In our group, we use high performance computing facilities to unravel the mysteries of the Universe. Due to the simulation of binary neutron star systems, we are able to constrain the behavior of matter at supranuclear densities and to estimate the expansion rate of the Universe. Our simulations are the fundament to develop new models to describe the gravitational wave signals released during the coalescence of compact binaries and to model electromagnetic signatures created during and after the collision of ultracompact neutron stars.
Binary Neutron Star Merger Simulation
Numerical relativity simulation of the last few milliseconds of two inspiraling and merging neutron stars. Higher densities are shown in blue, lower densities are shown in cyan. The final black hole is shown in gray.
Credits: - T. Dietrich (University of Potsdam), S. Ossokine, H. Pfeiffer, A. Buonanno (Max Planck Institute for Gravitational Physics)
18th of May 2021
On 16th of June Prof. Dietrich will hold his inaugural lectures at the Science faculty of the University of Potsdam.
12th of May 2021
44.1 Million CPUhs granted
on SuperMUC_NG for the project `Analyzing and Interpreting Compact Binary Mergers' .
11th of May 2021
Theoretical Astrophysics group supports analysis of the shortest long gamma-ray burst observed yet; paper accepted in Nature Astronomy.