Published April 15, 2011 | Version v1
Journal article

Higgs G inflation

  • 1. Research Center for the Early Universe (RESCEU), Graduate School of Science, University of Tokyo, Tokyo 113-0033 (Japan)
  • 2. Department of Physics, Graduate School of Science, University of Tokyo, Tokyo 113-0033 (Japan)
  • 3. Department of Physics, Kyoto University, Kyoto 606-8502 (Japan)
  • 4. Hakubi Center, Kyoto University, Kyoto 606-8302 (Japan)
  • 5. Department of Physics, Tokyo Institute of Technology, Tokyo 152-8551 (Japan)
  • 6. Institute for the Physics and Mathematics of the Universe (IPMU), The University of Tokyo, Kashiwa, Chiba, 277-8568 (Japan)

Description

A new class of inflation models within the context of G inflation is proposed, in which the standard model Higgs boson can act as an inflaton thanks to Galileon-like nonlinear derivative interaction. The generated primordial density perturbation is shown to be consistent with the present observational data. We also make a general discussion on potential-driven G-inflation models, and find a new consistency relation between the tensor-to-scalar ratio r and the tensor spectral index nT, r=-32√(6)nT/9, which is crucial in discriminating the present models from standard inflation with a canonical kinetic term.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
83
Journal Issue
8
Journal Page Range
p. 083515-083515.10
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Optional Information

Notes
(c) 2011 American Institute of Physics