Effects of primordial magnetic fields on 21 cm multifrequency angular power spectra
Abstract: The cosmic 21 cm line signal of neutral hydrogen provides the possibility to constrain the matter power spectrum. Primordial magnetic fields present before decoupling have an effect on the linear matter power spectrum. The redshifted 21 cm line signal is observed at different frequencies allowing to determine multifrequency angular power spectra. These are presented for cosmological models including the adiabatic, primordial curvature mode as well as the compensated magnetic mode for different values of the magnetic field parameters. For multifrequency angular power spectra frequency ranges have been set around central frequencies of uGMRT Band 3 data as well as MeerKAT L band data. For these signal-over-noise ratios are obtained as well as for SKA1-MID which is part of the currently under construction SKAO.
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