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(11) : 113103 DOI: 10.1088/1674-1137/40/11/113103

A possible interpretation of the Higgs mass by the cosmological attractive relaxion

  • 1.

      Theoretical Physics Division, Institute of High Energy Physics, Chinese Academy of Sciences, P. O. Box 918-4, Beijing 100049, China

  • 2.

      CAS Key Laboratory for Researches in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Chinese Academy of Sciences, Hefei 230026, China

  • 3.

      Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Science, P. O. Box 918-3, Beijing 100049, China

  • Recently, a novel idea [1] has been proposed to relax the electroweak hierarchy problem through the cosmological inflation and the axion periotic potential. Here, we further assume that only the attractive inflation is needed to explain the light mass of the Higgs boson, where we do not need a specified periodic potential of the axion field. Attractive inflation during the early universe drives the Higgs boson mass from the large value in the early universe to the small value at present, where the Higgs mass is an evolving parameter of the Universe. Thus, the small Higgs mass can technically originate from the cosmological evolution rather than dynamical symmetry or anthropics. Further, we study the possible collider signals or constraints at a future lepton collier and the possible constraints from the muon anomalous magnetic moment. A concrete attractive relaxion model is also discussed, which is consistent with the data of Planck 2015.
      PCAS:
  • 加载中

  • References

    [1] P. W. Graham, D. E. Kaplan, and S. Rajendran, Phys. Rev. Lett., 115: 221801(2015)
    [2] S. Dimopoulos and H. Georgi, Nucl. Phys. B, 193:150(1981)
    [3] L. Randall and R. Sundrum, Phys. Rev. Lett., 83:3370(1999)
    [4] N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, Phys. Lett. B, 429: 263(1998)
    [5] L. Susskind, Phys. Rev. D, 20:2619(1979)
    [6] S. Weinberg, Phys. Rev. D, 19:1277(1979)
    [7] L. F. Abbott, Phys. Lett. B, 150:427(1985)
    [8] A. Strumia, arXiv:hepph/1504.08331
    [9] J. R. Espinosa, C. Grojean, G. Panico et al, Phys. Rev. Lett., 115: 251803(2015)
    [10] E. Hardy, JHEP, 1511: 077(2015)
    [11] S. P. Patil and P. Schwaller, JHEP, 1602: 077(2016)
    [12] O. Antipin and M. Redi, JHEP, 1512: 031(2015)
    [13] J. Jaeckel, V. M. Mehta, and L. T. Witkowski, Phys. Rev. D, 93:063522(2016)
    [14] R. S. Gupta, Z. Komargodski, G. Perez et al, JHEP, 1602: 166(2016)
    [15] B. Batell, G. F. Giudice, and M. McCullough, JHEP, 1512: 162(2015)
    [16] O. Matsedonskyi, JHEP, 1601: 063(2016)
    [17] J. Ellis, arXiv:hepph/1509.07336
    [18] L. Marzola and M. Raidal, arXiv:hepph/1510.00710
    [19] K. Choi and S. H. Im, JHEP, 1601: 149(2016)
    [20] D. E. Kaplan and R. Rattazzi, Phys. Rev. D, 93:085007(2016)
    [21] S. Di Chiara, K. Kannike, L. Marzola et al, Phys. Rev. D, 93:103527(2016)
    [22] N. Fonseca, L. de Lima, C. S. Machado et al, arXiv:hepph/1601.07183
    [23] J. L. Evans, T. Gherghetta, N. Nagata et al, arXiv:hepph/1602.04812
    [24] A. Fowlie, C. Balazs, G. White et al, arXiv: hepph/1602.03889
    [25] R. Kallosh and A. Linde, JCAP, 1306: 028(2013)
    [26] R. Kallosh and A. Linde, JCAP, 1306: 027(2013)
    [27] R. Kallosh and A. Linde, JCAP, 1307: 002(2013)
    [28] S. Ferrara, R. Kallosh, A. Linde et al, Phys. Rev. D, 88: 085038(2013)
    [29] R. Kallosh, A. Linde and D. Roest, Phys. Rev. Lett., 112: 011303(2014)
    [30] R. Kallosh, A. Linde and D. Roest, JHEP, 1311:198(2013)
    [31] R. Kallosh, A. Linde and D. Roest, JHEP, 1408: 052(2014)
    [32] R. Kallosh, A. Linde and D. Roest, JHEP, 1409: 062(2014)
    [33] M. Galante, R. Kallosh, A. Linde et al, Phys. Rev. Lett., 114:141302(2015)
    [34] R. Kallosh and A. Linde, Phys. Rev. D, 91:083528(2015)
    [35] A. Linde, JCAP, 1505: 003(2015)
    [36] J. J. M. Carrasco, R. Kallosh, and A. Linde, Phys. Rev. D, 92: 063519(2015)
    [37] J. J. M. Carrasco, R. Kallosh, and A. Linde, JHEP, 1510: 147(2015)
    [38] [Planck Collaboration], arXiv:astroph.CO/1502.01589
    [39] G.'t Hooft, C. Itzykson, A. Jaffe et al, NATO Sci. Ser. B, 59:1(1980).
    [40] Y. Ueno and K. Yamamoto, Phys. Rev. D, 93: 083524(2016)
    [41] K. A. Olive et al, Chin. Phys. C, 38: 090001(2014)
    [42] F. P. Huang, C. S. Li, D. Y. Shao et al, Eur. Phys. J. C, 74: 2990(2014)
    [43] Y. F. Cai and D. A. Easson, Int. J. Mod. Phys. D, 21: 1250094(2013)
    [44] Y. F. Cai, Y. C. Chang, P. Chen et al, Phys. Rev. D, 88: 083508(2013)
    [45] V. F. Mukhanov, H. A. Feldman, and R. H. Brandenberger, Phys. Rept., 215: 203(1992).
    [46] Planck Collaboration, arXiv: astroph.CO/1502.02114
    [47] S. Dodelson and E. Stewart, Phys. Rev. D, 65: 101301(2002) E. D. Stewart, Phys. Rev. D, 65: 103508(2002)

