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gr-qc2024
The representation and computational efficiency of the Tolman-Oppenheimer-Volkoff equations in isotropic coordinates
Dániel Barta
This study aims to provide an analytical scheme for computing equilibrium configurations of relativistic stars by solving the Tolman-Oppenheimer-Volkoff equations directly in isotr…
gr-qc2024
Comparing eccentric waveform models based on post-Newtonian and effective-one-body approaches, over an observationally relevant parameter space
Balázs Kacskovics, Dániel Barta
We used two numerical models, namely the \texttt{CBwaves} and \texttt{SEOBNRE} algorithms, based on the post-Newtonian and effective-one-body approaches for binary black holes evol…