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Don Winget and his research can be found at

This work will help explore the physical nature of dark matter. Don and his research group use these same data sets to do extreme physics, constraining masses of theoretically proposed particles вЂ“ such as axions and plasmon neutrons. This is currently the only technique sensitive to the kinds of planets we have in our Solar System. He developed and is now implementing a new technique for finding planetary systems like our own solar system. Winget co-founded the Whole Earth Telescope (WET) which uses essentially all of the major optical observatories on the planet working together to defeat dawn. In 1987, he developed a new method for measuring the age of the Galaxy, currently the most accurate method for dating the stellar components of the galaxy. In 1985, he made the first direct measurement of stellar evolution. This was the first time in the 300 year old field of pulsating variable stars that anyone predicted a new class of pulsating variable stars before their discovery. Don Winget predicted and discovered a new class of pulsating variable stars. in Physics and Astronomy from the University of Rochester in 1982.

in Physics from the University of Illinois in 1976 and his Ph.D. Smith Centennial Professor in Astronomy and University Distinguished Teaching ProfessorДepartment of Astronomy and McDonald Observatory, The University of Texas at Austin Physics visitors, and physics students, joined President Jones for a small celebration of the end of our colloquium series.ДЄpril 29-The Scientific Potential of White Dwarf Stars: From the Telescope to the Laboratory and Back Again, Adventures in High Energy Density Plasmas'Дr. Some of these questions will be highlighted in this presentation, with a focus on a broadly understood strongly-interacting many-body problem. Through these research frontiers, nuclear scientists are addressing the basic questions that drive our field. Nuclear science today is focused on three broad but highly related research frontiers: (1) quantum chromodynamics, which ultimately will tell us how nuclei are held together (2) the structure of atomic nuclei and nuclear astrophysics, which addresses the origin of the elements and (3) a new standard model of fundamental particles. Witek Nazarewicz and his research can be found at

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Nazarewicz has helped organize more than 30 meetings and conferences and presently serves on 14 professional committees and editorial boards.В More information about Prof. He has given ~165 invited talks at major international conferences and more than 200 invited seminars and colloquia. He has also made more than 150 contributions to major conferences, published in their respective proceedings. He is listed by ISI among the most highly-cited physicists. He is the author of seven review papers and more than 270 refereed publications in scientific journals. Witek Nazarewicz is a distinguished theorist with broad expertise in nuclear physics and computational many-body problem. He was named a 2008 Carnegie Centenary Professor by the Carnegie Trust in Scotland.

Institute of Physics, and a member of the Polish Physical Society and the European Physical Society. Nazarewicz is a Fellow of the American Association for the Advancement of Science, American Physical Society and the U.K. He has held several visiting positions, including professorships at Lund University, the University of Cologne, Kyoto University, and the University of Liverpool. He is also a member of the Joint Institute for Heavy Ion Research directorate. He is an adjunct faculty member in the Oak Ridge National Laboratory Physics Division and has been serving as the Scientific Director of the ORNL Holifield Radioactive Ion Beam Facility since 1999. Witold Nazarewicz is a Professor of Physics at both the University of Tennessee and Warsaw University, Poland. from Warsaw Institute of Technology in 1981. Professor Witek Nazarewicz received his Ph.D. Witold Nazarewicz University of Tennessee at Knoxville and Oak Ridge National Laboratory Spring 2010 Colloquia Physics and Astronomy Colloquium - Spring - 2010 (4-5pm, Science Bldg.