  • Access

    加载中

Get Citation
Fa-Peng Huang, Yifu Cai, Hong Li and Xinmin Zhang. A possible interpretation of the Higgs mass by the cosmological attractive relaxion[J]. Chinese Physics C, 2016, 40(11): 113103. doi: 10.1088/1674-1137/40/11/113103
Fa-Peng Huang, Yifu Cai, Hong Li and Xinmin Zhang. A possible interpretation of the Higgs mass by the cosmological attractive relaxion[J]. Chinese Physics C, 2016, 40(11): 113103.  doi: 10.1088/1674-1137/40/11/113103 shu
Milestone
Received: 2016-05-26
Revised: 2016-07-10
Fund

    Supported by NSFC (11121092, 11033005, 11375220,11421303), CAS PilotB Program, the China Postdoctoral Science Foundation (2016M590133), Chinese National Youth Thousand Talents Program, the USTC start-up funding (KY2030000049), Youth Innovation Promotion Association Project and Outstanding Young Scientists Project of the Chinese Academy of Sciences

Article Metric

Article Views(1720)
PDF Downloads(71)
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:

A possible interpretation of the Higgs mass by the cosmological attractive relaxion

    Corresponding author: Fa-Peng Huang,
  • 1.  Theoretical Physics Division, Institute of High Energy Physics, Chinese Academy of Sciences, P. O. Box 918-4, Beijing 100049, China
  • 2.  CAS Key Laboratory for Researches in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Chinese Academy of Sciences, Hefei 230026, China
  • 3.  Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Science, P. O. Box 918-3, Beijing 100049, China
  • Received Date: 2016-05-26
  • Accepted Date: 2016-07-10
  • Available Online: 2016-11-05
Fund Project:  Supported by NSFC (11121092, 11033005, 11375220,11421303), CAS PilotB Program, the China Postdoctoral Science Foundation (2016M590133), Chinese National Youth Thousand Talents Program, the USTC start-up funding (KY2030000049), Youth Innovation Promotion Association Project and Outstanding Young Scientists Project of the Chinese Academy of Sciences

Abstract: Recently, a novel idea [1] has been proposed to relax the electroweak hierarchy problem through the cosmological inflation and the axion periotic potential. Here, we further assume that only the attractive inflation is needed to explain the light mass of the Higgs boson, where we do not need a specified periodic potential of the axion field. Attractive inflation during the early universe drives the Higgs boson mass from the large value in the early universe to the small value at present, where the Higgs mass is an evolving parameter of the Universe. Thus, the small Higgs mass can technically originate from the cosmological evolution rather than dynamical symmetry or anthropics. Further, we study the possible collider signals or constraints at a future lepton collier and the possible constraints from the muon anomalous magnetic moment. A concrete attractive relaxion model is also discussed, which is consistent with the data of Planck 2015.

    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