- Access by Xinjiang University
Composite inflation from super Yang-Mills theory, orientifold, and one-flavor QCD
Phys. Rev. D 86, 125035 – Published 21 December, 2012
DOI: https://doi.org/10.1103/PhysRevD.86.125035
Abstract
Recent investigations have shown that inflation can be driven by four-dimensional strongly interacting theories nonminimally coupled to gravity. We explore this paradigm further by considering composite inflation driven by orientifold field theories. The advantage of using these theories resides in the fact that at large number of colors they feature certain super Yang-Mills properties. In particular, we can use for inflation the bosonic part of the Veneziano-Yankielowicz effective theory. Furthermore, we include the as well as fermion mass corrections at the effective Lagrangian level allowing us to explore the effects of these corrections on the inflationary slow-roll parameters. Additionally, the orientifold field theory with fermionic matter transforming according to the two-index antisymmetric representation for three colors is QCD. Therefore, this model can be interpreted as a new nonminimally coupled QCD theory of inflation. The scale of composite inflation, for all the models presented here, is of the order of . Unitarity studies of the inflaton scattering suggest that the cutoff of the model is at the Planck scale.
Article Text
References (46)
- A. H. Guth, Phys. Rev. D 23, 347 (1981).
- A. D. Linde, Phys. Lett. 108B, 389 (1982).
- A. Albrecht and P. J. Steinhardt, Phys. Rev. Lett. 48, 1220 (1982).
- P. Channuie, J. J. Joergensen, and F. Sannino, J. Cosmol. Astropart. Phys. 05 (2011) 007.
- F. Bezrukov, P. Channuie, J. J. Joergensen, and F. Sannino, Phys. Rev. D 86, 063513 (2012).
- N. Evans, J. French, and K.-Y. Kim, J. High Energy Phys. 11 (2010) 145.
- N. Evans, J. French, and K.-Y. Kim, arXiv:1208.3060.
- A. Armoni, M. Shifman, and G. Veneziano, Nucl. Phys. B667, 170 (2003).
- A. Armoni, M. Shifman, and G. Veneziano, Phys. Rev. Lett. 91, 191601 (2003).
- E. Corrigan and P. Ramond, Phys. Lett. 87B, 73 (1979).
- T. A. Ryttov and F. Sannino, Phys. Rev. D 73, 016002 (2006).
- A. Armoni and B. Kol, J. High Energy Phys. 07 (1999) 011.
- C. Angelantonj and A. Armoni, Nucl. Phys. B578, 239 (2000).
- F. Sannino and M. Shifman, Phys. Rev. D 69, 125004 (2004).
- J. Schechter, Phys. Rev. D 21, 3393 (1980).
- C. Rosenzweig, J. Schechter, and C. G. Trahern, Phys. Rev. D 21, 3388 (1980).
- P. Di Vecchia and G. Veneziano, Nucl. Phys. B171, 253 (1980).
- E. Witten, Ann. Phys. (N.Y.) 128, 363 (1980).
- P. Nath and R. L. Arnowitt, Phys. Rev. D 23, 473 (1981).
- A. Salomone, J. Schechter, and T. Tudron, Phys. Rev. D 23, 1143 (1981).
- K. Kawarabayashi and N. Ohta, Nucl. Phys. B175, 477 (1980).
- A. A. Migdal and M. A. Shifman, Phys. Lett. 114B, 445 (1982).
- G. Veneziano and S. Yankielowicz, Phys. Lett. 113B, 231 (1982).
- J. M. Cornwall and A. Soni, Phys. Rev. D 29, 1424 (1984).
- J. M. Cornwall and A. Soni, Phys. Rev. D 32, 764 (1985).
- J. R. Ellis and J. Lanik, Phys. Lett. 150B, 289 (1985).
- H. Gomm and J. Schechter, Phys. Lett. 158B, 449 (1985).
- F. Sannino and J. Schechter, Phys. Rev. D 60, 056004 (1999).
- F. Sannino, Phys. Rev. D 66, 034013 (2002).
- A. Mocsy, F. Sannino, and K. Tuominen, Phys. Rev. Lett. 91, 092004 (2003).
- A. Mocsy, F. Sannino, and K. Tuominen, Phys. Rev. Lett. 92, 182302 (2004).
- K. Hagiwara et al. (Particle Data Group Collaboration), Phys. Rev. D 66, 010001 (2002).
- V. A. Novikov, M. A. Shifman, A. I. Vainshtein, and V. I. Zakharov, Nucl. Phys. B229, 381 (1983).
- M. A. Shifman and A. I. Vainshtein, arXiv:hep-th/9902018.
- N. M. Davies, T. J. Hollowood, V. V. Khoze, and M. P. Mattis, Nucl. Phys. B559, 123 (1999).
- S. Ferrara and B. Zumino, Nucl. Phys. B87, 207 (1975).
- F. Bezrukov, D. Gorbunov, and M. Shaposhnikov, J. Cosmol. Astropart. Phys. 06 (2009) 029.
- F. L. Bezrukov and M. Shaposhnikov, Phys. Lett. B 659, 703 (2008).
- B. L. Spokoiny, Phys. Lett. 147B, 39 (1984).
- T. Futamase and K. i. Maeda, Phys. Rev. D 39, 399 (1989).
- D. S. Salopek, J. R. Bond, and J. M. Bardeen, Phys. Rev. D 40, 1753 (1989).
- R. Fakir and W. G. Unruh, Phys. Rev. D 41, 1783 (1990).
- E. Komatsu and T. Futamase, Phys. Rev. D 59, 064029 (1999).
- S. Tsujikawa and B. Gumjudpai, Phys. Rev. D 69, 123523 (2004).
- A. Feo, P. Merlatti, and F. Sannino, Phys. Rev. D 70, 096004 (2004).
- A. Masiero and G. Veneziano, Nucl. Phys. B249, 593 (1985).