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> 2017, Vol. 41> Issue(11) : 114102 DOI: 10.1088/1674-1137/41/11/114102

Effect of tensor correlations on the depletion of nuclear Fermi sea within the extended BHF approach

  • 1.

     Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China

  • 2.

     Department of Physics, Iowa State University, Ames, IA, 50011 USA

  • 3.

      Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China

  • 4.

     University of Chinese Academy of Sciences, Beijing 100049, China

  • We have investigated the effect of tensor correlations on the depletion of the nuclear Fermi sea in symmetric nuclear matter within the framework of the extended Brueckner-Hartree-Fock approach by adopting the AV18 two-body interaction and a microscopic three-body force. The contributions from various partial wave channels including the isospin-singlet T=0 channel, the isospin-triplet T=1 channel and the T=0 tensor 3SD1 channel have been calculated. The T=0 neutron-proton correlations play a dominant role in causing the depletion of nuclear Fermi sea. The T=0 correlation-induced depletion turns out to stem almost completely from the 3SD1 tensor channel. The isospin-singlet T=0 3SD1 tensor correlations are shown to be responsible for most of the depletion, which amounts to more than 70 percent of the total depletion in the density region considered. The three-body force turns out to lead to an enhancement of the depletion at high densities well above the empirical saturation density and its effect increases as a function of density.
      PCAS:
  • 加载中

  • References

    [1] T. Otsuka, T. Suzuki, R. Fujimoto1, H. Grawe, and Y. Akaishi, Phys. Rev. Lett., 95:232502(2005)
    [2] T. Otsuka, T. Suzuki, M. Honma, Y. Utsuno, N. Tsunoda, K. Tsukiyama, and M. Hjorth-Jensen, Phys. Rev. Lett., 104:012501(2010)
    [3] I. Vidana, A. Polls and C. Providencia, Phys. Rev. C, 84:062801(2011)
    [4] L. Frankfurt, M. Sargsian, and M. Strikman, Int. J. Mod. Phys. A, 23:2991(2008)
    [5] J. P. Jeukenne, A. Lejeune, and C. Mahaux, Phys. Rep., 25:83(1976)
    [6] B. Vonderfecht, W. Dickhoff, A. Polls, and A. Ramos, Phys. Rev. C, 44:R1265(1991)
    [7] J. M. Cavedon, B. Frois, D. Goutte et al, Phys. Rev. Lett., 49:978(1982)
    [8] V. R. Pandharipande, I. Sick, and P. K. A. deWitt Huberts, Rev. Mod. Phys., 69:981(1997)
    [9] O. Hen, G. A. Miller, E. Piasetzky, and L. B. Weinstein, arXiv:1611.09748
    [10] A. Ramos, A. Polls, and W. H. Dickhoff, Nucl. Phys. A, 503:1(1989)
    [11] W. H. Dickhoff and M. Mther, Rep. Prog. Phys., 55:1947(1992)
    [12] W. Dickhoff and C. Barbieri, Prog. Part. Nucl. Phys., 52:377(2004)
    [13] P. K. A. deWitt Huberts, J. Phys. G, 16:507(1990)
    [14] L. Lapiks, J. Wesseling, and R. B. Wiringa, Phys. Rev. Lett., 82:4404(1999)
    [15] R. Starink, M. F. van Batenburg, E. Cisbani et al, Phys. Lett. B, 474:33(2000)
    [16] M. F. van Batenburg, Ph. D. thesis, University of Utrecht, 2001(unpublished)
    [17] D. Rohe et al (E97-006 Collaboration), Phys. Rev. Lett., 93:182501(2004)
    [18] R. A. Niyazov et al (CLAS Collaboration), Phys. Rev. Lett., 92:052303(2004); K. S. Egiyan et al (CLAS Collaboration), Phys. Rev. Lett., 96:082501(2006)
    [19] F. Benmokhtar et al (Jefferson Lab Hall A Collaboration), Phys. Rev. Lett., 94:082305(2005); R. Shneor et al (Jefferson Lab Hall A Collaboration), Phys. Rev. Lett., 99:072501(2007)
    [20] J. L. S. Aclander, J. Alster, D. Barton et al, Phys. Lett. B, 453:211(1999); A. Tang, J. W. Watson, J. Aclander et al, Phys. Rev. Lett., 90:042301(2003); E. Piasetzky, M. Sargsian, L. Frankfurt, M. Strikman, and J. W. Watson, Phys. Rev. Lett., 97:162504(2006)
    [21] C. J. G. Onderwater, K. Allaart, E. C. Aschenauer et al, Phys. Rev. Lett., 81:2213(1998)
    [22] L. A. Riley, P. Adrich, T. R. Baugher et al, Phys. Rev. C, 78:011303(2008)
    [23] R. Subedi, R. Shneor, P. Monaghan et al, Science, 320:1476(2008) and reference therein
    [24] R. Schiavilla, R. B. Wiringa, S. C. Pieper, and J. Carlson, Phys. Rev. Lett., 98:132501(2007)
    [25] H. Mther, G. Knehr, and A. Polls, Phys. Rev. C, 52:2955(1995)
    [26] T. Alm, G. Rpke, A. Schnell, N. H. Kwong, and H. S. Khler, Phys. Rev. C, 53:2181(1996)
    [27] Y. Dewulf, D. Van Neck, and M. Waroquier, Phys. Rev. C, 65:054316(2002); Y. Dewulf, W. H. Dickhoff, D. Van Neck, E. E. Stoddard, and M. Waroquier, Phys. Rev. Lett., 90:152501(2003)
    [28] T. Frick, H. Mther, A. Rios, A. Polls, and A. Ramos, Phys. Rev. C, 71:014313(2005)
    [29] A. Rios, A. Polls, I. Vidana, Phys. Rev. C, 79:025802(2009); A. Rios, A. Polls, and W. Dickhoff, Phys. Rev. C, 79:064308(2009)
    [30] R. Sartor and C. Mahaux, Phys. Rev. C, 21:1546(1980)
    [31] P. Grang:J. Cugnon, and A. Lejeune, Nucl. Phys. A, 473:365(1987)
    [32] M. Jaminon and C. Mahaux, Phys. Rev. C, 41:697(1990)
    [33] M. Baldo, I. Bombaci, G. Giansiracusa, U. Lombardo, C. Mahaux, and R. Sartor, Phys. Rev. C, 41:1748(1990)
    [34] M. Baldo, I. Bombaci, G. Giansiracusa, and U. Lombardo, Nucl. Phys. A, 530:135(1991)
    [35] C. Mahaux and R. Sartor, Nucl. Phys. A, 553:515(1993)
    [36] Kh. S. A. Hassaneen and H. Mther, Phys. Rev. C, 70:054308(2004)
    [37] P. Bozek, Phys. Rev. C, 59:2619(1999); P. Bozek, Phys. Rev. C, 65:054306(2002)
    [38] V. Soma and P. Bozek, Phys. Rev. C, 78:054003(2008)
    [39] S. Fantoni and V. R. Pandharipande, Nucl. Phys. A, 427:473(1984)
    [40] O. Benhar, A. Fabrocini, and S. Fantoni, Nucl. Phys. A, 505:267(1989); O. Benhar, A. Fabrocini, and S. Fantoni, Phys. Rev. C, 41:R24(1990)
    [41] Yin Peng, Jian-Yang Li, Pei Wang, and Wei Zuo, Phys. Rev. C, :(2013)
    [42] P. Grang, A. Lejeune, M. Martzolff, and J.-F.Mathiot, Phys. Rev. C, 40:1040(1989)
    [43] W. Zuo, A. Lejeune, U. Lombardo et al, Nucl. Phys. A, 706:418(2002); Eur. Phys. J. A, 14:469(2002)
    [44] B. D. Day, Rev. Mod. Phys., 50:495(1978)
    [45] R. B. Wiringa, V. G. J. Stoks, and R. Schiavilla, Phys. Rev. C, 51:38(1995)
    [46] M. Baldo, I. Bombaci, L. S. Ferreira, G. Giansiracusa, and U. Lombardo, Phys. Lett. B, 209:135(1988); Phys. Lett. B, 215:19(1988)
    [47] W. Zuo, I. Bombaci, and U. Lombardo, Phys. Rev. C, 60:024605(1999)

