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(6) : 064103 DOI: 10.1088/1674-1137/42/6/064103

Two-neutron halo state of 15B around 3.48 MeV by a three-body model

  • 1.

      School of Physics, Nanjing University, Nanjing 210093, China

  • 2.

      School of Physics Science and Engineering, Tongji University, Shanghai 200092, China

  • 3.

      Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China

  • We investigate low-lying bound states of the neutron-rich nucleus 15B by assuming it is a three-body system made of an inert core 13B and two valence neutrons. The three-body wave functions are obtained using the Faddeev formalism. Special attention is paid to the excited state at 3.48(6) MeV observed in the 13C(14C,12N)15B reaction, whose properties are less clear theoretically. In our three-body model, besides the ground state 3/21-, a second 3/22- state is discovered at around 3.61 MeV, which might be identified with the excited state observed at 3.48(6) MeV. We study this 3/22- state in detail. It turns out to be a two-neutron halo state with a large matter radius rm≈4.770 fm.
      PCAS:
  • 加载中

  • References

    [1] A. S. Jensen, K. Riisager, D. V. Fedorov, and E. Garrido, Rev. Mod. Phys., 76: 215 (2004)
    [2] J. Meng and P. Ring, Phys. Rev. Lett., 80: 460 (1998) [nucl-th/9612045].
    [3] J. Terasaki, S. Q. Zhang, S. G. Zhou, and J. Meng, Phys. Rev. C, 74: 054318 (2006)
    [4] M. Grasso, S. Yoshida, N. Sandulescu, and N. Van Giai, Phys. Rev. C, 74: 064317 (2006) [nucl-th/0603060]
    [5] M. Pfutzner, M. Karny, L. V. Grigorenko, and K. Riisager, Rev. Mod. Phys., 84: 567 (2012) [arXiv:1111.0482 [nucl-ex]]
    [6] A. M. Poskanzer, S. W. Cosper, E. K. Hyde, and J. Cerny, Phys. Rev. Lett., 17: 1271 (1966)
    [7] M. Stanoiu et al, Eur. Phys. J. A, 22: 5 (2004)
    [8] R. Kalpakchieva et al, Eur. Phys. J. A, 7: 451 (2000)
    [9] A. Estrade et al, Phys. Rev. Lett., 113(13): 132501 (2014)
    [10] M. Tanaka et al, Acta Phys. Polon. B, 48: 461 (2017)
    [11] N. A. F. M. Poppelier, L. D. Wood, and P. W. M. Glaudemans, Phys. Lett. B, 157: 120 (1985)
    [12] E. K. Warburton and B. A. Brown, Phys. Rev. C, 46: 923 (1992)
    [13] Y. Kanada-Enyo and H. Horiuchi, Phys. Rev. C, 52: 647 (1995)
    [14] M. V. Zhukov, B. V. Danilin, D. V. Fedorov, J. M. Bang, I. J. Thompson, and J. S. Vaagen, Phys. Rept., 231: 151 (1993)
    [15] I. Brida, F. M. Nunes, and B. A. Brown, Nucl. Phys. A, 775: 23 (2006) [nucl-th/0606048]
    [16] F. M. Nunes, J. A. Christley, I. J. Thompson, R. C. Johnson, and V. D. Efros, Nucl. Phys. A, 609: 43 (1996)
    [17] C. Romero-Redondo, E. Garrido, D. V. Fedorov, and A. S. Jensen, Phys. Rev. C, 77: 054313 (2008) [arXiv:0804.2351 [nucl-th]]
    [18] T. Tarutina, I. J. Thompson, and J. A. Tostevin, Nucl. Phys. A, 733: 53 (2004)
    [19] Z. Ren and G. Xu, Phys. Lett. B, 252: 311 (1990)
    [20] W. Horiuchi and Y. Suzuki, Phys. Rev. C, 74: 034311 (2006) [nucl-th/0605055]
    [21] L. Zhang, Z. Ren, M. Lyu, and C. Ji, Phys. Rev. C, 91(2): 024001 (2015) [arXiv:1501.00071 [nucl-th]]
    [22] M. V. Zhukov and I. J. Thompson, Phys. Rev. C, 52: 3505 (1995)
    [23] E. Garrido, D. V. Fedorov, and A. S. Jensen, Nucl. Phys. A, 733: 85 (2004) [nucl-th/0312086]
    [24] Y. Chu, Z. Ren, and C. Xu, Eur. Phys. J. A, 37: 361 (2008)
    [25] D. V. Federov, A. S. Jensen and K. Riisager, Phys. Rev. Lett., 73: 2817 (1994) [nucl-th/9409018]
    [26] Z. Ren, Phys. Rev. C, 49: 1281 (1994)
    [27] Z. Ren and G. Xu, Commun. Theor. Phys., 25: 203 (1996)
    [28] Q. Lin and Z. Ren, J. Phys. G, 39: 035102 (2012)
    [29] F. Ajzenberg-Selove, Nucl. Phys. A, 523: 1 (1991)
    [30] E. Sauvan et al, Phys. Lett. B, 491: 1 (2000) [nucl-ex/0007013]
    [31] I. J. Thompson, F. M. Nunes and B. V. Danilin, Comput. Phys. Commun., 161: 87 (2004) [nucl-th/0406071]
    [32] L. W. Nordheim, Phys. Rev., 78: 294 (1950)
    [33] S. Bedoor et al, Phys. Rev. C, 93(4): 044323 (2016)
    [34] D. Gogny, P. Pires, and R. De Tourreil, Phys. Lett. B, 32: 591 (1970)
    [35] E. Garrido, D. V. Fedorov, and A. S. Jensen, Phys. Rev. C, 68: 014002 (2003) [nucl-th/0305053]
    [36] R. Kanungo et al, Phys. Lett. B, 608: 206 (2005)
    [37] D. Baye, Phys. Rev. Lett., 58: 2738 (1987)
    [38] D. Baye and J.-M. Sparenberg, Phys. Rev. Lett., 73: 2789 (1994)
    [39] J.-M. Sparenberg and D. Baye, Phys. Rev. Lett., 79: 3802 (1997)

