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> 2016, Vol. 40> Issue(2) : 023102 DOI: 10.1088/1674-1137/40/2/023102

Survival of charged ρ condensation at high temperature and density

  • 1.

      Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

  • 2.

     Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

  • 3.

     Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences, Beijing 100049, China

  • The charged vector ρ mesons in the presence of external magnetic fields at finite temperature T and chemical potential μ have been investigated in the framework of the Nambu-Jona-Lasinio model. We compute the masses of charged ρ mesons numerically as a function of the magnetic field for different values of temperature and chemical potential. The self-energy of the ρ meson contains the quark-loop contribution, i.e. the leading order contribution in 1/Nc expansion. The charged ρ meson mass decreases with the magnetic field and drops to zero at a critical magnetic field eBc, which indicates that the charged vector meson condensation, i.e. the electromagnetic superconductor can be induced above the critical magnetic field. Surprisingly, it is found that the charged ρ condensation can even survive at high temperature and density. At zero temperature, the critical magnetic field just increases slightly with the chemical potential, which indicates that charged ρ condensation might occur inside compact stars. At zero density, in the temperature range 0.2-0.5 GeV, the critical magnetic field for charged ρ condensation is in the range of 0.2-0.6 GeV2, which indicates that a high temperature electromagnetic superconductor might be created at LHC.
      PCAS:
  • 加载中

  • References

    [1] V. Skokov, A. Y. Illarionov and V. Toneev, Int. J. Mod. Phys. A, 24: 5925 (2009)
    [2] W. -T. Deng and X. -G. Huang, Phys. Rev. C, 85: 044907 (2012)
    [3] M. N. Chernodub, Phys. Rev. D, 82: 085011 (2010); [arXiv:1008.1055 [hep-ph]]
    [4] M. N. Chernodub, Phys. Rev. Lett., 106: 142003 (2011); [arXiv:1101.0117 [hep-ph]]
    [5] Y. Hidaka and A. Yamamoto, Phys. Rev. D, 87 (9): 094502 (2013); [arXiv:1209.0007 [hep-ph]]
    [6] C. Li and Q. Wang, Phys. Lett. B, 721: 141 (2013); [arXiv:1301.7009 [hep-th]]
    [7] M. Frasca, JHEP, 1311: 099 (2013); [arXiv:1309.3966 [hep-ph]]
    [8] H. Liu, L. Yu and M. Huang, Phys. Rev. D, 91: (1): 014017 (2015); [arXiv:1408.1318 [hep-ph]]
    [9] O. Larina, E. Luschevskaya, O. Kochetkov and O. V. Teryaev, PoS LATTICE, 2014: 120 (2014); [arXiv:1411.0730 [hep-lat]]
    [10] N. Callebaut, D. Dudal and H. Verschelde, PoS FACESQCD , 046 (2010); [arXiv:1102.3103 [hep-ph]]
    [11] M. Ammon, J. Erdmenger, P. Kerner and M. Strydom, Phys. Lett. B, 706: 94 (2011); [arXiv:1106.4551 [hep-th]]
    [12] M. A. Andreichikov, B. O. Kerbikov, V. D. Orlovsky and Y. A. Simonov, Phys. Rev. D, 87: (9): 094029 (2013); [arXiv:1304.2533 [hep-ph]]
    [13] Kunlun Wang, QCD phase transition and properties of phases with Dyson-Schwinger equations, Ph.D. Thesis (Beijing: Peking University, 2013) (in Chinese)
    [14] Y. Nambu and G. Jona-Lasinio, Phys. Rev., 122: 345 (1961)
    [15] Y. Nambu and G. Jona-Lasinio, Phys. Rev., 124: 246 (1961)
    [16] S. Klimt, M. F. M. Lutz, U. Vogl and W. Weise, Nucl. Phys. A, 516: 429 (1990)
    [17] U. Vogl and W. Weise, Prog. Part. Nucl. Phys., 27: 195 (1991)
    [18] S. P. Klevansky, Rev. Mod. Phys., 64: 649 (1992)
    [19] T. Hatsuda and T. Kunihiro, Phys. Rept., 247: 221 (1994); [hep-ph/9401310]
    [20] S. Fayazbakhsh, S. Sadeghian and N. Sadooghi, Phys. Rev. D, 86: 085042 (2012); [arXiv:1206.6051 [hep-ph]]
    [21] K. Fukushima, D. E. Kharzeev and H. J. Warringa, Nucl. Phys. A, 836: 311 (2010); [arXiv:0912.2961 [hep-ph]]
    [22] A. K. Das and M. B. Hott, Mod. Phys. Lett. A, 9: 3383 (1994); [hep-ph/9406426]
    [23] Y. B. He, J. Hufner, S. P. Klevansky and P. Rehberg, Nucl. Phys. A, 630: 719 (1998); [nucl-th/9712051]
    [24] M. Frasca and M. Ruggieri, Phys. Rev. D, 83: 094024 (2011); [arXiv:1103.1194 [hep-ph]]
    [25] P. Rehberg and S. P. Klevansky, Annals Phys., 252: 422 (1996); [hep-ph/9510221]
    [26] J. Chao, P. Chu and M. Huang, Phys. Rev. D, 88: 054009 (2013); L. Yu, H. Liu and M. Huang, Phys. Rev. D, 90: (7): 074009 (2014); L. Yu, J. Van Doorsselaere and M. Huang, Phys. Rev. D, 91: (7): 074011 (2015)

