Detectability Scaling Laws for Environmental Phase Modulation in Gravitational-Wave Signals
Jericho Cain

TL;DR
This paper investigates how environmental phase modulations in gravitational-wave signals can be detected without templates, revealing a simple scaling law between phase distortion and SNR that determines detectability.
Contribution
It introduces a template-free method to quantify the detectability of environmental phase modulations in gravitational waves, establishing a universal scaling law for detection performance.
Findings
Detection depends on the product of phase distortion and SNR
Detection performance follows a sigmoid function of the scaling parameter
Moderate distortions are detectable at low SNR, smaller ones need higher SNR
Abstract
Environmental effects such as hierarchical triple motion can introduce cumulative phase modulation in gravitational-wave signals through time-dependent line-of-sight acceleration. Whether such smooth time-warp distortions are observable depends jointly on deformation strength and signal-to-noise ratio (SNR), yet this relationship has not been quantified in a template-free framework. We study the detectability of these distortions using time-frequency representations derived from the continuous wavelet transform. Instead of reconstruction error alone, we analyze trajectory-level statistics, in particular the evolution of the power-weighted frequency centroid. We find that environmental modulation can be detected using a single-sample statistic referenced to an isolated-binary distribution, without requiring matched templates. Across a grid of cumulative phase distortions and SNR,…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Advanced Frequency and Time Standards · Geophysics and Sensor Technology