  • Access

    加载中

Get Citation
Dong Bai, Zhongzhou Ren and Tiekuang Dong. Two-neutron halo state of 15B around 3.48 MeV by a three-body model[J]. Chinese Physics C, 2018, 42(6): 064103. doi: 10.1088/1674-1137/42/6/064103
Dong Bai, Zhongzhou Ren and Tiekuang Dong. Two-neutron halo state of 15B around 3.48 MeV by a three-body model[J]. Chinese Physics C, 2018, 42(6): 064103.  doi: 10.1088/1674-1137/42/6/064103 shu
Milestone
Received: 2018-01-15
Revised: 2018-03-26
Fund

    Supported by National Natural Science Foundation of China (Grant No. 11535004, 11761161001, 11375086, 11120101005, 11175085 and 11235001), by the National Major State Basic Research and Development of China, Grant No. 2016YFE0129300, and by the Science and Technology Development Fund of Macau under Grant No. 068/2011/A.

Article Metric

Article Views(1672)
PDF Downloads(37)
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:

Two-neutron halo state of 15B around 3.48 MeV by a three-body model

    Corresponding author: Zhongzhou Ren,
  • 1.  School of Physics, Nanjing University, Nanjing 210093, China
  • 2.  School of Physics Science and Engineering, Tongji University, Shanghai 200092, China
  • 3.  Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
  • Received Date: 2018-01-15
  • Accepted Date: 2018-03-26
  • Available Online: 2018-06-05
Fund Project:  Supported by National Natural Science Foundation of China (Grant No. 11535004, 11761161001, 11375086, 11120101005, 11175085 and 11235001), by the National Major State Basic Research and Development of China, Grant No. 2016YFE0129300, and by the Science and Technology Development Fund of Macau under Grant No. 068/2011/A.

Abstract: We investigate low-lying bound states of the neutron-rich nucleus 15B by assuming it is a three-body system made of an inert core 13B and two valence neutrons. The three-body wave functions are obtained using the Faddeev formalism. Special attention is paid to the excited state at 3.48(6) MeV observed in the 13C(14C,12N)15B reaction, whose properties are less clear theoretically. In our three-body model, besides the ground state 3/21-, a second 3/22- state is discovered at around 3.61 MeV, which might be identified with the excited state observed at 3.48(6) MeV. We study this 3/22- state in detail. It turns out to be a two-neutron halo state with a large matter radius rm≈4.770 fm.

    HTML

Reference (39)

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