On the first test of the Weak Equivalence Principle in low Earth orbit
Anna M. Nobili, Alberto Anselmi

TL;DR
The Microscope experiment in low Earth orbit tested the Weak Equivalence Principle with unprecedented precision, revealing thermal noise effects and data handling challenges that impact the interpretation of its results.
Contribution
This work critically assesses the Microscope experiment's results, focusing on thermal noise, acceleration spikes, and data processing methods, providing insights for future tests.
Findings
Tested WEP to 1e-15 accuracy in orbit
Identified thermal noise and stray potentials affecting measurements
Highlighted data processing issues with artificial gap filling
Abstract
The Weak Equivalence Principle is the founding pillar of General Relativity and as such it should be verified as precisely as possible. The Microscope experiment tested it in low Earth orbit, finding that Pt and Ti test masses fall toward Earth with the same acceleration to about 1e-15, an improvement of about two orders of magnitude over ground tests. Space missions, even if small, are expensive and hard to replicate; yet, the essence of physics is repeatability. This work is an assessment of the Microscope results based on the laws of physics and knowledge from previous experiments, focusing on the limiting thermal noise and the treatment of acceleration outliers. Thermal noise reveals anomalies that we explain by stray sub-microVolt potentials caused by patch charges, giving rise to an unstable zero. The measurements were affected by numerous acceleration spikes occurring at the…
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Taxonomy
TopicsRadioactive Decay and Measurement Techniques
