CMB anisotropy due to tangled magnetic fields in reionized models

@article{Seshadri2005CMBAD,
  title={CMB anisotropy due to tangled magnetic fields in reionized models},
  author={T R Seshadri and Kandaswamy Subramanian},
  journal={Physical Review D},
  year={2005},
  volume={72},
  pages={023004}
}
Primordial tangled cosmological Magnetic Fields source rotational velocity perturbations of the baryon fluid, even in the post-recombination universe. These vortical modes inturn leave a characteristic imprint on the temperature anisotropy of the Cosmic Microwave Background (CMB), if the CMB photons can be rescattered after recombination. Observations from WMAP indicate that the Universe underwent a relatively early reionization (z{sub ri}{approx}15), which does indeed lead to a significant… Expand

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