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Physical Review D
We compute the secondary CMBR anisotropy signal from the reionization of the universe in the presence of tangled magnetic fields. We consider the tangled magnetic-field-induced scalar, vector, and tensor modes for our analysis. The most interesting signal for l<10 arise from tensor perturbations. In particular, we show that the enhancement observed by WMAP in the TE cross-correlation signal for l<10 could be explained by tensor TE cross-correlation from tangled magnetic fields generated duringdoi:10.1103/physrevd.72.103003 fatcat:uppfwwkbgfdxnlf7nuakzalju4