The theory of CMB anisotropies
Ruth Durrer

TL;DR
This review comprehensively covers the theoretical framework of CMB anisotropies, including gauge-invariant perturbation theory, analytical approximations, damping effects, observational status, and the numerical system of equations.
Contribution
It provides an updated, detailed overview of the theory of CMB anisotropies, including analytical methods and the full differential system for numerical analysis.
Findings
Analytical approximations for acoustic peak positions derived
Discussion of Silk damping via analytic approximation
Overview of current observational status and parameter estimation
Abstract
This is a review of the theory of CMB anisotropies, an updated version of a course given at the troisieme cycle de la Suisse Romande. An introduction to gauge invariant cosmological perturbation theory is given and the theory CMB anisotropies is develiped in this context. Simple analytical approximations for the acoustic peak positions for adiabatic and isocurvature perturbations are derived. Silk damping is discussed by an analytic approximation. A short description of the present status of observations and parameter estimation followed by a critical discussion terminate the review. The full system of differential equations for CMB anisotropies and polarization needed in a numerical treatment is also developed and given in an appendix.
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Taxonomy
TopicsCosmology and Gravitation Theories · Radiative Heat Transfer Studies · Gas Dynamics and Kinetic Theory
