Experimental Status of Gravitational-Strength Forces in the Sub-Centimeter Regime
Joshua C. Long, Hilton W. Chan, John C. Price
TL;DR
This paper surveys experimental constraints on gravitational-strength Yukawa forces at sub-centimeter scales, using a Yukawa-modified potential $V(r) = - G \frac{m_1 m_2}{r} [1 + \alpha e^{-r/\lambda}]$ to map excluded regions in the $\alpha$–$\lambda$ parameter space. It synthesizes limits from classical torsion-balance tests and Casimir-force measurements, and outlines a theoretical landscape where light bosons, moduli, dilatons, axions, and large extra dimensions predict sizable forces at μm–mm ranges. It then proposes a high-frequency (≈1 kHz) mechanical-oscillator experiment with coordinated source and detector masses, deriving explicit expressions for the expected Yukawa torque and the thermal-noise-limited sensitivity, projecting reach down to around $\lambda \approx 50\ \mu\mathrm{m}$ and spanning roughly 10 decades in parameter space. The work underscores the continued motivation to probe sub-centimeter gravity with macroscopic devices, given compelling predictions from string-inspired theories and extra-dimensional scenarios, and highlights the potential for substantial improvements over existing limits.
Abstract
We review the experimental constraints on additional macroscopic Yukawa forces for interaction ranges below 1 cm., and summarize several theoretical predictions of new forces in this region. An experiment using 1 kHz mechanical oscillators as test masses should be sensitive to much of the parameter space covered by the predictions.
