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The dark universe: dark matter and dark energy
This video was recorded at CERN Academic Training Lectures 2008. According to the standard cosmological model, 95% of the present mass density of the universe is dark: roughly 70% of the total in the form of dark energy and 25% in the form of dark matter. In a series of four lectures, I will begin by presenting a brief review of cosmology, and then I will review the observational evidence for dark matter and dark energy. I will discuss some of the proposals for dark matter and dark energy, and connect them to high-energy physics. I will also present an overview of an observational program to quantify the properties of dark energy.
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This work is licensed under a Attribution-NonCommercial-NoDerivs 3.0 United States
