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M Zaldarriaga (Harvard University)
I will discuss the physical mechanisms that generate Polarization in the Cosmic Microwave Background and the current observational status. I will explain what we expect to learn from future measurements of the polarization such as details about how the universe reionized and what was the energy scale of inflation.
The author(s) of this abstract have provided an email address for comments about the abstract: mzaldarriaga@cfa.harvard.edu
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Bulletin of the American Astronomical Society, 35 #3
© 2003. The American Astronomical Soceity.