×
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

Predictions of decay modes for the superheavy nuclei most suitable for synthesis

  • The competition between α-decay and spontaneous fission of superheavy nuclei (SHN) is investigated by the generalized liquid drop model (GLDM) and the modified Swiatecki's formula respectively. The theoretical decay modes are in good agreement with the experimental results. Predictions are made for as-yet unobserved superheavy nuclei. The theoretical calculations show that the nuclei 298120, 295119, 290118, 291117, 287117, 294116, 289116, 286116, 285116, 284115, 283115, 283114, 282114, 280113, 276112, 275112, 274112, 273111, 272110, 265109 may be synthesized experimentally in the near future since they not only have relatively large predicted cross sections but can also be identified via α-decay chains.
      PCAS:
  • 加载中
  • [1] S. Hofmann and G. Munzenberg, Rev. Mod. Phys., 72: 733 (2000)
    [2] S. Hofmann, Radiochim. Acta., 99: 405 (2011)
    [3] K. Morita et al, J. Phys. Soc. Jpn., 76: 045001 (2007)
    [4] Yu. Ts. Oganessian et al, Phys. Rev. C, 70: 064609 (2004)
    [5] Yu. Ts. Oganessian et al, Phys. Rev. C, 74: 044602 (2006)
    [6] Yu. Ts. Oganessian et al, Phys. Rev. Lett., 104: 142502 (2010)
    [7] A. Baran, Z. Lojewski, K. Sieja and M. Kowal, Phys. Rev. C, 72: 044310 (2005)
    [8] D. N. Poenaru, R. A. Gherghescu and W. Greiner, J. Phys. G, 40: 105105 (2013)
    [9] Y. Qian and Z. Ren, Phys. Rev. C, 90: 064308 (2014)
    [10] A. Staszczak, A. Baran and W. Nazarewicz, Phys. Rev. C, 87: 024320 (2013)
    [11] K.P. Santhosh and B. Priyanka, Phys. Rev. C, 87: 064611 (2013)
    [12] K. P. Santhosh and B. Priyanka, Phys. Rev. C, 89: 064604 (2014)
    [13] P. Mller and J. R. Nix, Nucl. Phys. A, 549: 84 (1992)
    [14] P. R. Chowdhury, D. N. Basu and C. Samanta, Phys. Rev. C, 75: 047306 (2007)
    [15] D. S. Delion, R. J. Liotta and R. Wyss, Phys. Rev. C, 76: 044301 (2007)
    [16] V. Y. Denisov and A. A. Khudenko, Phys. Rev. C, 81: 034613 (2010)
    [17] A. I. Budaca and I. Silisteanu, Phys. Rev. C, 88: 044618 (2013)
    [18] Y. Qian, Z. Ren and D. Ni, Phys. Rev. C, 89: 024318 (2014)
    [19] P. Jachimowicz, M. Kowal and J. Skalski, Phys. Rev. C, 89: 024304 (2014)
    [20] K. Varga, R. G. Lovas and R. J. Liotta, Phys. Rev. Lett., 69: 37 (1992)
    [21] B. Buck, A. C. Merchant and S. M. Perez, Phys. Rev. C, 51: 559 (1995)
    [22] G. Royer, Nucl. Phys. A, 848: 279 (2010)
    [23] P. Mohr, Phys. Rev. C, 73: 031301 (2006)
    [24] C. Xu and Z. Ren, Phys. Rev. C, 74: 014304 (2006)
    [25] D. N. Poenaru, I. H. Plonski and W. Greiner, Phys. Rev. C, 74: 014312 (2006)
    [26] C. Qi, F. R. Xu, R. J. Liotta and R. Wyss, Phys. Rev. Lett., 103: 072501 (2009)
    [27] H. F. Zhang and G. Royer, Phys. Rev. C, 77: 054318 (2008)
    [28] D. Ni and Z. Ren, Nucl. Phys. A, 825: 145 (2009)
    [29] X. Bao, H. Zhang, H. Zhang, G. Royer and J. Li, Nucl. Phys. A, 921: 85 (2014)
    [30] M. Bender, W. Nazarewicz and P. G. Reinhard, Phys. Lett. B, 515: 42 (2001)
    [31] A. Sobiczewski and I. Muntian, Nucl. Phys. A, 734: 176 (2004)
    [32] A. Dobrowolski, K. Pomorski and J. Bartel, Phys. Rev. C, 75: 024613 (2007)
    [33] R. Smolanczuk, J. Skalski and A. Sobiczewski, Phys. Rev. C, 52: 1871 (1995)
    [34] R. Smolanczuk, Phys. Rev. C, 56: 812 (1997)
    [35] A. Sobiczewski and K. Pomorski, Prog. Part. Nucl. Phys, 58: 292 (2007)
    [36] Glenn T. Seaborg, Phys. Rev., 85: 157 (1952)
    [37] W. WhiteHouse and W. Galbraith, Nature, 169: 494 (1952)
    [38] J. R. Huizenga, Phys. Rev., 94: 158 (1954)
    [39] W. Swiatecki, Phys. Rev., 100: 937 (1955)
    [40] X. J. Bao, S. Q. Guo, H. F. Zhang, Y. Z. Xing, J. M. Dong and J. Q. Li, J. Phys. G, 42: 085101 (2015)
    [41] X. J. Bao, Y. Gao, J. Q. Li and H. F. Zhang, Phys. Rev. C, 92: 034612 (2015)
    [42] X. J. Bao, Y. Gao, J. Q. Li and H. F. Zhang, Phys. Rev. C, 93: 044615 (2016)
    [43] G. Royer and R. A. Gherghescu, Nucl. Phys. A, 699: 479 (2002)
    [44] H. F. Zhang, G. Royer, Y. J. Wang, J. M. Dong, W. Zuo and J. Q. Li, Phys. Rev. C, 80: 057301 (2009)
    [45] A. Sobiczewski, Z. Patyk, and S. Cwiok, Phys. Lett. B, 224: 1 (1989)
    [46] V. E. Viola, Jr. and G. T. Seaborg, J. Inorg. Nucl. Chem., 28: 741 (1966)
    [47] G. Royer, J. Phys. G: Nucl. Part. Phys., 26: 1149(2000)
    [48] H.F. Zhang, Y. Gao, N. Wang, J.Q. Li, E.G. Zhao and G.Royer, Phys. Rev. C, 85: 014325 (2012).
    [49] N. Wang, M. Liu, X. Z. Wu, J Meng, Phys. Lett. B, 734: 215(2014)
    [50] Y. Z. Wang at al, Phys. Rev. C, 92: 064301 (2015)
    [51] Mller P, Nix J, Myers W and Swiatecki W, At. DataNucl.Data Tables, 59: 185 (1995)
    [52] Yu Ts Oganessian, V K Utyonkov, Rep. Prog. Phys., 78:036301 (2015)
    [53] J. Dong, W. Zuo and W. Scheid, Phys. Rev. Lett., 107: 012501(2011)
    [54] Z. Ren and C. Xu, Nucl. Phys. A, 759: 64 (2005)
    [55] C. Xu, Z. Ren and Y. Guo, Phys. Rev. C, 78: 044329 (2008)
    [56] M. Warda and J. L. Egido, Phys. Rev. C, 86: 014322 (2012)
    [57] K. P. Santhosh and C. Nithya, Phys. Rev. C, 94: 054621 (2016)
  • 加载中

