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《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.
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  • [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)
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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
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Received: 2017-06-22
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    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

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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.

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