Export citation

Export citation

Choose format for download:

Download Citation
  • Access by Xinjiang University

Spontaneous scalar-vector Galileons from a Weyl biconnection model

Nima Khosravi*

  • School of Astronomy, Institute for Research in Fundamental Sciences (IPM), P.O. Box 19395-5531, Tehran, Iran

  • *nima@ipm.ir

Phys. Rev. D 89, 124027 – Published 24 June, 2014

DOI: https://doi.org/10.1103/PhysRevD.89.124027

Abstract

The Weyl biconnection model manifests a natural framework to automatically produce the structure of the Galileon theory. It is shown that this framework can explain the scalar and vector Galileon as well as their interactions by generalizing the Weyl nonmetricity, and as such it can be interpreted as a geometrical realization for Galileons. The nonmetricity part enjoys a U(1) gauge invariance. The result is interestingly nontrivial since the structure of the Galileon theory appears spontaneously, and not by demanding the absence of the Ostrogradsky ghost. This fact suggests a possible deeper conceptual relation between the Weyl biconnection model and the absence of the Ostrogradsky ghost.

Article Text

References (10)

  1. This is not the only reason to look for modified gravity. The other issue is to explain why the CC density is larger or smaller than the present matter energy density. In addition, the proposal of inflation in the early Universe suggests a similar accelerating phase, which had an end: could this happen for a late-time accelerating phase [2]?

  2. L. Amendola et al.., Living Rev. Relativity 16, 6 (2013).
  3. N. Arkani-Hamed, “Robustness of GR. Attempts to Modify Gravity,” https://video.ias.edu/pitp-2011-arkani-hamed1; T. P. Sotiriou, arXiv:1404.2955.
  4. A. Nicolis, R. Rattazzi, and E. Trincherini, Phys. Rev. D 79, 064036 (2009).
  5. C. Deffayet, G. Esposito-Farese, and A. Vikman, Phys. Rev. D 79, 084003 (2009).
  6. C. Deffayet, X. Gao, D. A. Steer, and G. Zahariade, Phys. Rev. D 84, 064039 (2011); T. Kobayashi, M. Yamaguchi, and J. I. Yokoyama, Prog. Theor. Phys. 126, 511 (2011); G. W. Horndeski, Int. J. Theor. Phys. 10, 363 (1974).
  7. G. Tasinato, J. High Energy Phys. 04 (2014) 067; L. Heisenberg, J. Cosmol. Astropart. Phys. 05 (2014) 015.
  8. N. Khosravi, Phys. Rev. D 89, 024004 (2014).
  9. Note that we have the relation π.π[Π]π.Π.π32π.π[Π], where is an equality up to a total derivative.

  10. N. Arkani-Hamed, H. Georgi, and M. D. Schwartz, Ann. Phys. (Amsterdam) 305, 96 (2003).

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation