The Cosmic Microwave Background (CMB) radiation has enabled us to probe conditions in the early universe with incredible precision. The QUaD experiment is one of the first to report detailed measurements of the polarization of the CMB, which provides extra information that complements temperature measurements. Dr. Church will discuss the implications of the QUaD data and set the stage for what we can expect from future, more sensitive experiments.
Cosmic Microwave Background Measurements with the QUaD Experiment
Details
Date
Wednesday, June 23 2010 - 12:00 pm, PDT
Speaker
Sarah Church
Affiliation
Deputy Director of KIPAC, Stanford University
Description
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