# Measurement of the Newtonian Constant of Gravitation $G$ by Precision   Displacement Sensors

**Authors:** Akio Kawasaki

arXiv: 1903.11223 · 2020-03-02

## TL;DR

This paper proposes a novel method to measure the gravitational constant G using precision displacement sensors, leveraging existing technologies like gravitational wave detectors and optically-levitated microspheres to improve accuracy and explore non-Newtonian gravity.

## Contribution

It introduces a new measurement scheme for G utilizing displacement sensors, analyzing setups with gravitational wave detectors and microspheres for enhanced precision.

## Key findings

- High sensitivity of gravitational wave detectors enables high signal-to-noise ratio in G measurement.
- Optically-levitated microspheres offer a compact, tunable alternative for G measurement.
- Developments in force calibration are crucial for achieving better accuracy than current methods.

## Abstract

The Newtonian constant of gravitation $G$ historically has the largest relative uncertainty over all other fundamental constants with some discrepancies in values between different measurements. We propose a new scheme to measure $G$ by detecting the position of a test mass in a precision displacement sensor induced by a force modulation from periodically rotating source masses. To seek different kinds of experimental setups, laser interferometers for the gravitational wave detection and optically-levitated microspheres are analyzed. The high sensitivity of the gravitational wave detectors to the displacement is advantageous to have a high signal-to-noise ratio of $10^{-6}$ with a few hours of the measurement time, whereas the tunability of parameters in optically-levitated microspheres can enable competitive measurements with a smaller scale setup dedicated to the $G$ measurement. To achieve an accuracy of $G$ better than currently available measurements, developments in force calibration is essential. These measurements can provide an alternative method to measure $G$ precisely, potentially leading to the improvement in the accuracy of $G$, as well as a better search for non-Newtonian gravity at a length scale of $\sim1$ m.

## Full text

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## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1903.11223/full.md

## References

48 references — full list in the complete paper: https://tomesphere.com/paper/1903.11223/full.md

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Source: https://tomesphere.com/paper/1903.11223