Tuesday, February 21, 2006

Dark energy and the future of the universe

I just gave this talk at the UO Center for High Energy Physics (PDF slides). I'm giving it as a colloquium at Washington University in St. Louis and the University of Kansas later in the spring, so no peeking if you are from one of those places.

Title: Dark Energy and the Future of the Universe

Abstract: Recent observations of Type Ia supernovae, cosmic microwave background radiation and large scale structure indicate that the expansion rate of the universe is increasing. A number of models describing exotic forms of matter, generically referred to as dark energy (not to be confused with dark matter), have been proposed to explain this acceleration. For example, the dark energy may be due to Einstein's cosmological constant. In this talk I will give an introduction to big bang cosmology and dark energy, with emphasis on the dark energy equation of state and how it determines the future (large time evolution) of the universe.

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