Numerical simulations of scalar dark matter around binary neutron star mergers

The numerical gravitational waveforms for the binary configurations simulated in the paper "Numerical simulations of scalar dark matter around binary neutron star mergers" The waveforms are produced using the NR code BAM, for different scalar field masses, profiles (Cloud and Gaussian-decay), different binary masses, and for three different resolutions, along with vacuum reference simulations, labelled 'No field'. Computations for this paper have been performed on the DFG-funded research cluster Jarvis at the University ofPotsdam (INST 336/173-1; Project No. 502227537).