Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
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
Chinese Physics C> 2018, Vol. 42> Issue(7) : 074103 DOI: 10.1088/1674-1137/42/7/074103

α particle preformation and shell effect for heavy andsuperheavy nuclei

  • 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, CAS, Lanzhou 730000, China

  • The α particle preformation factor is extracted within a generalized liquid drop model for Z=84-92 isotopes and N=126, 128, 152, 162, 176, 184 isotones. The calculated results show clearly that the shell effects play a key role in α particle preformation. The closer the proton and neutron numbers are to the magic numbers, the more difficult the formation of the α cluster inside the mother nucleus is. The preformation factors of the isotopes reflect that N=126 is a magic number for Po, Rn, Ra, and Th isotopes, but for U isotopes the weakening of the influence of the N=126 shell closure is evident. The trend of the factors for N=126 and N=128 isotones also support this conclusion. We extend the calculations for N=152, 162, 176, 184 isotones to explore the magic numbers for heavy and superheavy nuclei, which are probably present near Z=108 to N=152, 162 isotones and Z=116 to N=176, 184 isotones. The results also show that another subshell closure may exist after Z=124 in the superheavy nuclei. This is useful for future experiments.
      PCAS:
  • 加载中

  • References

    [1] Z. Ren and G. Xu, Phys. Rev. C, 36: 456 (1987)
    [2] R. G. Lovas, R. J. Liotta, A. Insolia, K. Varga, and D. S.Delion, Phys. Rep., 294: 265 (1998)
    [3] F. Garcia, O. Rodriguez, M. Gonalves, S. B. Duarte, O. A. P. Tavares, and F. Guzman, J. Phys. G, 26: 755 (2000)
    [4] G. Audi, O. Bersillon, J. Blachot, and A. H. Wapstra, Nucl. Phys. A, 729: 3 (2003)
    [5] T. N. Ginter et al, Phys. Rev. C, 67: 064609 (2003)
    [6] P. E. Hodgson and E. Betak, Phys. Rep., 374: 1 (2003)
    [7] Z. G. Gan, J. S. Guo, X. L. Wu, Z. Qin, H. M. Fan, X. G. Lei, H. Y. Liu, B. Guo, H. G. Xu, R. F. Chen, C. F. Dong, F. M. Zhang, H. L. Wang, C. Y. Xie, Z. Q. Feng, Y. Zhen, L. T. Song, P. Luo, H. S. Xu, X. H. Zhou, G. M. Jin, and Z. Ren, Eur. Phys. J. A, 20: 385 (2004)
    [8] D. Seweryniak et al, Phys. Rev. C, 73: 061301(R) (2006)
    [9] A. P. Leppanen et al, Phys. Rev. C, 75: 054307 (2007)
    [10] Yu. Ts. Oganessian et al, Phys. Rev. C, 72: 034611 (2005); 74:044602 (2006)
    [11] P. Schuck, Y. Funaki, H. Horiuchi, G. Rpke, A. Tohsaki, and T. Yamada, Nuclear Physics A, 738(Supplement C): 245 94-100 (2004)
    [12] K. Morita et al, J. Phys. Soc. Jpn., 76: 045001 (2007)
    [13] Yu. Ts. Oganessian et al, Phys. Rev. C, 76: 011601(R) (2007)
    [14] G. Gamow, Z. Phys., 51: 204 (1928)
    [15] E. U. Condon and R. W. Gurney, Nature (London), 122: 439 (1928)
    [16] B. Buck, A. C. Merchant, and S. M. Perez, At. Data Nucl. Data Tables, 54: 53 (1993)
    [17] P. Mohr, Phys. Rev. C, 73: 031301(R) (2006)
    [18] D. N. Poenaru and M. Ivascu, Rev. Roum. Phys., 28: 309 (1983)
    [19] K. Varga, R. G. Lovas, and R. J. Liotta, Phys. Rev. Lett., 69:37 (1992)
    [20] G. Royer and B. Remaud, Nucl. Phys. A, 444: 447 (1985)
    [21] S. B. Duarte et al, At. Data Nucl. Data Tables, 80: 235 (2002)
    [22] D. N. Basu, Phys. Lett. B, 566: 90 (2003); P. Roy Chowdhury, D. N. Basu, and C. Samanta, Phys. Rev. C, 75: 047306 (2007)
    [23] B. A. Brown, Phys. Rev. C, 46: 811 (1992)
    [24] G. Royer, J. Phys. G, 26: 1149 (2000); G. Royer and R. Moustabchir, Nucl. Phys. A, 683: 182 (2001)
    [25] R. K. Gupta, M. Balasubramaniam, C. Mazzocchi, M. LaCommara, W. Scheid, Phys. Rev. C, 65: 024201 (2002)
    [26] D. N. Poenaru, I. H. Plonski, and W. Greiner, Phys. Rev. C, 74: 014312 (2006)
    [27] H. F. Zhang, W. Zuo, J. Q. Li, and G. Royer, Phys. Rev. C, 74: 017304 (2006)
    [28] H. F. Zhang and G. Royer, Phys. Rev. C, 76: 047304 (2007)
    [29] C. Xu and Z. Z. Ren, Phys. Rev. C, 74: 014304 (2006); Nucl. Phys. A, 760: 303 (2005)
    [30] J. C. Pei, F. R. Xu, Z. J. Lin, and E. G. Zhao, Phys. Rev. C, 76: 044326 (2007)
    [31] H. F. Zhang and G. Royer, Phys. Rev. C, 77: 054318 (2008)
    [32] L. Ma, Z. Y. Zhang, Z. G. Gan, H. B. Yang, L. Yu, J. Jiang, J. G. Wang, Y. L. Tian, Y. S. Wang, and S. Guo, Phys. Rev. C, 91: (2015)
    [33] M. Sun, Z. Liu, T. H. Huang et al, Physics Letters B, 771: 303 (2017)
    [34] G. Royer, J. Phys. G: Nucl. Part. Phys., 26 (2000)
    [35] P. Moller, A. J. Sierk, T. Ichikawa, and H. Sagawa, Atomic Data and Nuclear Data Tables, 109: 110 (2016)
    [36] G. Royer, Journal of Physics G Nuclear Particle Physics, 26:1149 (2000)
    [37] J. Khuyagbaatar, A. Yakushev, Ch. E. Dllmann et al, Physical Review Letters, 115: 242502 (2015)
    [38] R. Ferrer, A. Barzakh, B. Bastin et al, Nature Communications, 8: 14520 (2017)

