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Renormalization-group flows and fixed points in Yukawa theories

Esben Mølgaard1,2 and Robert Shrock2

  • 1The Centre for Cosmology and Particle Physics Phenomenology CP3-Origins, and the Danish Institute for Advanced Study DIAS, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark
  • 2C. N. Yang Institute for Theoretical Physics and Department of Physics and Astronomy, Stony Brook University, Stony Brook, New York 11794, USA

Phys. Rev. D 89, 105007 – Published 8 May, 2014

DOI: https://doi.org/10.1103/PhysRevD.89.105007

Abstract

We study renormalization-group flows in Yukawa theories with massless fermions, including determination of fixed points and curves that separate regions of different flow behavior. We assess the reliability of perturbative calculations for various values of Yukawa coupling y and quartic scalar coupling λ by comparing the properties of flows obtained with the beta functions of these couplings calculated to different orders in the loop expansion. The results provide a determination of the region in y and λ where calculations up to two loops can yield reasonably reliable results. In the regime of weak couplings where the perturbative calculations are most reliable, we find that the theories have no nontrivial fixed points, and the flow is toward a free theory in the infrared.

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References (25)

  1. Some early studies on the renormalization group in quantum field theory include E. C. G. Stueckelberg and A. Peterman, Helv. Phys. Acta 26, 499 (1953); M. Gell-Mann and F. Low, Phys. Rev. 95, 1300 (1954); N. N. Bogolubov and D. V. Shirkov, Doklad. Akad. Nauk SSSR 103, 391 (1955); C. G. Callan, Phys. Rev. D 2, 1541 (1970); K. Symanzik, Commun. Math. Phys. 18, 227 (1970); See also K. Wilson, Phys. Rev. D 3, 1818 (1971).
  2. W. E. Caswell, Phys. Rev. Lett. 33, 244 (1974); D. R. T. Jones, Nucl. Phys. B75, 531 (1974).
  3. T. Banks and A. Zaks, Nucl. Phys. B196, 189 (1982).
  4. E. Gardi and M. Karliner, Nucl. Phys. B529, 383 (1998); E. Gardi, G. Grunberg, and M. Karliner, J. High Energy Phys. 07 (1998) 007; T. A. Ryttov and R. Shrock, Phys. Rev. D 83, 056011 (2011); C. Pica and F. Sannino, 83, 035013 (2011); T. A. Ryttov and R. Shrock, 85, 076009 (2012); R. Shrock, 87, 105005 (2013); 87, 116007 (2013).
  5. B. Holdom, Phys. Lett. B 694, 74 (2010).
  6. R. Shrock, Phys. Rev. D 88, 036003 (2013); 89, 045019 (2014).
  7. Some of the many recent papers on this include J. Ellis, J. R. Espinosa, G. F. Giudice, A. Hoecker, and A. Riotto, Phys. Lett. B 679, 369 (2009); M. Shaposhnikov and C. Wetterich, 683, 196 (2010); F. Bezrukov and M. Shaposhnikov, J. High Energy Phys. 07 (2009) 089; J. Elias-Miro, J. R. Espinosa, G. F. Giudice, G. Isadori, A. Riotto, and A. Strumia, Phys. Lett. B 709, 222 (2012); G. Degrassi, S. Di Vita, J. Elias-Miro, J. R. Espinosa, G. F. Giudice, G. Isadori, and A. Strumia, J. High Energy Phys. 08 (2012) 098; F. Bezrukov, M. Yu. Kalmykov, B. A. Kniehl, and M. Shaposhnikov, 10 (2012) 140; L. A. Anchordoqui, I. Antoniadis, H. Goldberg, X. Huang, D. Lust, T. Taylor, and B. Vlcek, 02 (2013) 074; I. Masina, Phys. Rev. D 87, 053001 (2013); F. Jegerlehner, arXiv:1305.6652; V. Branchina and E. Messina, Phys. Rev. Lett. 111, 241801 (2013); H. Gies, C. Gneiting, and R. Sondenheimer, Phys. Rev. D 89, 045012 (2014); E. Eichten, at the CP3 Workshop, Southern Denmark University, 2013; D. Buttazzo, G. Degrassi, G. F. Giudice, F. Sala, A. Salvio, and A. Strumia, J. High Energy Phys. 12 (2013) 089; C. Hill, Phys. Rev. D 89, 073003 (2014).
  8. M. Holthausen, K. S. Lim, and M. Lindner, J. High Energy Phys. 02 (2012) 037; K. G. Chetyrkin and M. F. Zoller, 06 (2012) 033; 04 (2013) 091; 09 (2013) 155(E); L. N. Mihaila, J. Salomon, and M. Steinhauser, Phys. Rev. D 86, 096008 (2012).
