Cosmological Perturbations with Multiple Fluids and Fields
arXiv:astro-ph/0103244 · doi:10.1088/0264-9381/19/3/308
Abstract
We consider the evolution of perturbed cosmological spacetime with multiple fluids and fields in Einstein gravity. Equations are presented in gauge-ready forms, and are presented in various forms using the curvature (Φor Ï_Ï) and isocurvature (S_{(ij)} or δÏ_{(ij)}) perturbation variables in the general background with K and Î. We clarify the conditions for conserved curvature and isocurvature perturbations in the large-scale limit. Evolutions of curvature perturbations in many different gauge conditions are analysed extensively. In the multi-field system we present a general solution to the linear order in slow-roll parameters.
19 pages, 6 figures, revised thoroughly; published version in Class. Quant. Grav