  • Access

    加载中

Get Citation
Yan-Wei Zhao, Shu-Qing Guo and Hong-Fei Zhang. α particle preformation and shell effect for heavy andsuperheavy nuclei[J]. Chinese Physics C, 2018, 42(7): 074103. doi: 10.1088/1674-1137/42/7/074103
Yan-Wei Zhao, Shu-Qing Guo and Hong-Fei Zhang. α particle preformation and shell effect for heavy andsuperheavy nuclei[J]. Chinese Physics C, 2018, 42(7): 074103.  doi: 10.1088/1674-1137/42/7/074103 shu
Milestone
Received: 2018-02-01
Revised: 2018-04-09
Fund

    Supported by National Natural Science Foundation of China (11675066, 11475050), Fundamental Research Funds for the Central Universities (lzujbky-2017-ot04) and Feitian Scholar Project of Gansu Province

Article Metric

Article Views(1715)
PDF Downloads(52)
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:

α particle preformation and shell effect for heavy andsuperheavy nuclei

  • 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, CAS, Lanzhou 730000, China
  • Received Date: 2018-02-01
  • Accepted Date: 2018-04-09
  • Available Online: 2018-07-05
Fund Project:  Supported by National Natural Science Foundation of China (11675066, 11475050), Fundamental Research Funds for the Central Universities (lzujbky-2017-ot04) and Feitian Scholar Project of Gansu Province

Abstract: The α particle preformation factor is extracted within a generalized liquid drop model for Z=84-92 isotopes and N=126, 128, 152, 162, 176, 184 isotones. The calculated results show clearly that the shell effects play a key role in α particle preformation. The closer the proton and neutron numbers are to the magic numbers, the more difficult the formation of the α cluster inside the mother nucleus is. The preformation factors of the isotopes reflect that N=126 is a magic number for Po, Rn, Ra, and Th isotopes, but for U isotopes the weakening of the influence of the N=126 shell closure is evident. The trend of the factors for N=126 and N=128 isotones also support this conclusion. We extend the calculations for N=152, 162, 176, 184 isotones to explore the magic numbers for heavy and superheavy nuclei, which are probably present near Z=108 to N=152, 162 isotones and Z=116 to N=176, 184 isotones. The results also show that another subshell closure may exist after Z=124 in the superheavy nuclei. This is useful for future experiments.

    HTML

Reference (38)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: cpc@ihep.ac.cn

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: info@rhhz.net

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return