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arXiv · 1008.0603

G-inflation: inflation driven by the Galileon field

Tsutomu Kobayashi·Masahide Yamaguchi·Jun'ichi Yokoyama
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Abstract

We propose a new class of inflation model, G-inflation, which has a Galileon-like nonlinear derivative interaction of the form $G(ϕ, (\nablaϕ)^2)\Boxϕ$ in the Lagrangian with the resultant equations of motion being of second order. It is shown that (almost) scale-invariant curvature fluctuations can be generated even in the exactly de Sitter background and that the tensor-to-scalar ratio can take a significantly larger value than in the standard inflation models, violating the standard consistency relation. Furthermore, violation of the null energy condition can occur without any instabilities. As a result, the spectral index of tensor modes can be blue, which makes it easier to observe quantum gravitational waves from inflation by the planned gravitational-wave experiments such as LISA and DECIGO as well as by the upcoming CMB experiments such as Planck and CMBpol.

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Tsutomu Kobayashi, Masahide Yamaguchi, Jun'ichi Yokoyama. 2010-12-09. G-inflation: inflation driven by the Galileon field. https://doi.org/10.1103/physrevlett.105.231302

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