AbstractThis work details an experimental protocol for the direct observation of quantumgravitational radiation (graviton emission). The experiment is based on the ”graz-ing” interaction between ultra-relativistic hadron beams and an array of levitatednanodiamonds. By integrating the spin-detection technique of Hoang et al. (2016)with the fundamentals of gravity-mediated entanglement (Bose, 2017; Marletto,2017), we propose a protocol that isolates the quadrupolar (spin-2) signature ofgravity from electromagnetic dipolar (spin-1) noise. The success of this experimentwould provide the first direct evidence of the corpuscular nature of gravity throughdetection windows synchronized with high-energy accelerator infrastructure.We pro-vide estimates for the event rate (∼1-5 Hz) and a hybrid shielding strategy to ensurefeasibility within high-energy accelerator environments.
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Lucas Campos Achcar
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Lucas Campos Achcar (Thu,) studied this question.
synapsesocial.com/papers/69e321aa40886becb6540c0d — DOI: https://doi.org/10.5281/zenodo.19610002