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The Smooth Universe ·
Three Lectures
Scott
Dodelson
(Fermilab)
April 3 – 10, 2006
The past decade has seen an explosion in the quantity and quality of
comsological data. Coincident with this, we have developed a coherent
picture of the evolution of the universe,
one which relies heavily on physics beyond the
Standard Model. These lectures provide an overview of this picture, with
an emphasis on the evidence for dark matter, dark energy, and
inflation. This evidence comes from observations of distant supernovae,
anisotropies in the cosmic microwave background, and surveys of the matter
distribution in the universe.
Part 1 · Monday,
April 3 · Video
Part 2 · Wednesday,
April 5 · Video
Part 3 · Monday, April 10 · Video
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