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arxiv: gr-qc/0604081 · v3 · submitted 2006-04-19 · 🌀 gr-qc · astro-ph· hep-th

Second Order Gauge-Invariant Perturbations during Inflation

classification 🌀 gr-qc astro-phhep-th
keywords ordersecondgaugeinvariantperturbationscontributioncurvatureduring
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The evolution of gauge invariant second-order scalar perturbations in a general single field inflationary scenario are presented. Different second order gauge invariant expressions for the curvature are considered. We evaluate perturbatively one of these second order curvature fluctuations and a second order gauge invariant scalar field fluctuation during the slow-roll stage of a massive chaotic inflationary scenario, taking into account the deviation from a pure de Sitter evolution and considering only the contribution of super-Hubble perturbations in mode-mode coupling. The spectra resulting from their contribution to the second order quantum correlation function are nearly scale-invariant, with additional logarithmic corrections to the first order spectrum. For all scales of interest the amplitude of these spectra depend on the total number of e-folds. We find, on comparing first and second order perturbation results, an upper limit to the total number of e-folds beyond which the two orders are comparable.

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