paper

Non-Minimal Two-Loop Inflation

arXiv:1502.06301 · doi:10.1016/j.physletb.2015.04.038

Abstract

We investigate the chaotic inflationary model using the two-loop effective potential of a self-interacting scalar field theory in curved spacetime. We use the potential which contains a non-minimal scalar curvature coupling and a quartic scalar self-interaction. We analyze the Lyapunov stability of de Sitter solution and show the stability bound. Calculating the inflationary parameters, we systematically explore the spectral index and the tensor-to-scalar ratio , with varying the four parameters, the scalar-curvature coupling , the scalar quartic coupling , the renormalization scale and the e-folding number . It is found that the two-loop correction on is much larger than the leading-log correction, which has previously been studied. We show that the model is consistent with the observation by Planck with WMAP and a recent joint analysis of BICEP2.

11pages, 7figures

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Non-Minimal Two-Loop Inflation · wovepaper