Export citation

Export citation

Choose format for download:

Download Citation
  • Access by Xinjiang University

Is the Higgs boson associated with Coleman-Weinberg dynamical symmetry breaking?

Christopher T. Hill

  • Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA

Phys. Rev. D 89, 073003 – Published 4 April, 2014

DOI: https://doi.org/10.1103/PhysRevD.89.073003

Abstract

The Higgs mechanism may be a quantum phenomenon, i.e., a Coleman-Weinberg potential generated by the explicit breaking of scale symmetry in Feynman loops. We review the relationship of scale symmetry and trace anomalies, and we show that the Coleman-Weinberg potential can be defined as the solution to a differential renormalization group equation that follows from the trace of the improved stress tensor. We propose a simple phenomenological model with “maximal visibility” at the LHC containing a “dormant” Higgs doublet [no VEV, coupled to standard model gauge interactions SU(2)×U(1)] with a mass of 380GeV. We discuss the LHC phenomenology and UV challenges of such a model. We also give a schematic model in which new heavy fermions, with masses 230GeV, can drive a Coleman-Weinberg potential at two loops. The role of the “improved stress tensor” is emphasized, and we propose a nongravitational term, analogous to the θ term in QCD, which generates it from a scalar action.

Article Text

References (41)

  1. See e.g., D. M. Ghilencea and G. G. Ross, Nucl. Phys. B868, 65 (2013).
  2. S. Cassel, D. M. Ghilencea, and G. G. Ross, Nucl. Phys. B835, 110 (2010).
  3. A. Delgado, M. Garcia, and M. Quiros, arXiv:1312.3235.
  4. H. Baer, V. Barger, P. Huang, D. Mickelson, A. Mustafayev, and X. Tata, Phys. Rev. D 87, 115028 (2013).
  5. C. T. Hill and E. H. Simmons, Phys. Rep. 381, 235 (2003); 390, 553(E) (2004).
  6. W. A. Bardeen, Fermilab-Conf-95-391-T; (private communication).
  7. C. T. Hill, arXiv:hep-th/0510177.
  8. T. Appelquist and F. Sannino, Phys. Rev. D 59, 067702 (1999); O. Antipin, M. Mojaza, and F. Sannino, arXiv:1310.0957; R. Foadi, M. T. Frandsen, and F. Sannino, Phys. Rev. D 87, 095001 (2013).
  9. R. Shrock, arXiv:1305.4572.
  10. V. A. Miransky, M. Tanabashi, and K. Yamawaki, Phys. Lett. B 221, 177 (1989); Mod. Phys. Lett. A 04, 1043 (1989).
  11. W. A. Bardeen, C. T. Hill, and M. Lindner, Phys. Rev. D 41, 1647 (1990).
  12. H. S. Fukano, M. Kurachi, S. Matsuzaki, and K. Yamawaki, arXiv:1311.6629; Y. Aoki et al., arXiv:1309.0711.
  13. H.-C. Cheng, B. A. Dobrescu, and J. Gu, arXiv:1311.5928; R. S. Chivukula, B. A. Dobrescu, H. Georgi, and C. T. Hill, Phys. Rev. D 59, 075003 (1999); B. A. Dobrescu and C. T. Hill, Phys. Rev. Lett. 81, 2634 (1998).
  14. S. Weinberg, Phys. Rev. Lett. 19, 1264 (1967).
  15. E. Fermi, Z. Phys. 88, 161 (1934).
  16. S. R. Coleman and E. J. Weinberg, Phys. Rev. D 7, 1888 (1973).
  17. C. T. Hill, in “Profound implications of the Higgs boson,” Proceedings of U.S. Atlas Physics Workshop, July 15, 2013, Argonne National Laboratory, Chicago, https://sites.google.com/site/usatlasphysicsworkshop2013/, and seminars at the ANL Theory Group, University of Chicago and Fermilab, 2013.
  18. C. G. Callan, Jr., S. R. Coleman, and R. Jackiw, Ann. Phys. (N.Y.) 59, 42 (1970).
  19. W. A. Bardeen, Fermilab-Conf-08-118-T.
  20. L. Alexander-Nunneley and A. Pilaftsis, J. High Energy Phys. 09 (2010) 021; J. S. Lee and A. Pilaftsis, Phys. Rev. D 86, 035004 (2012).
  21. T. Hambye and A. Strumia, Phys. Rev. D 88, 055022 (2013).
  22. T. Hambye and M. H. G. Tytgat, Phys. Lett. B 659, 651 (2008); T. Hur, D. Jung, P. Ko, and J. Lee, 696, 262 (2011); T. Hur and P. Ko, Phys. Rev. Lett. 106, 141802 (2011).
  23. R. Dermisek, T. Jung, and H. Kim, arXiv:1308.0891.
  24. R. Barbieri, L. J. Hall, and V. S. Rychkov, Phys. Rev. D 74, 015007 (2006); L. Lopez Honorez, E. Nezri, J. F. Oliver, and M. H. G. Tytgat, J. Cosmol. Astropart. Phys. 02 (2007) 028; J. R. Espinosa and M. Quiros, Phys. Rev. D 76, 076004 (2007); R. Foot, A. Kobakhidze, K. L. McDonald, and R. R. Volkas, 77, 035006 (2008); A. Arhrib, R. Benbrik, and N. Gaur, 85, 095021 (2012); K. Ishiwata, Phys. Lett. B 710, 134 (2012); C. D. Carone and R. Ramos, Phys. Rev. D 88, 055020 (2013); T. G. Steele and Z.-W. Wang, Phys. Rev. Lett. 110, 151601 (2013); T. G. Steele, Z.-W. Wang, D. Contreras, and R. B. Mann, arXiv:1310.1960 [hep-ph]; V. Elias, R. B. Mann, D. G. C. McKeon, and T. G. Steele, Nucl. Phys. B678, 147 (2004); B703, 413(E) (2004); F. A. Chishtie, D. G. C. McKeon, and T. G. Steele, Phys. Rev. D 77, 065007 (2008); F. A. Chishtie, T. Hanif, J. Jia, R. B. Mann, D. G. C. McKeon, T. N. Sherry, and T. G. Steele, 83, 105009 (2011); A. Farzinnia, H.-J. He, and J. Ren, Phys. Lett. B 727, 141 (2013); C. Englert, J. Jaeckel, V. V. Khoze, and M. Spannowsky, J. High Energy Phys. 04 (2013) 060; V. V. Khoze and G. Ro, 10 (2013) 075; V. V. Khoze, 11 (2013) 215; M. Holthausen, J. Kubo, K. S. Lim, and M. Lindner, 12 (2013) 076; R. Foot, A. Kobakhidze, K. L. McDonald, and R. R. Volkas, arXiv:1310.0223; E. Gabrielli, M. Heikinheimo, K. Kannike, A. Racioppi, M. Raidal, and C. Spethmann, Phys. Rev. D 89, 015017 (2014); M. Aoki, S. Kanemura, and H. Yokoya, Phys. Lett. B 725, 302 (2013).
  25. S. L. Glashow and S. Weinberg, Phys. Rev. D 15, 1958 (1977).
  26. C. T. Hill, Ph.D. thesis, Caltech, 1977, p. 100., http://thesis.library.caltech.edu/4505/; the general non-Z2-invariant two-doublet scheme appeared earlier: P. Sikivie, Phys. Lett. B 65, 141 (1976.
  27. N. G. Deshpande and E. Ma, Phys. Rev. D 18, 2574 (1978).
  28. C. T. Hill and G. G. Ross (to be published).
  29. M. Gell-Mann and F. E. Low, Phys. Rev. 95, 1300 (1954).
  30. W. D. Goldberger, B. Grinstein, and W. Skiba, Phys. Rev. Lett. 100, 111802 (2008).
  31. Note that here we can define ϕ(x)=ϕ(x)+δϕ(x)=ϕ(x)+ζμμϕ(x)+δϕ(x) and hence δϕ(x)=ζμμϕ(x), and no additional terms are generated; alternatively we can do an active transformation ϕ(x)ϕ(x)+ζμμϕ(x) and additional terms are generated but vanish by integration by parts and use of equations of motion.

