No reviews yet. Be the first to rate Falk!
Falk Herwig is a Professor of Astrophysics at the University of Victoria in the Department of Physics and Astronomy, where he also serves as Director of the Astronomy Research Centre. He leads the Computational Stellar Astrophysics group, which uses high-performance computing to perform 3D hydrodynamics simulations exploring stellar convection, internal gravity waves, and the nuclear origins of the elements. His research focuses on stellar evolution, hydrodynamics, and nuclear astrophysics of single and binary stars, including nucleosynthesis simulations, the origin of the elements in stars and stellar explosions, and the chemical evolution of galaxies. Herwig obtained his PhD from the University of Kiel and the Astrophysikalisches Institut Potsdam in Germany. He has held postdoctoral positions in Potsdam and Victoria prior to his faculty appointment at the University of Victoria. Herwig has authored or co-authored over 200 peer-reviewed articles, with research contributions including studies on the evolution of helium white dwarfs, convective overshooting in asymptotic giant branch stars, and the formation of hydrogen-deficient post-AGB stars. His work is associated with collaborations such as the NuGrid collaboration and the Joint Institute for Nuclear Astrophysics. He maintains an active research program supported by allocations on Canadian high-performance computing resources.
Herwig’s professional activities center on advancing understanding of stellar interiors and element production through computational methods. As group leader, he oversees a team that includes senior research associates, postdoctoral fellows, and graduate students, many co-supervised with researchers at TRIUMF. His expertise encompasses stellar hydrodynamics and the origin of the elements, areas in which he has contributed foundational insights through both theoretical modeling and simulation. Publicly available information from university profiles confirms his role in the Faculty of Science and ongoing leadership in computational astrophysics initiatives at the institution.
Discover how University of Victoria researchers used supercomputers to solve the red giant stars mystery, revealing rotation's role in chemical mixing. Implications for stellar evolution and our Sun.
Photo by Mufid Majnun on Unsplash
Photo by Shubham Sharan on Unsplash
Photo by Shubham Sharan on Unsplash
Photo by Evan Marvell on Unsplash
Photo by Markus Winkler on Unsplash
Photo by Patrick Robert Doyle on Unsplash
Photo by Brandi Redd on Unsplash
Have a story or a research paper to share? Become an Expert Academic Contributor and publish your work on AcademicJobs.com.
Write news and research articles as a expert academic in your field publish your work on AcademicJobs.com
