Abstract
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 re-ionization.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 254 |
| Number of pages | 1 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 2 |
| Issue number | 14 |
| DOIs | |
| State | Published - Aug 2006 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
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