Impact of Inhomogeneous Reionization on Cosmic Microwave Background Anisotropy

@article{Knox1998ImpactOI,
  title={Impact of Inhomogeneous Reionization on Cosmic Microwave Background Anisotropy},
  author={Lloyd Knox and Rom'an Scoccimarro and Scott Dodelson},
  journal={Physical Review Letters},
  year={1998},
  volume={81},
  pages={2004-2007}
}
It is likely that the reionization of the Universe did not occur homogeneously. Using a model that associates ionized patches with overdense regions, we find that the resulting cosmic microwave background (CMB) anisotropy power spectrum peaks at angular scales corresponding to the extent of the ionized regions, and has a width that reflects the correlations between them. There is considerable uncertainty in the amplitude. Neglecting inhomogeneous reionization in the determination of… 

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References

SHOWING 1-2 OF 2 REFERENCES

Large-scale structure in the Universe

A variety of observations constrain models of the origin of large-scale cosmic structures. Enough observational data have accumulated to constrain (and perhaps determine) the power spectrum of

Astrophys

  • J. 284, L9
  • 1984