Bootstrapping from inflationary magnetogenesis to CMB initial conditions
arXiv:1303.3895 · doi:10.1088/0264-9381/30/20/205017
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.
34 pages, 5 figures
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- Reduced bispectrum seeded by helical primordial magnetic fields
- Scaling laws and sum rules for the B-mode polarization
- Statistical anisotropy from inflationary magnetogenesis
- Tensor B mode and stochastic Faraday mixing
- Spectator Higgs, large-scale gauge fields and the non-minimal coupling to gravity