arXiv:1012.4238·v1·Cosmology and Nongalactic Astrophysics
Higgs G-inflation
Kohei Kamada🇯🇵 · Tsutomu Kobayashi🇯🇵 · Masahide Yamaguchi🇯🇵 · Jun'ichi Yokoyama🇯🇵
Abstract
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 non-linear 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 and the tensor spectral index , , which is crucial in discriminating the present models from standard inflation with a canonical kinetic term.
Comments: 10 pages, 4 figures