvinov, Yu A.
作者单位1.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
2.Chinese Acad Sci, CAS Key Lab High Precis Nucl Spect, Inst Modern Phys, Lanzhou 730000, Gansu, Peoples R China
3.Chinese Acad Sci, Ctr Nucl Matter Sci, Inst Modern Phys, Lanzhou 730000, Gansu, Peoples R China
4.South China Normal Univ, Inst Modern Phys, Chinese Acad Sci, Joint Res Ctr Modern Phys & Clean Energy, Lanzhou 730000, Gansu, Peoples R China
5.GSI Helmholtzzentrum Schwerionenforsch, Planckstr 1, D-64291 Darmstadt, Germany
6.Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany
7.Chinese Acad Sci, Natl Astron Observ, CAS Key Lab Opt Astron, Beijing 100012, Peoples R China
8.Natl Lab Heavy Ion Accelerator Facil Lanzhou, Res Ctr Hadron Phys, Hefei 230026, Anhui, Peoples R China
9.Univ Sci & Technol China, Hefei 230026, Anhui, Peoples R China
10.Univ Paris 11, CNRS, IN2P3, CSNSM, F-91405 Orsay, France
推荐引用方式
GB/T 7714
Zhang, Y. H.,Zhang, P.,Zhou, X. H.,et al. Isochronous mass measurements of T-z =-1 f p-shell nuclei from projectile fragmentation of Ni-58[J]. PHYSICAL REVIEW C,2018,98(1):16.
APA Zhang, Y. H..,Zhang, P..,Zhou, X. H..,Wang, M..,Litvinov, Yu A..,...&Xu, F. R..(2018).Isochronous mass measurements of T-z =-1 f p-shell nuclei from projectile fragmentation of Ni-58.PHYSICAL REVIEW C,98(1),16.
MLA Zhang, Y. H.,et al."Isochronous mass measurements of T-z =-1 f p-shell nuclei from projectile fragmentation of Ni-58".PHYSICAL REVIEW C 98.1(2018):16.

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来源:国家天文台

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