Using the entropy-based flux limiter in both eccentricity reduction and evolution yields apparent fifth-order convergence in binary neutron star waveform phase.
Following [7, 9], we use the curvature scalar Ψ 4 to compute the GWs on spheres at distance r from the origin
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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.