CMB Constraints on a Stochastic Background of Primordial Magnetic Fields
arXiv:1005.0148 · doi:10.1103/PhysRevD.83.123533
Abstract
We constrain a stochastic background of primordial magnetic field (PMF) by its contribution to the angular power spectrum of cosmic microwave background anisotropies. We parametrize such stochastic background by a power-law spectrum with index and by its Gaussian smoothed amplitude on a comoving length . We give an approximation for the spectra of the relevant correlators of the energy-momentum of the stochastic background of PMF for any . By using the WMAP 7 year data in combination with ACBAR, BICEP and QUAD we obtain the constraint nG at 95% confidence level for a stochastic background of non-helical PMF. We discuss the relative importance of the scalar and vector contribution to CMB anisotropies in obtaining these constraints. We then forecast {\sc Planck} capabilities in constraining .
13 pages, 7 figures, 3 tables. Revised version accepted for publication in Phys. Rev. D, conclusions unchanged
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