The Density Perturbation Power Spectrum to Second-Order Corrections in the Slow-Roll Expansion
arXiv:astro-ph/0101225 · doi:10.1016/S0370-2693(01)00616-5
Abstract
We set up a formalism that can be used to calculate the power spectrum of the curvature perturbations produced during inflation up to arbitrary order in the slow-roll expansion, and explicitly calculate the power spectrum and spectral index up to second-order corrections.
11 pages, errors corrected
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