Get Citation
Jun-Hong Liu, Shu-Qing Guo, Xiao-Jun Bao and Hong-Fei Zhang. Predictions of decay modes for the superheavy nuclei most suitable for synthesis[J]. Chinese Physics C, 2017, 41(7): 074106. doi: 10.1088/1674-1137/41/7/074106
Jun-Hong Liu, Shu-Qing Guo, Xiao-Jun Bao and Hong-Fei Zhang. Predictions of decay modes for the superheavy nuclei most suitable for synthesis[J]. Chinese Physics C, 2017, 41(7): 074106.  doi: 10.1088/1674-1137/41/7/074106 shu
Milestone
Received: 2017-03-05
Fund

    Supported by National Natural Science Foundation of China (11675066) and Feitian Scholar Project of Gansu Province

Article Metric

Article Views(1743)
PDF Downloads(40)
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:

Predictions of decay modes for the superheavy nuclei most suitable for synthesis

    Corresponding author: Hong-Fei Zhang,
  • 1.  School of Nuclear Science and Technology, Lanzhou University, Lanzhou 730000, China
  • 2.  College of Physics and Information Science, Hunan Normal University, Changsha 410006, China
Fund Project:  Supported by National Natural Science Foundation of China (11675066) and Feitian Scholar Project of Gansu Province

Abstract: The competition between α-decay and spontaneous fission of superheavy nuclei (SHN) is investigated by the generalized liquid drop model (GLDM) and the modified Swiatecki's formula respectively. The theoretical decay modes are in good agreement with the experimental results. Predictions are made for as-yet unobserved superheavy nuclei. The theoretical calculations show that the nuclei 298120, 295119, 290118, 291117, 287117, 294116, 289116, 286116, 285116, 284115, 283115, 283114, 282114, 280113, 276112, 275112, 274112, 273111, 272110, 265109 may be synthesized experimentally in the near future since they not only have relatively large predicted cross sections but can also be identified via α-decay chains.

    HTML

Reference (57)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return