# Entropy-limited higher-order central scheme for neutron star merger simulations

@article{Doulis2022EntropylimitedHC, title={Entropy-limited higher-order central scheme for neutron star merger simulations}, author={Georgios Doulis and Florian Atteneder and Sebastiano Bernuzzi and Bernd Br{\"u}gmann}, journal={Physical Review D}, year={2022} }

Numerical relativity simulations are the only way to calculate exact gravitational waveforms from binary neutron star mergers and to design templates for gravitational-wave astronomy. The accuracy of these numerical calculations is critical in quantifying tidal eﬀects near merger that are currently one of the main sources of uncertainty in merger waveforms. In this work, we explore the use of an entropy-based ﬂux-limiting scheme for high-order, convergent simulations of neutron star spacetimes…

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