  9. O. Antipin, M. Gillioz, J. Krog, E. Mølgaard, and F. Sannino, J. High Energy Phys. 08 (2013) 034; O. Antipin, M. Mojaza, and F. Sannino, Phys. Rev. D 89, 085015 (2014), and references therein.
  10. H. Yukawa, Proc. Phys. Math. Soc. Jpn. 17, 48 (1935).
  11. T. P. Cheng, E. Eichten, and L.-F. Li, Phys. Rev. D 9, 2259 (1974).
  12. L. Maiani, G. Parisi, and R. Petronzio, Nucl. Phys. B136, 115 (1978); R. Flores and M. Sher, Phys. Rev. D 27, 1679 (1983); M. A. Beg, C. Panagiotakopoulos, and A. Sirlin, Phys. Rev. Lett. 52, 883 (1984); M. Lindner, Z. Phys. C 31, 295 (1986).
  13. I-H. Lee and R. E. Shrock, Phys. Rev. Lett. 59, 14 (1987); Phys. Lett. B 199, 541 (1987); J. Shigemitsu, 189, 164 (1987); I-H. Lee and R. E. Shrock, Nucl. Phys. B305, 305 (1988); J. Shigemitsu, Phys. Lett. B 226, 364 (1989); A. Hasenfratz and T. Neuhaus, 220, 435 (1989); I-H. Lee, J. Shigemitsu, and R. E. Shrock, Nucl. Phys. B330, 225 (1990); B334, 265 (1990); A. Hasenfratz, W.-Q. Liu, and T. Neuhaus, Phys. Lett. B 236, 339 (1990); L. Lin, I. Montvay, H. Wittig, and G. Münster, Nucl. Phys. B355, 511 (1991); J. Shigemitsu, Nucl. Phys. B, Proc. Suppl. 20, 515 (1991); R. E. Shrock, in Quantum Fields on the Computer, edited by M. Creutz (World Scientific, Singapore, 1992), pp. 150–210.
  14. Z. Fodor, K. Holland, J. Kuti, D. Nogradi, and C. Schroeder, Proc. Sci., LAT2007 (2007) 056 [arXiv:0710.3151]; P. Gerhold and K. Jansen, J. High Energy Phys. 04 (2010) 094.
  15. B. Grinstein and P. Uttayarat, J. High Energy Phys. 07 (2011) 038; O. Antipin, S. Di Chiara, M. Mojaza, E. Mølgaard, and F. Sannino, Phys. Rev. D 86, 085009 (2012); O. Antipin, M. Mojaza, and F. Sannino, Phys. Lett. B 712, 119 (2012).
  16. O. Antipin, M. Mojaza, and F. Sannino, Phys. Rev. D 87, 096005 (2013); O. Antipin, M. Gillioz, E. Mølgaard, and F. Sannino, 87, 125017 (2013).
  17. B. Grinstein, A. Stergiou, and D. Stone, J. High Energy Phys. 11 (2013) 195.
  18. G. ’t Hooft, Nucl. Phys. B61, 455 (1973); W. A. Bardeen, A. J. Buras, D. W. Duke, and T. Muta, Phys. Rev. D 18, 3998 (1978).
  19. T. A. Ryttov and R. Shrock, Phys. Rev. D 86, 065032 (2012); 86, 085005 (2012).
  20. T. A. Ryttov, Phys. Rev. D 89, 016013 (2014).
  21. There have been many studies of nonrelativistic bound states due to Yukawa interactions, but these are not directly relevant to our work, since our models are constructed to be invariant under global chiral symmetries and hence to avoid any bare fermion termsso that the fermions are ultrarelativistic. Some explorations of possible relativistic fermion-fermion bound states resulting from a strong Yukawa interaction include St. Glazek, A. Harindranath, S. Pinsky, J. Shigemitsu, and K. Wilson, Phys. Rev. D 47, 1599 (1993); M. Mangin-Brinet, J. Carbonell, and V. A. Karmanov, 64, 125005 (2001).
  22. S. R. Coleman and E. J. Weinberg, Phys. Rev. D 7, 1888 (1973); E. Gildener and S. Weinberg, 13, 3333 (1976).
  23. P. Q. Hung, Phys. Rev. Lett. 42, 873 (1979); A. D. Linde, Phys. Lett. 92B, 119 (1980); H. D. Politzer and S. Wolfram, 82B, 242 (1979); M. Sher, Phys. Rep. 179, 273 (1989).
  24. The purpose of this assumption of negligibly small mϕ compared with the range of μ of interest for our RG flows is to ensure that the ϕ field is dynamical; if mϕ were μ for the values of μ of interest, then we could integrate it out, obtaining a low-energy effective field theory consisting of just the fermions ψ and χ with a resultant four-fermion operator (1/mϕ2)a[ψ¯a,LχR][χ¯RψLa]+H.c.

  25. M. Fischler and J. Oliensis, Phys. Lett. 119B, 385 (1982); Phys. Rev. D 28, 2027 (1983); M. E. Machacek and M. T. Vaughn, Nucl. Phys. B236, 221 (1984); B249, 70 (1985); I. Jack and H. Osborn, B249, 472 (1985); C. Ford, I. Jack, and D. R. T. Jones, B387, 373 (1992); B504, 551(E) (1997); V. Barger, M. S. Berger, and P. Ohmann, Phys. Rev. D 47, 1093 (1993); M.-x. Luo, H.-w. Wang, and Y. Xiao, 67, 065019 (2003).

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