  32. C. T. Hill, C. N. Leung, and S. Rao, Nucl. Phys. B262 (1985) 517.
  33. G. Buchalla, G. Burdman, C. T. Hill, and D. Kominis, Phys. Rev. D 53, 5185 (1996).
  34. This is only an estimate as we do not have the two-loop contribution to β1. These corrections are not required in the two-loop estimate of the trilinear, etc., corrections to the Higgs potential below since we input mh2 in that case.

  35. D. J. Muller and S. Nandi, Nucl. Phys. B, Proc. Suppl. 52A, 192 (1997); J. C. Lee, K. Y. Lee, and J. K. Kim, Phys. Lett. B 424, 133 (1998); H.-J. He, T. M. P. Tait, and C. P. Yuan, Phys. Rev. D 62, 011702 (2000); E. Malkawi, T. M. P. Tait, and C. P. Yuan, Phys. Lett. B 385, 304 (1996).
  36. A. Semenov, arXiv:1005.1909.
  37. C. H. Llewellyn Smith and G. G. Ross, Phys. Lett. B 105, 38 (1981).
  38. G. Marques Tavares, M. Schmaltz, and W. Skiba, Phys. Rev. D 89, 015009 (2014).
  39. see, e.g., S. L. Adler, Rev. Mod. Phys. 54, 729 (1982) and Refs. therein; E. Tomboulis, Phys. Lett. B 97, 77 (1980). This is a renormalizable, D=4 theory of gravity that generates MPlanck in a QCD-like way, where Einstein gravity is recovered as the low energy effective theory, in analogy to a chiral Lagrangian of mesons for QCD. Research into Weyl gravity was largely superceded by superstring theory in 1984. String theory, however, assumes a classical input mass, the string constant, and is a priori hard to reconcile with the hypothesis of classical scale invariance and mass generated by quantum loops.
  40. This dual derivation of the conserved current is fundamental to any gauge theory, and is analogous to the fact that the electromagnetic current can be obtained by locally varying the vector potential in the Dirac action, δAμ, or by varying the phase of the electron wave function, δψ=iθ(x)ψ. Doing both at the same time with δAμ=μθ is just a gauge transformation, under which the Dirac action is invariant.

  41. The reason for introducing the source term is to remove all the linear cross terms, ϕ^, arising from the shift. In this perturbative approach there remain O(3/2) terms, δm2ϕcϕ^. These we ignore since we are working to O(). We then add back a term +Jϕc which cancels the Jϕc arising from the shift. The general formalism of the Legendre transformed potential is given in Ref. [16].

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation