Deep learning algorithms have the potential to dramatically improve predictive models of chirp like gravitational waves.
We assess how accurate models of gravitations waves should be to avoid systematic errors in the measurement of the binaries' parameters.
Results from the LIGO Scientific Collaboration and Virgo Collaboration (LVC) for coalescing binary black holes and binary neutron stars from the GTWC-1 catalog.
Accelerating semi-analytic models of gravitational waves.
Numerical solutions of Einstein's equations are the only way to describe the merger accurately.
Dynamical systems can have solutions which a shape that mimics itself on different scales.