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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.
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  • 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)

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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

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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.

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