Dr. Claudius Birke
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James Watt, Christoph Federat, Claudius Birke, Christian Klingenberg
Mitigating numerical dissipation in simulations of subsonic turbulent flows,
Monthly Notices of the Royal Astronomical Society, vol. 544, issue 4 (2025) -
Claudius Birke, Walter Boscheri, Christian Klingenberg
A well-balanced semi-implicit IMEX finite volume scheme for ideal Magnetohydrodynamics at all Mach numbers,
Journal of Scientific Computing, vol. 98, no. 34, (2024) -
Claudius Birke, Christophe Chalons, Christian Klingenberg
A low Mach two-speed relaxation scheme for the compressible Euler equations with gravity
Communications in Mathematical Sciences, vol. 21 (2023) -
Giovanni Leidi, Claudius Birke, Robert Andrassy, Johann Higl, Philipp Edelmann, Gabriel Wiest, Christian Klingenberg, Friedrich Röpke
A finite-volume scheme for modelling compressible MHD flows at low Mach numbers in stellar interiors,
Astronomy & Astrophysics, vol. 668, no A13 (2022)
Conference Proceedings:
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Claudius Birke, Christian Klingenberg
A Low Mach Two-speed Relaxation Scheme for Ideal MHD Equations
Springer Proceedings in Mathematics & Statistics, Finite Volume and Complex Applications X (2023) -
Claudius Birke, Walter Boscheri, Christian Klingenberg
A high order semi-implicit scheme for ideal magnetohydrodynamics
Springer Proceedings in Mathematics & Statistics, Finite Volume and Complex Applications X (2023) -
Claudius Birke, Christian Klingenberg
Finding an Approximate Riemann Solver via Relaxation: Concept and Advantages
SEMA SIMAI Springer Series: Proceedings of HYP 2022 (2023)
| Oct. 2013 – Sept. 2019 | Bachelor and Master studies of Business Mathematics, University of Cologne, Cologne, Germany |
| Sept. 2019 | Master degree Master thesis: Entropy-stable space-time DG method for the compressible Euler equations in 2D Advisor: Prof. Dr.-Ing. Gregor Gassner |
| Oct. 2019 - Feb. 2024 | PhD studies, Institute of Mathematics, University of Wuerzburg, Germany Advisor: Prof. Dr. Christian Klingenberg |
| May 2024 | PhD |
In my research I work on finite volume methods for the compressible Euler as well as magnetohydrodynamics equations including gravitational source terms. The focus is on the development of methods that are able to maintain hydrostatic equilibria and at the same time provide accurate numerical solutions for problems with low Mach numbers. These methods find practical application, for example, in astrophysics for the simulation of gas flows in the interior of stars.
