Michael Wiescher

Michael Wiescher received his Diploma Degree in condensed matter physics at the University of M√ľnster, Germany, in 1974. He received his Ph.D. in nuclear physics at the same university in 1980 with a thesis on stellar hydrogen burning in massive stars. Following post-doctoral research at Ohio State University, the University of Mainz, Germany, and the California Institute of Technology, he joined the faculty of the Physics Department at the University of Notre Dame, in 1986. He holds the Freimann Chair of Physics and serves as the Director of the Nuclear Science Laboratory at Notre Dame and as the Director of the Joint Institute for Nuclear Astrophysics (JINA), an NSF Physics Frontier Center of the University of Notre Dame, Michigan State University, and the University of Chicago. He is also Adjunct Professor at Michigan State University and the University of Surrey, UK. His research interests include the measurement and simulation of nuclear reaction rates and nucleosynthesis processes in stellar evolution and explosion environments. Michael Wiescher is a Fellow of the American Physical Society and the Humboldt Gesellschaft in Germany. In 2003 he was awarded the Bethe Prize of the Divisions of Nuclear Physics and Astrophysics of the American Physical Society. He has given more than 100 invited presentations at national and international conferences and nearly 100 seminars and colloquia, and has published more than 200 refereed articles.

Michael Wiescher Published August 17, 2009

Astrophysics | Nuclear Physics

Advances in experimental techniques that measure nuclear reactions that occur in stars are opening new opportunities for understanding the stellar and chemical evolution of our Universe.