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| Main Authors: | , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2509.13321 |
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Table of Contents:
- The experimental possibility of detecting gravitational waves via their induced time perturbations is explored here, expanding from previous work. The oscillations of the time-time component in the metric are made explicit when working in asynchronous gauges: the desynchronization between a perturbed clock and a reference unperturbed clock constitutes the corresponding observable core target of a detector. To this end we explore the experimental techniques currently available for a preliminary assessment towards a feasibility study. We survey the state of the art in the fields of high precision timing and information preservation, necessary for achieving geodesic non-locality. A synthesis for a feasible prototype detector with the desired characteristics is presented. The optimum point between existing technologies is found around the 1 Hz frequency band, opening the window for the observation of classes of speculated sources of gravitational radiation such as intermediate mass black hole binaries.