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 = -326nT/9, which is crucial in discriminating the present models from standard inflation with a canonical kinetic term. © 2011 American Physical Society.
CITATION STYLE
Kamada, K., Kobayashi, T., Yamaguchi, M., & Yokoyama, J. (2011). Higgs G inflation. Physical Review D - Particles, Fields, Gravitation and Cosmology, 83(8). https://doi.org/10.1103/PhysRevD.83.083515
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