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• W2018984913 abstract "We study scalar mode perturbations (magnetosonic waves) induced by a helical stochastic cosmological magnetic field and derive analytically the corresponding cosmic microwave background (CMB) temperature and polarization anisotropy angular power spectra. We show that the presence of a stochastic magnetic field, or an homogeneous magnetic field, influences the acoustic oscillation pattern of the CMB anisotropy power spectrum, effectively acting as a reduction of the baryon fraction. We find that the scalar magnetic energy density perturbation contribution to the CMB temperature anisotropy is small compared to the contribution to the CMB $E$-polarization anisotropy." @default.
• W2018984913 created "2016-06-24" @default.
• W2018984913 creator A5062376442 @default.
• W2018984913 creator A5071569623 @default.
• W2018984913 date "2007-01-10" @default.
• W2018984913 modified "2023-09-23" @default.
• W2018984913 title "CMB anisotropies due to cosmological magnetosonic waves" @default.
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• W2018984913 doi "https://doi.org/10.1103/physrevd.75.023002" @default.
• W2018984913 hasPublicationYear "2007" @default.
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