Detecting gravitational wave signals using a flexible model for the
amplitude and frequency evolution
Detecting gravitational wave signals using a flexible model for the
amplitude and frequency evolution
We currently lack good waveform models for many gravitational wave sources. Examples where models are lacking include neutron star post merger signals, core collapse supernovae, and signals of unknown origin. Wavelet based techniques have proven effective at detecting and characterizing these signals. Here we introduce a new method that uses …