×
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

Stability of super heavy nuclei associated with the updated nuclear data

  • The stability of super heavy nuclei (SHN) from Z=104 to Z=126 is analyzed systematically, associated with the following theoretical mass tables:FRDM2012[At. Data Nucl. Data Tables 109-110(2016)], WS2010[Phys. Rev. C 82, 044304(2010)], WS-LZ-RBF[J. Phys. G:Nucl. Part. Phys. 42, 095107(2015)] and the updated experimental data AME2016[Chinese Physics C 41, 040002(2017)]. The nucleus with the biggest mean binding energy in each isotopic chain shows systematic regular behavior, indicating that the mean binding energy is a good criterion to classify SHN by their stability. Based on binding energy, the α-decay energy Qα, two-proton separation energy S2p, and two-neutron separation energy S2n are extracted and analyzed. It is found that N=152 and N=162 are sub-magic numbers, N=184 is a neutron magic number, and Z=114 is a proton magic number, which may provide useful information for the synthesis and identification of SHN.
      PCAS:
  • 加载中
  • [1] A. Sobiczewski, F. Gareev, and B. Kalinkin, Phys. Lett., 22:500(1966)
    [2] S. Hofmann and G. Mnzenberg, Rev. Mod. Phys., 72:733(2000)
    [3] S. Hofmann, D. Ackermann, S. Antaic,P. Cagarda, B. Kindler, P. Kuusiniemi, M. Leino, B. Lommel, O. Malyshev et al, Nucl. Phys. A, 734:93(2004)
    [4] Yu.Ts. Oganessian, V. Utyonkov, Y. V. Lobanov, F. S. Abdullin, A. Polyakov, L. Shirokovsky, Y. S. Tsyganov, G. Gulbekian, S. Bogomolov, A. Mezentsev et al, Phys. Rev. C, 69:021601(2004)
    [5] Yu.Ts. Oganessian, V. Utyonkov, Y. V. Lobanov, F. S. Abdullin, A. Polyakov, L. Shirokovsky, Y. S. Tsyganov, G. Gulbekian, S. Bogomolov, B. gikal et al, Phys. Rev. C, 70:064609(2004)
    [6] Yu.Ts. Oganessian, V. Utyonkov, S. Dmitriev, Y. V. Lobanov, M. Itkis, A. Polyakov, Y. S. Tsyganov, A. Mezentsev, A. Mezentsev, A. Yeremin, A. Voinov et al, Phys. Rev. C, 72:034611(2005)
    [7] Yu.Ts. Oganessian, V. Utyonkov, Y. V. Lobanov, F. S. Abdullin, A. Polyakov, R. Sagaidak, I. Shirokovsky, Y. S. Tsyganov, A. Voinov, G. Gulbekian et al, Phys. Rev. C, 74:044602(2006)
    [8] Yu.Ts. Oganessian, V. Utyonkov, Y. V. Lobanov, F. S. Abdullin, A. N. Polyakov, R. N. Sagaidak, I. V. Shirokovsky, Y. S. Tsyganov, A. A. Voinov, G. G. Gulbekian et al, Phys. Rev. C, 76:011601(2007)
    [9] Yu.Ts. Oganessian, F. S. Abdullin, P. Bailey, D. Benker, M. Bennett, S. Dmitriev, J. G. Ezold, J. Hamilton, R. A. Henderson, M. Itkis et al, Phys. Rev. Lett., 104:142502(2010)
    [10] Kosuke Morita, Kouji Morimoto, Daiya Kaji, Takhiro Akiyama, Sin-ichi Goto, Hiromitsu Haba et al, Journal of the physical Society of Japan, 73(10):2593-2596(2004)
    [11] S. Patra, C. L. Wu, C. Praharaj, and R. K. Gupta, Nucl. Phys. A, 651:117(1999)
    [12] P. Mohr et al, Phys. Rev. C, 73:031301(2006)
    [13] P. Mller, W. D. Myers, H. Sagawa, and S. Yoshida, Phys. Rev. Lett., 108:052501(2012)
    [14] N. Wang, M. Liu and X. Wu, Phys. Rev. C, 81:044322(2010)
    [15] N. Wang, Z. Liang, M. Liu, and X. Wu, Phys. Rev. C, 82:044304(2010)
    [16] M. Liu, N. Wang, Y. Deng, and X. Wu, Phys. Rev. C, 84:014333(2011)
    [17] V. Strutinsky and F. Ivanjuk, Nucl. Phys. A, 255:405(1975)
    [18] H. Zhang, J. Dong, N. Ma, G. Royer, J. Li, Nucl. Phys. A, 929:38(2014)
    [19] P. Moller and J. R. Nix, J. Phys. G:Nucl. Part. Phys., 20:1681(1994)
    [20] A. Baran, Z. Lojewski, K. Sieja, and M. Kowal, Phys. Rev. C, 72:044310(2005)
    [21] Z. Patyk and A. Sobiczewski, Nucl. Phys. A, 533:132(1991)
    [22] W. Myers and W. Swiatecki, Nucl. Phys. A, 601:141(1996)
    [23] R. Chasman and I. Ahmad, Phys. Lett. B, 392:255(1997)
    [24] V. Strutinsky et al, Nucl. Phys. A, 122:1(1968)
    [25] S. Ćwiok and J. Dobaczewski, P. H. Heenen, P. Magierski, and W. Nazarewicz, Nucl. Phys. A, 611:211(1996)
    [26] A. Kruppa, M. Bender, W. Nazarewicz, P. G. Reinhard, and T. Vertse, Phys. Rev. C, 61:034313(2000)
    [27] M. Bender, K. Rutz, P. G. Reinhard, J. A. Maruhn, and W. Greiner, Phys. Rev. C, 60:034304(1999)
    [28] K. Rutz, M. Bender, T. Brvenich, T. Schilling, P. G. Reinhard, J. Maruhn, and W. Greiner, Phys. Rev. C, 56:238(1997)
    [29] S. Goriely, N. Chamel, and J. Pearson, Phys. Rev. C, 88:061302(2013)
    [30] M. Wang, G. Audi et al, Chinese Physics C, 41:040002(2017)
    [31] N. N. Ma, H. F. Zhang, X. J. Bao, P. H. Chen, J. M. Dong, J. Q. Li, and H. F. Zhang, J. Phys. G:Nucl. Part. Phys., 42:095107(2015)
    [32] P. Mller, A. Sierk, T. Ichikawa, and H. Sagawa, At. Data Nucl.Data Tab., 109:1(2016)
    [33] Jun-Hong Liu, Shu-Qing Guo, Xiao-Jun Bao, and Hong-Fei Zhang, Chinese Physics C, 41:074106(2017)
    [34] P. Mller, J. Nix, W. Myers, and W. Swiatecki, At. Data Nucl. Data Tab., 59:185(1995)
    [35] K. Rutz, M. Bender, T. Brvenich, T. Schilling, P. G. Reinhard, J. Maruhn, and W. Greiner, Phys. Rev. C, 56:238(1997)
    [36] M. Ismail, W. M. Seif, and A. Abdurrahman, Phys. Rev. C, 94:024316(2016)
    [37] J. Dvorak, R. Krcken, F. Nebel, Z. Novackova, A. Semchenkov, A. Trler, B. Wierczinski, and A. Yakushev, Phys. Rev. C, 94:024316(2016)
  • 加载中

