中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Shell evolution of N=40 isotones towards Ca-60: First spectroscopy of Ti-62

文献类型:期刊论文

作者Cortes, M. L.1,2; Rodriguez, W.1,3; Doornenbal, P.1; Obertelli, A.4,5; Holt, J. D.6; Lenzi, S. M.7,8; Menendez, J.9; Nowacki, F.10; Ogata, K.11,12; Poves, A.13,14
刊名PHYSICS LETTERS B
出版日期2020-01-10
卷号800页码:7
ISSN号0370-2693
关键词Shell evolution Radioactive beams Gamma-ray spectroscopy
DOI10.1016/j.physletb.2019.135071
通讯作者Cortes, M. L.(liliana.cortes@lnl.infn.it)
英文摘要Excited states in the N = 40 isotone Ti-62 were populated via the V-63( p, 2p)Ti-62 reaction at similar to 200MeV/nucleonat the Radioactive Isotope Beam Factory and studied using gamma-ray spectroscopy. The energies of the 2(1)(+) -> 0(gs)(+) and 4(1)(+) -> 2(1)(+) transitions, observed here for the first time, indicate a deformed Ti-62 ground state. These energies are increased compared to the neighboring Cr-64 and Fe-66 isotones, suggesting a small decrease of quadrupole collectivity. The present measurement is well reproduced by large-scale shell-model calculations based on effective interactions, while ab initio and beyond mean-field calculations do not yet reproduce our findings. The shell-model calculations for Ti-62 show a dominant configuration with four neutrons excited across the N = 40 gap. Likewise, they indicate that the N = 40 island of inversion extends down to Z = 20, disfavoring a possible doubly magic character of the elusive Ca-60. (C) 2019 The Authors. Published by Elsevier B.V.
WOS关键词MAGIC NUMBER ; DEFORMATION ; SCATTERING ; STATE ; DECAY ; BE-12
资助项目Japan Society for the Promotion of Science (JSPS)[JP16K05352] ; Ministerio de Ciencia, Innovacion y Universidades(Spain)[SEV-2016-0597] ; Ministerio de Ciencia, Innovacion y Universidades(Spain)[PGC-2018-94583] ; RIKEN Special Postdoctoral Researcher Program ; Vietnam Ministry of Science and Technology (MOST) through the Physics Development Program[DTDLCN.25/18] ; HIC for FAIR ; Croatian Science Foundation[1257] ; Croatian Science Foundation[7194] ; European Regional Development Fund[GINOP-2.3.3-15-2016-00034] ; National Research, Development and Innovation Fund of Hungary[K128947] ; Spanish Ministerio de Economia y Competitividad[FPA2017-84756-C4-2-P] ; National Research Foundation of Korea[2018R1A5A1025563] ; National Research Foundation of Korea[2019M7A1A1033186] ; European Research Council through the ERC[MINOS-258567] ; JSPS KAKENHI[18K03639] ; MEXT ; Joint Institute for Computational Fundamental Science (JICFuS) ; CNS-RIKEN joint project for large-scale nuclear structure calculations ; Natural Sciences and Engineering Research Council (NSERC) of Canada ; Deutsche Forschungsgemeinschaft[279384907 - SFB 1245] ; PRISMA Cluster of Excellence ; BMBF[05P18RDFN1] ; BMBF[05P19RDFN1] ; National Research Council Canada
WOS研究方向Astronomy & Astrophysics ; Physics
语种英语
出版者ELSEVIER
WOS记录号WOS:000503832500053
资助机构Japan Society for the Promotion of Science (JSPS) ; Ministerio de Ciencia, Innovacion y Universidades(Spain) ; RIKEN Special Postdoctoral Researcher Program ; Vietnam Ministry of Science and Technology (MOST) through the Physics Development Program ; HIC for FAIR ; Croatian Science Foundation ; European Regional Development Fund ; National Research, Development and Innovation Fund of Hungary ; Spanish Ministerio de Economia y Competitividad ; National Research Foundation of Korea ; European Research Council through the ERC ; JSPS KAKENHI ; MEXT ; Joint Institute for Computational Fundamental Science (JICFuS) ; CNS-RIKEN joint project for large-scale nuclear structure calculations ; Natural Sciences and Engineering Research Council (NSERC) of Canada ; Deutsche Forschungsgemeinschaft ; PRISMA Cluster of Excellence ; BMBF ; National Research Council Canada
源URL[http://119.78.100.186/handle/113462/141372]  
专题中国科学院近代物理研究所
通讯作者Cortes, M. L.
作者单位1.RIKEN, Nishina Ctr, 2-1 Hirosawa, Wako, Saitama 3510198, Japan
2.Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Legnaro, Italy
3.Univ Nacl Colombia, Sede Bogota, Fac Ciencias, Dept Fis, Bogota 111321, Colombia
4.Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France
5.Tech Univ Darmstadt, Inst Kernphys, D-64289 Darmstadt, Germany
6.TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3, Canada
7.Univ Padua, Dipartimento Fis & Astron, Via F Marzolo 8, I-35131 Padua, Italy
8.Ist Nazl Fis Nucl, Sez Padova, Via F Marzolo 8, I-35131 Padua, Italy
9.Univ Tokyo, Ctr Nucl Study, RIKEN Campus, Wako, Saitama 3510198, Japan
10.Univ Strasbourg, IPHC, CNRS IN2P3, F-67037 Strasbourg, France
推荐引用方式
GB/T 7714
Cortes, M. L.,Rodriguez, W.,Doornenbal, P.,et al. Shell evolution of N=40 isotones towards Ca-60: First spectroscopy of Ti-62[J]. PHYSICS LETTERS B,2020,800:7.
APA Cortes, M. L..,Rodriguez, W..,Doornenbal, P..,Obertelli, A..,Holt, J. D..,...&Zanetti, L..(2020).Shell evolution of N=40 isotones towards Ca-60: First spectroscopy of Ti-62.PHYSICS LETTERS B,800,7.
MLA Cortes, M. L.,et al."Shell evolution of N=40 isotones towards Ca-60: First spectroscopy of Ti-62".PHYSICS LETTERS B 800(2020):7.

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来源:近代物理研究所

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