  • Access

    加载中

Get Citation
Peng Yin, Jianmin Dong and Wei Zuo. Effect of tensor correlations on the depletion of nuclear Fermi sea within the extended BHF approach[J]. Chinese Physics C, 2017, 41(11): 114102. doi: 10.1088/1674-1137/41/11/114102
Peng Yin, Jianmin Dong and Wei Zuo. Effect of tensor correlations on the depletion of nuclear Fermi sea within the extended BHF approach[J]. Chinese Physics C, 2017, 41(11): 114102.  doi: 10.1088/1674-1137/41/11/114102 shu
Milestone
Received: 2017-05-28
Fund

    Supported by National Natural Science Foundation of China (11435014, 11175219), the 973 Program of China (2013CB834405) and the Knowledge Innovation Project (KJCX2-EW-N01) of the Chinese Academy of Sciences

Article Metric

Article Views(1598)
PDF Downloads(22)
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:

Effect of tensor correlations on the depletion of nuclear Fermi sea within the extended BHF approach

    Corresponding author: Peng Yin,
    Corresponding author: Wei Zuo,
  • 1. Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
  • 2. Department of Physics, Iowa State University, Ames, IA, 50011 USA
  • 3.  Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
  • 4. University of Chinese Academy of Sciences, Beijing 100049, China
  • Received Date: 2017-05-28
  • Available Online: 2017-11-05
Fund Project:  Supported by National Natural Science Foundation of China (11435014, 11175219), the 973 Program of China (2013CB834405) and the Knowledge Innovation Project (KJCX2-EW-N01) of the Chinese Academy of Sciences

Abstract: We have investigated the effect of tensor correlations on the depletion of the nuclear Fermi sea in symmetric nuclear matter within the framework of the extended Brueckner-Hartree-Fock approach by adopting the AV18 two-body interaction and a microscopic three-body force. The contributions from various partial wave channels including the isospin-singlet T=0 channel, the isospin-triplet T=1 channel and the T=0 tensor 3SD1 channel have been calculated. The T=0 neutron-proton correlations play a dominant role in causing the depletion of nuclear Fermi sea. The T=0 correlation-induced depletion turns out to stem almost completely from the 3SD1 tensor channel. The isospin-singlet T=0 3SD1 tensor correlations are shown to be responsible for most of the depletion, which amounts to more than 70 percent of the total depletion in the density region considered. The three-body force turns out to lead to an enhancement of the depletion at high densities well above the empirical saturation density and its effect increases as a function of density.

    HTML

Reference (47)

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