Bootstrapping from inflationary magnetogenesis to CMB initial conditions

TL;DR

This paper explores how inflationary magnetogenesis could influence the initial conditions of the CMB anisotropies, linking primordial magnetic fields to observable temperature and polarization spectra.

Contribution

It provides the first computation of CMB temperature and polarization spectra considering inflationary-origin magnetic fields without additional assumptions.

Findings

Angular power spectra are affected by primordial magnetic fields.

The analysis connects inflationary magnetogenesis to observable CMB features.

Results depend on key parameters of the cosmological model.

Abstract

The temperature and polarization anisotropies of the Cosmic Microwave Background are analyzed under the hypothesis that the same inflationary seed accounting for protogalactic magnetism also affects the Einstein-Boltzmann hierarchy whose initial conditions are assigned for typical correlation scales larger than the Hubble radius after matter-radiation equality but before decoupling. Since the primordial gauge spectrum depends on a combination of pivotal parameters of the concordance model, the angular power spectra of the temperature and of the polarization are computed, for the first time, in the presence of a putative large-scale magnetic field of inflationary origin and without supplementary hypotheses.