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arxiv: 1210.0308 · v2 · pith:JA34CL2Nnew · submitted 2012-10-01 · 🌌 astro-ph.CO · gr-qc

Primordial Magnetism in CMB B-modes

classification 🌌 astro-ph.CO gr-qc
keywords primordialb-modesfieldsmagneticbecausecorrelationsinducedmagnetism
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Cosmic Microwave Background (CMB) polarization B-modes induced by Faraday Rotation (FR) can provide a distinctive signature of primordial magnetic fields because of their characteristic frequency dependence and because they are only weakly damped on small scales. FR also leads to mode-coupling correlations between the E and B type polarization, and between the temperature and the B-mode. These additional correlations can further help distinguish magnetic fields from other sources of B-modes. We review the FR induced CMB signatures and present the constraints on primordial magnetism that can be expected from upcoming CMB experiments. Our results suggest that FR of CMB will be a promising probe of primordial magnetic fields.

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