Computational astrophysics studies in turbulence, magnetic fields, and star/galaxy formation and evolution
Study of the statistics of turbulent, magnetised gases, relevant for the structure and evolution of the interstellar medium, the formation and evolution of stars and galaxies, using a combination of supercomputer simulations, theory, analytical calculations, and comparison to observations.
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This project is open for Bachelor, Honours and PhD students.
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You would be part of Federrath's Research Group, studying the statistics of turbulent, magnetised gases, relevant for the structure and evolution of the interstellar medium, the formation and evolution of stars and galaxies, using a combination of supercomputer simulations, theory, analytical calculations, and comparison to observations.