×
近期发现有不法分子冒充我刊与作者联系,借此进行欺诈等不法行为,请广大作者加以鉴别,如遇诈骗行为,请第一时间与我刊编辑部联系确认(《中国物理C》(英文)编辑部电话:010-88235947,010-88236950),并作报警处理。
本刊再次郑重声明:
(1)本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
(2)本刊采编系统作者中心是投稿的唯一路径,该系统为ScholarOne远程稿件采编系统,仅在本刊投稿网网址(https://mc03.manuscriptcentral.com/cpc)设有登录入口。本刊不接受其他方式的投稿,如打印稿投稿、E-mail信箱投稿等,若以此种方式接收投稿均为假冒。
(3)所有投稿均需经过严格的同行评议、编辑加工后方可发表,本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿,并收取发表费用,均为假冒。
                  
《中国物理C》(英文)编辑部
2024年10月30日

Shell-model calculations for the semi-magic nucleus 85Br and systematic features of the N=50 odd-A isotones

  • Level structures of 85Br have been investigated using the shell-model code nushellx within a large model space containing the neutron-core excitations across the N=50 closed shell. The calculated results have been compared with the available experimental data. Reasonable agreement between the experimental and calculated values is obtained, which indicates that the neutron-core excitations are essential to reproduce the level structures of 85Br. The systematic features of neutron-core excitations in the N=50 isotones are investigated.
      PCAS:
  • 加载中
  • [1] C. Plettner et al, Phys. Rev. Lett., 85:2454 (2000)
    [2] J. Ljungvall et al, Phys. Rev. Lett., 100:102502 (2008)
    [3] R. Wadsworth et al, Phys. Lett. B, 701:306 (2011)
    [4] H. Schnare et al, Phys. Rev. Lett., 82:4408 (1999)
    [5] R. Schwengner et al, Phys. Rev. C, 66:024310 (2002)
    [6] S. Y. Wang et al, Phys. Lett. B, 703:40 (2011)
    [7] C. Liu et al, Phys. Rev. Lett., 116:112501 (2016)
    [8] J. K. Hwang, J. H. Hamilton, and A. V. Ramayya, Int. Jou. Mod. Phys. E, 21:1250020 (2012)
    [9] A. Gade et al, Phys. Rev. C, 81:064326 (2010)
    [10] A. Prvost et al, Eur. Phys. J. A, 22:391 (2004)
    [11] G. Winter, R. Schwengner, J. Reif, H. Prade, L. Funke, R. Wirowski, N. Nicolay, A. Dewald, and P. von Brentano, Phys. Rev. C, 48:1010 (1993)
    [12] E. A. Stefanova et al, Nucl. Phys. A, 669:14 (2000)
    [13] F. Ghazi Moradi et al, Phys. Rev. C, 89:044310 (2014)
    [14] Y. H. Zhang et al, Phys. Rev. C, 70:024301 (2004)
    [15] N. Fotiades et al, Phys. Rev. C, 71:064312 (2005)
    [16] Z. Q. Li et al, Phys. Rev. C, 94:014315 (2016)
    [17] F. Ghazi Moradi et al, Phys. Rev. C, 89:014301 (2014)
    [18] O. Sorlin, and M.-G. Porquet, Prog. Part. Nucl. Phys., 61:602 (2008)
    [19] T. Rzaca-Urban, W. Urban, J. L. Durell, A. G. Smith, and I. Ahmad, Phys. Rev. C, 76:027302 (2007)
    [20] K. Sieja, and F. Nowacki, Phys. Rev. C, 85:051301 (2012)
    [21] H. A. Roth et al, Phys. Rev. C, 50:1330 (1994)
    [22] J. Hakala et al, Phys. Rev. Lett., 101:052502 (2008)
    [23] A. Astier et al, Eur. Phys. J. A, 30:541 (2006)
    [24] D. Zwarts, Comput. Phys. Commun., 38:365 (1985)
    [25] T. Engeland, M. Hjorth-Jensen, and E. Osnes, Nucl. Phys. A, 701:416C (2002)
    [26] L. I. Govor, A. M. Demidov, V. A. Kurkin, and I. V. Mikhailov, Phys. At. Nucl., 71:1339 (2008)
    [27] P. E. Garrett et al, Phys. Rev. C, 68:024312 (2003)
    [28] P. W. Luo et al, Phys. Rev. C, 89:034318 (2014)
    [29] E. Sahin et al, Nucl. Phys. A, 893:1 (2012)
    [30] M. G. Porquet et al, Phys. Rev. C, 84:054305 (2011)
    [31] E. K. Warburton, J. W. Olness, C. J. Lister, R. W. Zurmuhle, and J. A. Becker, Phys. Rev. C, 31:1184 (1985)
    [32] P. C. Li, and W. W. Daehnick, Nucl. Phys. A, 462:26 (1987)
    [33] H. Fann, J. P. Schiffer, and U. Strohbusch, Phys. Lett. B, 44:19 (1973)
    [34] N. S. Pattabiraman, S. N. Chintalapudi, S. S. Ghugre, B. V. Tirumala Rao, M. L. N. Raju, T. Seshi Reddy, P. K. Joshi, R. Palit, and H. C. Jain, Phys. Rev. C, 65:044324 (2002)
    [35] T. Otsuka, T. Suzuki, R. Fujimoto, H. Grawe, and Y. Akaishi, Phys. Rev. Lett., 95:232502 (2005)
  • 加载中

Get Citation
Rui-Ju Guo, Zhi-Quan Li, Chen Liu, Yong-He Tian and Shou-Yu Wang. Shell-model calculations for the semi-magic nucleus 85Br and systematic features of the N=50 odd-A isotones[J]. Chinese Physics C, 2017, 41(8): 084105. doi: 10.1088/1674-1137/41/8/084105
Rui-Ju Guo, Zhi-Quan Li, Chen Liu, Yong-He Tian and Shou-Yu Wang. Shell-model calculations for the semi-magic nucleus 85Br and systematic features of the N=50 odd-A isotones[J]. Chinese Physics C, 2017, 41(8): 084105.  doi: 10.1088/1674-1137/41/8/084105 shu
Milestone
Received: 2017-03-16
Fund

    Supported by Natural Science Foundation of China (11622540,11461141001,U1432119) and Computations were Carried Out on an HP Proliant DL785G6 Server Hosted by the Institute of Space Science of Shandong University

Article Metric

Article Views(1516)
PDF Downloads(29)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Shell-model calculations for the semi-magic nucleus 85Br and systematic features of the N=50 odd-A isotones

    Corresponding author: Shou-Yu Wang,
  • 1. Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai 264209, China
Fund Project:  Supported by Natural Science Foundation of China (11622540,11461141001,U1432119) and Computations were Carried Out on an HP Proliant DL785G6 Server Hosted by the Institute of Space Science of Shandong University

Abstract: Level structures of 85Br have been investigated using the shell-model code nushellx within a large model space containing the neutron-core excitations across the N=50 closed shell. The calculated results have been compared with the available experimental data. Reasonable agreement between the experimental and calculated values is obtained, which indicates that the neutron-core excitations are essential to reproduce the level structures of 85Br. The systematic features of neutron-core excitations in the N=50 isotones are investigated.

    HTML

Reference (35)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return