Surrogate model of gravitational waveforms for quasi-circular, spin-aligned, asymmetric-mass black hole binaries based on the hybridization of WaSABI-C inspirals with numerical relativity waveforms

H. L. Iglesias, D. M. Shoemaker

With the incorporation of aligned-spin dynamics into self-force waveform models, such as the WaSABI-C inspiral model, and with the release of the SXS collaboration's third public c…