Gravitational-wave parameter estimation with machine-learning generated surrogate waveforms
The worldwide network of gravitational-wave detectors have detected more than 350 binary coalescence events till date. Future third-generation detectors, like Einstein telescope, are expected to detect orders-of-magnitude more signals from sources with more complicated characteristics, including eccentric orbits and high-mass ratio binaries. It is well-established that the computational cost of parameter estimation for signals from these kinds of sources will be extremely high. In particular, the process could be sped-up if generating theoretical waveform predictions, used for likelihood calcu
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- LinkedLinked via arxiv author · 85%Suyog Garg →
“Gravitational-wave parameter estimation with machine-learning generated surrogate waveforms”
- LinkedLinked via arxiv author · 85%Kipp Cannon →
“Gravitational-wave parameter estimation with machine-learning generated surrogate waveforms”
