Detectability of post-Newtonian classical and quantum gravity via quantum clock interferometry
Eyuri Wakakuwa
TL;DR
This work tackles the challenge of probing quantum gravity effects in the post Newtonian regime by proposing two quantum clock based schemes that isolate frame-dragging signatures in a symmetric geometry. It develops a consistent canonical path integral framework for quantum clocks in nonstatic spacetimes, derives the gravitomagnetic proper-time difference, and analyzes both a clock interferometry visibility test and a gravity induced entanglement (GIE) test. The paper also extends the quantum equivalence principle to nonstatic and quantum superposed geometries, showing how the proposed experiments could distinguish competing quantum gravity models, though the predicted effects are currently extremely small. Together these results establish a rigorous theoretical foundation and a clear path for future experiments to explore post-Newtonian quantum gravitational phenomena.
Abstract
Understanding physical phenomena at the intersection of quantum mechanics and general relativity remains a major challenge in modern physics. While various experimental approaches have been proposed to probe quantum systems in curved spacetime, most focus on the Newtonian regime, leaving post-Newtonian effects such as frame dragging largely unexplored. In this study, we propose and theoretically analyze an experimental scheme to investigate how post-Newtonian gravity affects quantum systems. We consider two setups: (i) a quantum clock interferometry setup designed to detect the gravitational field of a rotating mass, and (ii) a scheme exploring whether such effects could be used to generate gravity-induced entanglement. Due to the symmetry of the configuration, the proposed setup is insensitive to Newtonian gravitational contributions but remains sensitive to the frame-dragging effect. Furthermore, our scheme allows for testing whether the observed gravity-induced entanglement is consistent with the quantum equivalence principle. While the predicted effects appear too small to detect with current technology, our scheme offers a starting point for future experiments probing post-Newtonian quantum gravitational effects.
