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.
(B1) withθ A =θ B ≡θ: ˆHGravity ≈λ sin2 θ− 1 2 cos2 θ ˆxAˆxB + cos2 θ− 1 2 sin2 θ ˆyAˆyB − 3 2 cosθsinθ (ˆxAˆyB + ˆxB ˆyA)
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
quant-ph 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.