Residual particle-shield interactions and thermal vibrations impose strict positional and orientational fluctuation thresholds for observing genuine gravitationally induced entanglement, with magnetic effects dominant in superconducting setups.
If a fractionκ∈[0,1] of the electromagnetic modes can leak around the edges of the shield and re-establish a direct non-gravitational coupling
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Stability Thresholds for Gravitationally Induced Entanglement in Shielded Setups
Residual particle-shield interactions and thermal vibrations impose strict positional and orientational fluctuation thresholds for observing genuine gravitationally induced entanglement, with magnetic effects dominant in superconducting setups.