Speaker
Prof.
Tim Dietrich
(University of Potsdam)
Description
Numerical-relativity simulations are prerequisites for a reliable interpretation of multi-messenger events such as binary neutron star or black hole neutron star mergers. When using simulation results to interpret observational data, it is of uttermost importance to also ensure a proper discussion of the uncertainties of the simulations. Keeping this in mind, we show some of our most recent results and identify how simulation uncertainties could affect the development of gravitational-wave and electromagnetic models. Finally, we will discuss some of the most recent developments of our numerical-relativity code BAM and review its capability and shortcomings in simulating compact binary mergers.
