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(1495)
PDF Downloads(59)
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