Cosmic Microwave Background: Probing the Universe from Z=6 -1100

Details Cosmic Microwave Background: Probing the Universe from Z=6 -1100 Cosmic Microwave Background: Probing the Universe from Z=6 -1100

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...7e...6s&link_type=abstract

The Universe at z > 6, 26th meeting of the IAU, Joint Discussion 7, 17-18 August 2006, Prague, Czech Republic, JD07, #6

Physics

1

Scientific paper

Observations of cosmic microwave background temperature and polarization fluctuations are sensitive to both physical conditions at recombination (z = 1100) and physical process along the line of sight. I will discuss recent results from the Wilkinson Microwave Anisotropy Probe and planned ground and space-based observations. The talk will emphasize the role of CMB observations in determining the initial conditions for the growth of structure and as a probe of the physics of reionization.

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