| Literature DB >> 27081964 |
Wen-Hai Tan1, Shan-Qing Yang1, Cheng-Gang Shao1, Jia Li1, An-Bin Du1, Bi-Fu Zhan2, Qing-Lan Wang3, Peng-Shun Luo1, Liang-Cheng Tu1, Jun Luo1,4.
Abstract
By using a torsion pendulum and a rotating eightfold symmetric attractor with dual modulation of both the interested signal and the gravitational calibration signal, a new test of the gravitational inverse-square law at separations down to 295 μm is presented. A dual-compensation design by adding masses on both the pendulum and the attractor was adopted to realize a null experiment. The experimental result shows that, at a 95% confidence level, the gravitational inverse-square law holds (|α|≤1) down to a length scale λ=59 μm. This work establishes the strongest bound on the magnitude α of Yukawa-type deviations from Newtonian gravity in the range of 70-300 μm, and improves the previous bounds by up to a factor of 2 at the length scale λ≈160 μm.Year: 2016 PMID: 27081964 DOI: 10.1103/PhysRevLett.116.131101
Source DB: PubMed Journal: Phys Rev Lett ISSN: 0031-9007 Impact factor: 9.161