A Joint-Chirp-Rate-Time-Frequency Transform for BBH Merger Gravitational Wave Signal Detection
Xiyuan Li, Martin Houde, Jignesh Mohanty, S. R. Valluri

TL;DR
This paper introduces the JCTFT, a novel time-frequency transform that enhances detection of BBH merger gravitational waves by better capturing rapid frequency changes amidst noise, improving detection accuracy.
Contribution
The paper presents the JCTFT, a new transform that improves gravitational wave signal detection by incorporating chirp-rate information into spectrograms, outperforming traditional methods.
Findings
Average 14% improvement in merger detectability with JCTFT
Effective in noisy environments with SNR between 6 and 10
Applicable to current and future gravitational wave detectors
Abstract
Low-latency detection of Binary Black Hole (BBH) and Binary Neutron Star (BNS) merger Gravitational Wave (GW) signals is essential for enabling multi-messenger observations of such systems. The merger GW signals have varying frequencies and are contaminated by non-stationary noises. Earlier studies of non-templated merger signal detection techniques used traditional Fourier transform-based time-frequency decomposition methods for spectrogram generation, which have had difficulties identifying rapid frequency changes in merger signals with heavy background noise. To address this problem, we introduce the Joint-Chirp-rate-Time-Frequency Transform (JCTFT), in which complex-valued window functions are used to modulate the amplitude, frequency, and phase of the input signal. In addition, we outline the techniques for generating chirp-rate-enhanced time-frequency spectrograms from the results…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Seismic Imaging and Inversion Techniques
