• Theoretische Astrophysik

Theoretical Astrophysics Group

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 denisties 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. 

NEWS

Due to Corona:

„Lectures for the class multi-messenger astronomy will be held online for the first few weeks. More information are available via pulse/moodle. If you have further questions, please contact me.“