G-inflation: inflation driven by the Galileon field

Abstract

We propose a new class of inflation model, G-inflation, which has a Galileon-like nonlinear derivative interaction of the form $G(\varphi ,(\nabla \varphi {)}^2)\square \varphi$ 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.

5 pages, 1 figure; v2: major clarification; v3: original version of the article published in Phys. Rev. Lett. 105, 231302 (2010)

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Cited by in corpus (10)

• Galileon inflation
• Higgs G-inflation
• Observational constraints on Galileon cosmology
• Matter perturbations in Galileon cosmology
• Primordial non-Gaussianities in general modified gravitational models of inflation
• Primordial non-Gaussianity from G-inflation
• Cosmology of the selfaccelerating third order Galileon
• Galileon accretion
• Conservation of the nonlinear curvature perturbation in generic single-field inflation
• Goldstone's Theorem and Hamiltonian of Multi-galileon Modified Gravity