Tidal Accelerometry: Exploring the Cosmos Via Gravitational Correlations
Timir Datta, Ming Yin, Mike Wescott, Yeuncheol Jeong, Pawel Morawiec,, James Gambrell, Dan Overcash, Huaizhou Zhang, George Voulgaris

TL;DR
This paper discusses how tidal accelerometry, which measures gravitational correlations through low-frequency signals, can be used for high-precision cosmic observations and mass determinations.
Contribution
It introduces the concept of tidal signals as a tool for calibrating experiments and exploring celestial mass distributions independently of traditional methods.
Findings
Tidal signals can be observed in natural and laboratory settings.
High-precision accelerometry can determine solar system masses.
Potential to detect supermassive black holes using tidal accelerometry.
Abstract
Newtonian gravitation is non-radiative but is extremely pervasive and penetrates equally into every media because it cannot be shielded. The extra terrestrial fgravity is responsible for earth's trajectory. However its correlation or geodesic deviation is manifested as semi-diurnal and diurnal tides. Tidal signals, A(t) are temporal modulations in the field differential which can be observed in a wide variety of natural and laboratory situations. A(t) is a quasi-static, low frequency signal which arises from the relative changes in positions of the detector and source and is not part of the electromagnetic spectrum. Isaac Newton was the first to recognize the importance of tides in astrometry and attempetd to estimate lunar mass from ocean tides. By a case study we show, how the systematics of the gravitational correlation can be used for calibration and de-trending which can…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Pulsars and Gravitational Waves Research · Scientific Research and Discoveries
