Gravitational-wave matched filtering on a quantum computer
Doğa Veske, Cenk Tüysüz, Mirko Amico, Nicholas T. Bronn, Olivia T. Lanes, Imre Bartos, Zsuzsa Márka, Sebastian Will, Szabolcs Márka
TL;DR
This work demonstrates the first qubit-based matched filtering for gravitational-wave detection using a hybrid quantum-classical Monte Carlo algorithm that encodes data and templates via amplitude encoding and employs a divide-and-conquer encoding to enable a time-domain convolution with complexity around $O\big(L(\log N)^2\big)$. Implemented on noisy superconducting qubits through IBM Quantum hardware, the method achieves SNR results for GW190521 comparable to classical FFT-based approaches, validating the practicality of quantum-augmented signal processing with shallow circuits. While no asymptotic quantum advantage is yet observed over FFT, the study shows robust performance under current hardware and outlines pathways for energy-efficient scaling and application to higher-dimensional or multi-input problems as quantum hardware improves.
Abstract
State of the art quantum computers have very limited applicability for accurate calculations. Here we report the first experimental demonstration of qubit-based matched filtering for a detection of the gravitational-wave signal from a binary black hole merger. With our implementation on noisy superconducting qubits, we obtained a similar signal-to-noise ratio for the binary black hole merger as achievable with classical computation, providing evidence for the utility of qubits for practically relevant tasks. The algorithm we invented for this application is a Monte Carlo algorithm which uses quantum and classical computation together. It provides a quasi-quadartic speed-up for time-domain convolution, similar to achievable with fast Fourier transform.
