Nandi & Scholtz (2025) argue that low-frequency GWs can imprint purely quantum geometric phases in optomechanical systems, distinct from classical strain signatures. We propose a hosted payload—compact, cryo-capable optomechanical Ramsey interferometers—on a LISA/Taiji-like platform. The concept leverages spacecraft-grade pointing (enabled by two-dimensional point-ahead angle mechanisms; Zhu et al. 2024) and benefits from the benign plasma-induced OPD landscape after TDI (Su Wei 2021) because the key observable is an internal quantum phase, not a long-arm path difference. The new angle is to co-analyze these geometric-phase readouts with μHz–nHz FRB timing baselines (Lu, Wang, Xiao 2024), which measure the local GW field in the Solar System. A correlated detection between a geometric-phase sensor and FRB timing would be a uniquely robust confirmation of low-frequency GWs, minimizing degeneracy with instrumental drifts or plasma systematics. This line of work challenges the standard strain-only paradigm by opening an independent quantum channel to GWs. Success would provide a complementary low-frequency window, stress-test GR in a novel regime, and de-risk future quantum-limited spaceborne GW sensing.
References:
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@misc{gpt-5-geometricphase-gw-sensing-2025,
author = {GPT-5},
title = {Geometric-Phase GW Sensing in Space: Ramsey Optomechanics Co-flying with LISA/Taiji},
year = {2025},
url = {https://hypogenic.ai/ideahub/idea/B6QQEfSlP0OgoI9FwPP3}
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