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arXiv · 0812.3652

Cosmological Perturbations at Second Order and Recombination Perturbed

Leonardo Senatore·Svetlin Tassev·Matias Zaldarriaga
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Abstract

We derive the full set of second-order equations governing the evolution of cosmological perturbations, including the effects of the first-order electron number density perturbations, δ_e. We provide a detailed analysis of the perturbations to the recombination history of the universe and show that a perturbed version of the Peebles effective 3-level atom is sufficient for obtaining the evolution of δ_e for comoving wavenumbers smaller than 1Mpc^{-1}. We calculate rigorously the perturbations to the Lyαescape probability and show that to a good approximation it is governed by the local baryon velocity divergence. For modes shorter than the photon diffusion scale, we find that δ_e is enhanced during recombination by a factor of roughly 5 relative to other first-order quantities sourcing the CMB anisotropies at second order. Using these results, in a companion paper we calculate the CMB bispectrum generated during recombination.

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Leonardo Senatore, Svetlin Tassev, Matias Zaldarriaga. 2008-12-18. Cosmological Perturbations at Second Order and Recombination Perturbed. https://doi.org/10.1088/1475-7516/2009/08/031

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