Time Dispersion and Efficiency of Detection for Signals in Gravitational Wave Experiments
P.Astone, S.D'Antonio, G. Pizzella
TL;DR
This paper evaluates the detection efficiency and timing accuracy of gravitational wave signals using simulated data and real noise measurements from the EXPLORER and NAUTILUS detectors.
Contribution
It provides new insights into how detection efficiency and signal timing dispersion depend on the signal-to-noise ratio in gravitational wave experiments.
Findings
Detection efficiency increases with higher SNR.
Signal arrival time dispersion varies with noise conditions.
Results inform optimization of gravitational wave detection strategies.
Abstract
Using simulated signals and measured noise with the EXPLORER and NAUTILUS detectors we find the efficiency of signal detection and the signal arrival time dispersion versus the signal-to-noise ratio.
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