معرفی
Hendrik Schatz is a University Distinguished Professor in the Department of Physics & Astronomy at Michigan State University, where he also serves as Director of the JINA Center for the Evolution of the Elements, a NSF Physics Frontiers Center. His research is conducted at the intersection of nuclear physics and astrophysics, primarily at the National Superconducting Cyclotron Laboratory (NSCL) and the Facility for Rare Isotope Beams (FRIB).
His research focuses on understanding nuclear processes that occur in cosmic environments through experimental studies with radioactive beams. Key areas include:
- Experimental nuclear astrophysics using accelerator facilities
- X-ray bursts on neutron stars
- Neutron star crust composition and heating
- Rapid neutron capture process (r-process) for element formation
- Nuclear reactions in extreme astrophysical environments
Schatz's research program addresses fundamental questions about the origin of elements in nature, particularly those created in supernovae, hydrogen explosions on neutron stars and white dwarfs, and neutron star crusts. His group conducts experiments measuring beta delayed neutron emission, gamma ray spectroscopy of exotic nuclei, and mass measurements of neutron-rich nuclei using advanced detector systems like NERO, GRETINA, and the S800 spectrometer. A significant focus is utilizing the unique beams provided by the ReA3 facility for nuclear astrophysics research.
His research is embedded in the interdisciplinary framework of the Joint Institute for Nuclear Astrophysics (JINA), where graduate students participate in all stages of the research process, from experimental design to astrophysical modeling. This approach provides students with a comprehensive education spanning nuclear physics, astrophysics, and astronomy.
Schatz has published extensively in top journals including Nature, Physical Review Letters, and Astrophysical Journal, with recent work focusing on precision mass measurements, nuclear reaction rates for astrophysical models, and neutron star crust physics. His research has significant implications for understanding cosmic element formation and the behavior of matter under extreme conditions.
As an educator, Schatz teaches undergraduate physics courses, a graduate-level nuclear astrophysics course he developed, and participates in summer and winter schools. He has created extensive teaching materials available online, emphasizing cooperative learning techniques.
Contact Information:
- Email: schatz@msu.edu, schatz@nscl.msu.edu
- Phone: +1 (517) 908-7397
- Office: 2006 Cyclotron Building, 640 S Shaw Lane, East Lansing MI 48864
