Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries

@article{Pan2011PostNewtonianFM,
title={Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries},
author={Yi Pan and A. Buonanno and R. Fujita and E. Racine and H. Tagoshi},
journal={Physical Review D},
year={2011},
volume={83},
pages={109901}
}

‘m , agree quite well with the numerical amplitudes up to the Kerr-spin value q � 0:95 for orbital velocities v � 0:4. The numerical amplitudes are computed solving the Teukolsky equation with a spectral code. The agreement for prograde orbits and large spin values of the Kerr blackhole can be further improved at high velocities by properly factoring out the lower-order post-Newtonian contributions in � ‘m. The resummation procedure results in a better and systematic agreement between numerical… CONTINUE READING