arXiv Analytics

Sign in

arXiv:astro-ph/9405072AbstractReferencesReviewsResources

Reionization and the Cosmic Microwave Background

Joseph Silk

Published 1994-05-31Version 1

If the COBE detection of CMB fluctuations is used to normalize the power spectrum of primordial density fluctuations in a cold dark matter--dominated universe, early reionization is likely to result in a substantial diminution of primordial temperature fluctuations on degree scales. I argue that the reionization may be non--Gaussian because of feedback effects. Secondary fluctuations on arc--minute scales provide an important probe of the efficiency of rescattering.

Comments: 6 pages, plain Tex, figures can be requested from frost@bkyast.berkeley.edu, CfPA-94-th-02
Categories: astro-ph
Related articles: Most relevant | Search more
arXiv:astro-ph/9602019 (Published 1996-02-05, updated 1996-08-15)
Acoustic Signatures in the Cosmic Microwave Background
arXiv:astro-ph/0101449 (Published 2001-01-25, updated 2001-04-30)
Lensing-induced Non-Gaussian Signatures in the Cosmic Microwave Background
arXiv:astro-ph/9308019 (Published 1993-08-16)
Re-Ionization and its Imprint on the Cosmic Microwave Background