Magnetized LambdaCDM inhomogeneities and the cosmic dark ages

TL;DR

This paper derives exact solutions for perturbations in a magnetized LambdaCDM universe during the dark ages, comparing growth rates with standard models and constraining magnetic effects through CMB anisotropies.

Contribution

It provides exact solutions for magnetized perturbations during the dark ages and compares growth rates with standard cosmology, offering new constraints on cosmic magnetic fields.

Findings

Magnetized growth rate of matter perturbations analyzed

Constraints on magnetic fields from CMB anisotropies derived

Comparison with standard LambdaCDM growth index

Abstract

Exact solutions of the perturbations equations in the magnetized LambdaCDM scenario are presented. They apply during the dark ages and, more specifically, after the baryons are freed from the drag of the photons. The magnetized growth rate of matter perturbations is compared with the growth index obtained in the concordance paradigm and under the assumption that dark energy does not cluster for a redshift window ranging from the epoch of reionization to the stage of dark-energy dominance. The constraints derived from this analysis are shown to be qualitatively complementary and quantitatively competitive with the bounds stemming from the analysis of the distortion patterns induced by the magnetized adiabatic mode on the temperature and polarization anisotropies of the Cosmic Microwave Background.