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We present the constraints on the amplitude of magnetic fields generatedprior to the recombination using CMB temperature and polarization anisotropydata from Planck 2018 release, alone and in combination with those fromBICEP2/Keck array and the South Pole Telescope. We model the fields with ageneric parametrization and we make no assumptions on their origin in order toprovide general constraints on their characteristics. The analysis updates theformer corresponding Planck 2015 results both on data and numericalimplementation. We then perform forecasts for the next generation of CMBexperiments such as LiteBIRD satellite alone and in combination with futureground based experiments.

journal of cosmology and astroparticle physics

Constraints on primordial magnetic fields from magnetically-induced  perturbations: current status and future perspectives with LiteBIRD and  future ground based experiments