Get Citation
Peng-Cheng Li, Hong-Fei Zhang and Yong-Jia Wang. Stability of super heavy nuclei associated with the updated nuclear data[J]. Chinese Physics C, 2017, 41(11): 114103. doi: 10.1088/1674-1137/41/11/114103
Peng-Cheng Li, Hong-Fei Zhang and Yong-Jia Wang. Stability of super heavy nuclei associated with the updated nuclear data[J]. Chinese Physics C, 2017, 41(11): 114103.  doi: 10.1088/1674-1137/41/11/114103 shu
Milestone
Received: 2017-06-22
Fund

    Supported by National Natural Science Foundation of China (11675066, 11647306), Fundamental Research Funds for the Central Universities (lzujbky-2017-ot04) and Feitian Scholar Project of Gansu province

Article Metric

Article Views(1594)
PDF Downloads(60)
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:

Stability of super heavy nuclei associated with the updated nuclear data

    Corresponding author: Hong-Fei Zhang,
  • 1.  School of Nuclear Science and Technology, Lanzhou University, Lanzhou 730000, China
  • 2. School of Nuclear Science and Technology, Lanzhou University, Lanzhou 730000, China
  • 3. Joint Department for Nuclear Physics, Lanzhou University and Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
  • 4.  School of Science, Huzhou University, Huzhou 313000, China
Fund Project:  Supported by National Natural Science Foundation of China (11675066, 11647306), Fundamental Research Funds for the Central Universities (lzujbky-2017-ot04) and Feitian Scholar Project of Gansu province

Abstract: The stability of super heavy nuclei (SHN) from Z=104 to Z=126 is analyzed systematically, associated with the following theoretical mass tables:FRDM2012[At. Data Nucl. Data Tables 109-110(2016)], WS2010[Phys. Rev. C 82, 044304(2010)], WS-LZ-RBF[J. Phys. G:Nucl. Part. Phys. 42, 095107(2015)] and the updated experimental data AME2016[Chinese Physics C 41, 040002(2017)]. The nucleus with the biggest mean binding energy in each isotopic chain shows systematic regular behavior, indicating that the mean binding energy is a good criterion to classify SHN by their stability. Based on binding energy, the α-decay energy Qα, two-proton separation energy S2p, and two-neutron separation energy S2n are extracted and analyzed. It is found that N=152 and N=162 are sub-magic numbers, N=184 is a neutron magic number, and Z=114 is a proton magic number, which may provide useful information for the synthesis and identification of SHN.

    HTML

Reference (37)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return