  • Access

    加载中

Get Citation
Hao Liu, Lang Yu and Mei Huang. Survival of charged ρ condensation at high temperature and density[J]. Chinese Physics C, 2016, 40(2): 023102. doi: 10.1088/1674-1137/40/2/023102
Hao Liu, Lang Yu and Mei Huang. Survival of charged ρ condensation at high temperature and density[J]. Chinese Physics C, 2016, 40(2): 023102.  doi: 10.1088/1674-1137/40/2/023102 shu
Milestone
Received: 2015-07-23
Fund

    Supported by the NSFC (11275213, 11261130311) (CRC 110 by DFG and NSFC), CAS Key Project (KJCX2-EW-N01), and Youth Innovation Promotion Association of CAS. L.Yu is Partially Supported by China Postdoctoral Science Foundation (2014M550841)

Article Metric

Article Views(1551)
PDF Downloads(33)
Cited by(0)
Policy on re-use
To reuse of Open Access content published by CPC, for content published under the terms of the Creative Commons Attribution 3.0 license (“CC CY”), the users don’t need to request permission to copy, distribute and display the final published version of the article and to create derivative works, subject to appropriate attribution.
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:

Survival of charged ρ condensation at high temperature and density

    Corresponding author: Hao Liu,
    Corresponding author: Lang Yu,
    Corresponding author: Mei Huang,
  • 1.  Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
  • 2. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
  • 3. Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences, Beijing 100049, China
  • Received Date: 2015-07-23
  • Available Online: 2016-02-20
Fund Project:  Supported by the NSFC (11275213, 11261130311) (CRC 110 by DFG and NSFC), CAS Key Project (KJCX2-EW-N01), and Youth Innovation Promotion Association of CAS. L.Yu is Partially Supported by China Postdoctoral Science Foundation (2014M550841)

Abstract: The charged vector ρ mesons in the presence of external magnetic fields at finite temperature T and chemical potential μ have been investigated in the framework of the Nambu-Jona-Lasinio model. We compute the masses of charged ρ mesons numerically as a function of the magnetic field for different values of temperature and chemical potential. The self-energy of the ρ meson contains the quark-loop contribution, i.e. the leading order contribution in 1/Nc expansion. The charged ρ meson mass decreases with the magnetic field and drops to zero at a critical magnetic field eBc, which indicates that the charged vector meson condensation, i.e. the electromagnetic superconductor can be induced above the critical magnetic field. Surprisingly, it is found that the charged ρ condensation can even survive at high temperature and density. At zero temperature, the critical magnetic field just increases slightly with the chemical potential, which indicates that charged ρ condensation might occur inside compact stars. At zero density, in the temperature range 0.2-0.5 GeV, the critical magnetic field for charged ρ condensation is in the range of 0.2-0.6 GeV2, which indicates that a high temperature electromagnetic superconductor might be created at LHC.

    HTML

Reference (26)

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