Probing correlations of early magnetic fields using mu-distortion
arXiv:1404.5957 · doi:10.1088/1475-7516/2014/08/018
Abstract
The damping of a non-uniform magnetic field between the redshifts of about and injects energy into the photon-baryon plasma and causes the CMB to deviate from a perfect blackbody spectrum, producing a so-called -distortion. We can calculate the correlation of this distortion with the temperature anisotropy of the CMB to search for a correlation between the magnetic field and the curvature perturbation ; knowing the correlation would help us distinguish between different models of magnetogenesis. Since the perturbations which produce the -distortion will be much smaller scale than the relevant density perturbations, the observation of this correlation is sensitive to the squeezed limit of , which is naturally parameterized by (a parameter defined analogously to ). We find that a PIXIE-like CMB experiments has a signal to noise , where is the magnetic field's strength on -distortion scales normalized to today's redshift; thus, a 10 nG field would be detectable with . However, if the field is of inflationary origin, we generically expect it to be accompanied by a curvature bispectrum induced by the magnetic field. For sufficiently small magnetic fields, the signal will dominate, but for nG, one would have to consider the specifics of the inflationary magnetogenesis model. We also discuss the potential post-magnetogenesis sources of a correlation and explain why there will be no contribution from the evolution of the magnetic field in response to the curvature perturbation.
23 pages, 1 figure. v2: Noted that a competing effect could potentially be smaller than originally stated. Fixed references. Matches JCAP version