The Power Spectrum for a Multi-Component Inflaton to Second-Order Corrections in the Slow-Roll Expansion
arXiv:astro-ph/0202098 · doi:10.1016/S0370-2693(02)02004-X
Abstract
We derive the power spectrum of the density perturbations produced during inflation up to second-order corrections in the standard slow-roll approximation for an inflaton with more than one degree of freedom. We also present the spectral index up to first-order corrections including previously missing terms, and the running to leading order.
11 pages, no figure. KAIST-TH 2002/01
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