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Is the Higgs boson associated with Coleman-Weinberg dynamical symmetry breaking?
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 ] with a mass of . 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 , 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 term in QCD, which generates it from a scalar action.
Article Text
References (41)
- See e.g., D. M. Ghilencea and G. G. Ross, Nucl. Phys. B868, 65 (2013).
- S. Cassel, D. M. Ghilencea, and G. G. Ross, Nucl. Phys. B835, 110 (2010).
- A. Delgado, M. Garcia, and M. Quiros, arXiv:1312.3235.
- H. Baer, V. Barger, P. Huang, D. Mickelson, A. Mustafayev, and X. Tata, Phys. Rev. D 87, 115028 (2013).
- C. T. Hill and E. H. Simmons, Phys. Rep. 381, 235 (2003); 390, 553(E) (2004).
- W. A. Bardeen, Fermilab-Conf-95-391-T; (private communication).
- C. T. Hill, arXiv:hep-th/0510177.
- 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).
- R. Shrock, arXiv:1305.4572.
- V. A. Miransky, M. Tanabashi, and K. Yamawaki, Phys. Lett. B 221, 177 (1989); Mod. Phys. Lett. A 04, 1043 (1989).
- W. A. Bardeen, C. T. Hill, and M. Lindner, Phys. Rev. D 41, 1647 (1990).
- H. S. Fukano, M. Kurachi, S. Matsuzaki, and K. Yamawaki, arXiv:1311.6629; Y. Aoki et al., arXiv:1309.0711.
- 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).
- S. Weinberg, Phys. Rev. Lett. 19, 1264 (1967).
- E. Fermi, Z. Phys. 88, 161 (1934).
- S. R. Coleman and E. J. Weinberg, Phys. Rev. D 7, 1888 (1973).
- 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.
- C. G. Callan, Jr., S. R. Coleman, and R. Jackiw, Ann. Phys. (N.Y.) 59, 42 (1970).
- W. A. Bardeen, Fermilab-Conf-08-118-T.
- 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).
- T. Hambye and A. Strumia, Phys. Rev. D 88, 055022 (2013).
- 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).
- R. Dermisek, T. Jung, and H. Kim, arXiv:1308.0891.
- 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).
- S. L. Glashow and S. Weinberg, Phys. Rev. D 15, 1958 (1977).
- C. T. Hill, Ph.D. thesis, Caltech, 1977, p. 100., http://thesis.library.caltech.edu/4505/; the general non--invariant two-doublet scheme appeared earlier: P. Sikivie, Phys. Lett. B 65, 141 (1976.
- N. G. Deshpande and E. Ma, Phys. Rev. D 18, 2574 (1978).
- C. T. Hill and G. G. Ross (to be published).
- M. Gell-Mann and F. E. Low, Phys. Rev. 95, 1300 (1954).
- W. D. Goldberger, B. Grinstein, and W. Skiba, Phys. Rev. Lett. 100, 111802 (2008).
Note that here we can define and hence , and no additional terms are generated; alternatively we can do an active transformation and additional terms are generated but vanish by integration by parts and use of equations of motion.
- C. T. Hill, C. N. Leung, and S. Rao, Nucl. Phys. B262 (1985) 517.
- G. Buchalla, G. Burdman, C. T. Hill, and D. Kominis, Phys. Rev. D 53, 5185 (1996).
This is only an estimate as we do not have the two-loop contribution to . These corrections are not required in the two-loop estimate of the trilinear, etc., corrections to the Higgs potential below since we input in that case.
- 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).
- A. Semenov, arXiv:1005.1909.
- C. H. Llewellyn Smith and G. G. Ross, Phys. Lett. B 105, 38 (1981).
- G. Marques Tavares, M. Schmaltz, and W. Skiba, Phys. Rev. D 89, 015009 (2014).
- 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, theory of gravity that generates 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.
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, , or by varying the phase of the electron wave function, . Doing both at the same time with is just a gauge transformation, under which the Dirac action is invariant.
The reason for introducing the source term is to remove all the linear cross terms, , arising from the shift. In this perturbative approach there remain terms, . These we ignore since we are working to . We then add back a term which cancels the arising from the shift. The general formalism of the Legendre transformed potential is given in Ref. [16].