Using the entropy-based flux limiter in both eccentricity reduction and evolution yields apparent fifth-order convergence in binary neutron star waveform phase.
IV A provides compelling evidence that the use of the pure EFL case results in GWs with significantly improved accuracy and enhanced convergence properties
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Eccentricity reduction of binary neutron star initial data with the entropy based flux limiting scheme
Using the entropy-based flux limiter in both eccentricity reduction and evolution yields apparent fifth-order convergence in binary neutron star waveform phase.