A New delta N Formalism for Multi-Component Inflation
arXiv:astro-ph/0506262 · doi:10.1088/1475-7516/2005/10/004
Abstract
The delta N formula that relates the final curvature perturbation on comoving slices to the inflaton perturbation on flat slices after horizon crossing is a powerful and intuitive tool to compute the curvature perturbation spectrum from inflation. However, it is customarily assumed further that the conventional slow-roll condition is satisfied, and satisfied by all components, during horizon crossing. In this paper, we develop a new delta N formalism for multi-component inflation that can be applied in the most general situations. This allows us to generalize the idea of general slow-roll inflation to the multi-component case, in particular only applying the general slow-roll condition to the relevant component. We compute the power spectrum of the curvature perturbation in multi-component general slow-roll inflation, and find that under quite general conditions it is invertible.
24 pages, no figure
References in corpus (10)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- A General Analytic Formula for the Spectral Index of the Density Perturbations produced during Inflation
- Super-Horizon Scale Dynamics of Multi-Scalar Inflation
- Enhancement of superhorizon scale inflationary curvature perturbations
- The Spectrum of Density Perturbations produced during Inflation to Leading Order in a General Slow-Roll Approximation
- Second Order General Slow-Roll Power Spectrum
- The spectrum of cosmological perturbations produced by a multi-component inflaton to second order in the slow-roll approximation
- The Power Spectrum for a Multi-Component Inflaton to Second-Order Corrections in the Slow-Roll Expansion
- Scale Dependent Spectral Index in Slow Roll Inflation
- From the Spectrum to Inflation : An Inverse Formula for the General Slow-Roll Spectrum
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