Rate My Professor Christoph Federrath

Professor Christoph Federrath is a faculty member, Professor, and Associate Director for Higher Degree Research at the Research School of Astronomy and Astrophysics, Australian National University. He studied physics at the University of Würzburg from 2001 to 2007 and received his PhD (Dr. rer. nat.) in Turbulence and Star Formation from the University of Heidelberg in 2010. Following his doctoral work, Federrath held postdoctoral fellowships at the Institute for Theoretical Astrophysics in Heidelberg, the Ecole Normale Superieure de Lyon, and the Monash Centre for Astrophysics in Melbourne. He joined the Australian National University as an Australian Research Council Future Fellow and Stromlo Fellow, advancing to his current professorial role where he leads a research group focused on computational astrophysics.

Federrath's research centers on the physics and chemistry of star-forming gas clouds, star formation processes in the present-day and early Universe, fluid dynamics, turbulence, and magnetic fields. He develops theoretical models and conducts supercomputer simulations of molecular clouds, integrating turbulence, gravity, magnetic fields, radiation, stellar feedback, and chemical evolution, with direct comparisons to observations of galactic clouds. His work aims to create self-consistent models for predictions in galaxy, star, and planet formation. Notable publications include Beattie et al. (2025) 'Living Reviews in Computational Astrophysics'; Federrath et al. (2021) in Nature Astronomy on supersonic turbulence universality; Federrath (2020) in IAU Symposium 345; and Sharda, Federrath & Krumholz (2020) in Monthly Notices of the Royal Astronomical Society on magnetic field amplification. Federrath has received the Australian Research Council Future Fellowship, Stromlo Fellowship, and was a joint winner of the 2024 Anne Green Prize from the Astronomical Society of Australia. His scholarship demonstrates substantial influence in astrophysics, evidenced by an h-index of 71 and extensive citations documented on Google Scholar.