This conceptual theory paper proposes a flux-calibrated framework for testing whether mechanical rotation and optical orbital angular momentum can bias state selection in pressure-induced superconducting bismuth during the formation of the condensate. The proposed coaxial architecture combines a pressure-tuned bismuth annulus, a multilayer-graphene OAM detector, engineered radial-to-circumferential current routing, measured axial magnetic flux, torsional motion, cryogenic cooling, and independently calibrated rotational and optical bias channels. The central experimental question is whether the measured graphene-generated flux, ΦGGΦG, and the calibrated rotational bias, Φrotₑ₎ₓΦrot, add or oppose in a way that changes the probability, sign, or distribution of superconducting winding, persistent-current, trapped-flux, or vortex states. The paper separates the demonstrated graphene response from the unproven routing step. Optical OAM and polarization helicity generate a measured radial orbital-photogalvanic response, which must then be deliberately converted into a circumferential current and axial flux. Each stage is treated as independently measurable and falsifiable. The framework also defines timing windows, electrical mimic tests, symmetry requirements, defect and pinning controls, staged experimental validation, and explicit failure conditions. The work does not claim that rotation or structured light creates superconductivity. Pressure and cryogenic temperature establish the superconducting phase. The proposal is that small directional biases may influence which state forms while the condensate is still selecting among nearly degenerate outcomes. Developed through a symbiotic intelligence process between Chris Gabriel and GPT-5. 6 Thinking. Released under CC BY 4. 0.
Gabriel et al. (Fri,) studied this question.