Enhancing gravitational waveform models through dynamic calibration

@article{Setyawati2019EnhancingGW,
  title={Enhancing gravitational waveform models through dynamic calibration},
  author={Y. Setyawati and F. Ohme and S. Khan},
  journal={Physical Review D},
  year={2019},
  volume={99},
  pages={024010}
}
  • Y. Setyawati, F. Ohme, S. Khan
  • Published 2019
  • Physics
  • Physical Review D
  • Strategies to model the inspiral, merger and ringdown gravitational waveform of coalescing binaries are restricted in parameter space by the coverage of available numerical-relativity simulations. When more numerical waveforms become available, substantial efforts to manually (re-)calibrate models are required. The aim of this study is to overcome these limitations. We explore a method to combine the information of two waveform models: an accurate, but computationally expensive target model… CONTINUE READING
    4 Citations

    Figures and Tables from this paper

    References

    SHOWING 1-10 OF 69 REFERENCES
    Simple model of complete precessing black-hole-binary gravitational waveforms.
    • 283
    • PDF
    Numerical relativity waveform surrogate model for generically precessing binary black hole mergers
    • 79
    • Highly Influential
    • PDF
    Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries
    • 37
    • Highly Influential
    • PDF