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Distinguished Lecturer: Fall 2005


Dr. Joseph Silk
Savilian Professor
of Astronomy -
University of Oxford
JOSEPH SILK has been Savilian Professor of Astronomy at the University of Oxford since 1999. Prior to that, he was at the University of California, Berkeley, preceded by postdoctoral stints in Princeton and Cambridge. He obtained his Ph.D. from Harvard University. He has held an Alfred P. Sloan Foundation Fellowship, a Guggenheim fellowship, and a Blaise-Pascal International Research Chair. He is a Fellow of the Royal Society, the American Physical Society, the American Association for the Advancement of Science, and the Institute of Physics, as well as an honorary member of the French Physical Society. He is the author or coauthor of more than 350 papers in refereed journals, 150 conference and review articles, 70 popular articles, and has given more than 250 invited lectures at conferences. Dr. Silk has succeeded in revitalizing research activities in Astrophysics at Oxford including doubling the size of the program during his tenure as head from 1999-2004 - helping to bring Oxford to a leading role at the international level in cosmology and in the design studies of the European Extremely Large Telescope, a 50m class telescope, and of the Square Kilometre Array radio telescope. In addition to his teaching obligations at Oxford, Dr. Silk frequently gives lecture courses at international schools, radio interviews, and public lectures. He writes book reviews, popular articles, and books. His popular books include The Left Hand of Creation, The Big Bang, and A Short History of the Universe. Dr. Silk’s research interests are in theoretical cosmology, seeking insights about dark matter, galaxy formation, and the cosmic microwave background. He has made notable research contributions in the area of cosmic microwave background radiation, the relic glow from the Big Bang. He made key predictions that motivated increasingly more sensitive experimental searches for more than three decades until success was eventually achieved in the 1990s.

General Public Lecture
“The Dark Side of the Universe”
Wednesday, November 16, 2005   7:30 PM, PSF 173
Abstract: I will discuss how the old Big Bang cosmology from the Einstein/Friedmann/Lemaitre era was transformed by the concept of inflation. The ensuing emergence of cosmic structure is an outcome that has been studied by peering back through the mists of time, both by observing the most remote objects in the universe and by deciphering the fossil structure of nearby galaxies. One of the greatest mysteries in the cosmos is that it is mostly dark. What is the nature of the dark matter? Can we ever hope to detect it?

Department of Physics Colloquium
“A Voyage in Time: The Cosmic Microwave Background”
Thursday, November 17, 2005   4:00 PM, PSF 101
Abstract: One of our greatest challenges is understanding the origin of the structure of the universe. I will describe how the fossil radiation from the beginning of the universe, the cosmic microwave background, has provided a window for probing the initial conditions from which structure evolved. Infinitesimal variations in temperature on the sky, first discovered in 1992, provide the fossil fluctuations that seeded the formation of the galaxies. The microwave radiation has now been mapped with ground-based, balloon-borne and satellite telescopes, and provides the basis for precision cosmology. Its current status and future challenges will be described.
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