Probing non-Riemannian spacetime geometry
Dirk Puetzfeld, Yuri N. Obukhov

TL;DR
This paper derives matter equations of motion in non-Riemannian spacetimes, showing only microstructured test bodies couple to torsion, and concludes that satellite experiments like Gravity Probe B cannot detect spacetime torsion.
Contribution
It provides a derivation of matter motion equations in non-Riemannian geometry and clarifies the detectability of torsion with satellite experiments.
Findings
Test bodies with microstructure couple to non-Riemannian geometry.
Gravity Probe B cannot detect spacetime torsion.
Spacetime torsion remains undetectable with certain satellite experiments.
Abstract
The equations of motion for matter in non-Riemannian spacetimes are derived via a multipole method. It is found that only test bodies with microstructure couple to the non-Riemannian spacetime geometry. Consequently it is impossible to detect spacetime torsion with the satellite experiment Gravity Probe B, contrary to some recent claims in the literature.
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