Gauge-invariant perturbations at second order: multiple scalar fields on large scales
arXiv:astro-ph/0506532 · doi:10.1088/1475-7516/2005/11/005
Abstract
We derive the governing equations for multiple scalar fields minimally coupled to gravity in a flat Friedmann-Robertson-Walker (FRW) background spacetime on large scales. We include scalar perturbations up to second order and write the equations in terms of physically transparent gauge-invariant variables at first and second order. This allows us to write the perturbed Klein-Gordon equation at second order solely in terms of the field fluctuations on flat slices at first and second order.
16 pages, no figures, revtex4; v2: sign errors in Eqs. (4.16) and (7.6) corrected, application section added, typos corrected, reference added; v3: minor changes, as published version
References in corpus (7)
- Non-Gaussianity from Inflation: Theory and Observations
- A general proof of the conservation of the curvature perturbation
- Coupled dark energy: Towards a general description of the dynamics
- Adiabatic and entropy perturbations with interacting fluids and fields
- Gauge-Invariant Temperature Anisotropies and Primordial Non-Gaussianity
- Non-Gaussian perturbations in hybrid inflation
- On the conservation of second-order cosmological perturbations in a scalar field dominated universe
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