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Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms

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arxiv 2502.11823 v2 pith:YTYOAG4S submitted 2025-02-17 gr-qc astro-ph.HEastro-ph.IMphysics.data-an

classification gr-qcastro-ph.HEastro-ph.IMphysics.data-an
keywords gravitationalwavesftsbinariesdataframeworkinnerproduct
verification ladder T0 review T1 audit T2 compute T3 formal
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We introduce a framework based on short Fourier transforms (SFTs) to analyze long-duration gravitational wave signals from compact binaries. Targeted systems include binary neutron stars observed by third-generation ground-based detectors and massive black hole binaries observed by the LISA space mission. In short, ours is an extremely fast, scalable, and parallelizable implementation of the gravitational wave inner product, a core operation of gravitational wave matched filtering. By operating on disjoint data segments, SFTs allow for efficient handling of noise nonstationarities, data gaps, and detector-induced signal modulations. We present a pilot application to early warning problems in both ground- and space-based next-generation detectors. Overall, SFTs reduce the computing cost of evaluating an inner product by three to five orders of magnitude, depending on the specific application, with respect to a nonoptimized approach. We release public tools to operate using the SFT framework, including a vectorized and hardware-accelerated reimplementation of a time-domain waveform. The inner product is the key building block of all gravitational wave data treatments; by speeding up this low-level element so massively, SFTs provide an extremely promising solution for current and future gravitational wave data-analysis problems.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Non-stationary noise in gravitational wave analyses: The wavelet domain noise covariance matrix

    gr-qc 2025-11 conditional novelty 7.0 of 10

    For slowly varying detector noise, the Wilson-Daubechies-Meyer wavelet noise covariance matrix is approximately diagonal, with off-diagonal terms controlled by the time and frequency derivatives of the dynamic spectral model.

  2. Enhancing Taiji's Parameter Estimation under Non-Stationarity: a Time-Frequency Domain Framework for Galactic Binaries and Instrumental Noises

    gr-qc 2025-06 conditional novelty 7.0 of 10

    A time-frequency (STFT) Bayesian framework improves Taiji Galactic binary and noise parameter estimation under non-stationary noise compared with frequency-domain analysis.

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