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.
For the Hamiltonian given by (14), it is given by B= 0 0 1 0 0 0 0 1 with correlatorC(τ) = CA(τ) 0 0C B(τ) ! (C16) 27 a
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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.