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
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