When two black holes merge, a tremor ripples through the universe — a gravitational wave. Detectors on Earth catch this tremor, but to understand which black holes collided, the signal must be compared with thousands of templates. It's like searching for a specific melody in a huge music library by playing every record. Each year, more signals arrive, and old methods can't keep up.
The neural network from this work acts like a simultaneous interpreter: first it quickly conveys the gist, then it refines the details. The first part of the network compresses data about the masses and spins of the black holes into a short code and draws the wave from it. The second part corrects errors, especially at the moment of merger — the trickiest part. As a result, the waveform comes out nearly right: the error is less than one hundredth.
Previously, it was unclear whether such fast models could be trusted. Now it's clear: they can, if you know where they go wrong. This will speed up processing of future observations and help find interesting events faster.
The dynamic lower cutoff frequency varies from 11 to 60 Hz: light systems with low chirp mass live longer in the detector, so to fit the signal into one second, low frequencies must be cut off.