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Distinguishable consequence of classical gravity on quantum matter

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arxiv 2309.09105 v2 pith:R34XDT3T submitted 2023-09-16 gr-qc hep-thquant-ph

Distinguishable consequence of classical gravity on quantum matter

classification gr-qc hep-thquant-ph
keywords gravityclassicalquantummatterconsistentfluctuationsgravitationallymotion
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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What if gravity is classical? If true, a consistent co-existence of classical gravity and quantum matter requires that gravity exhibit irreducible fluctuations. These fluctuations can mediate classical correlations, but not quantum entanglement, between the quantized motion of the gravitationally interacting matter. We use a consistent theory of quantum-classical dynamics in the Newtonian limit of gravity to show that experimentally relevant observables can conclusively test the hypothesis that gravity is classical. This can be done for example by letting highly coherent source masses interact with each other gravitationally, and performing precise measurements of the cross-correlation of their motion. Theory predicts a characteristic phase response that distinguishes classical gravity from quantum gravity, and from naive sources of decoherence. Such experiments are imminently viable.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Minimal noise in non-quantized gravity

    quant-ph 2026-03 unverdicted novelty 7.0

    Non-quantized gravity models that preserve Galilean invariance and reproduce Newtonian interaction on average require a minimal noise injection to remain non-entangling.

  2. Stochastic modes in postquantum classical gravity

    hep-th 2026-05 unverdicted novelty 5.0

    Postquantum classical gravity requires stochastic spacetime fluctuations consisting of a diffusing spin-2 field and spin-0 scalar whose noise is constrained by LISA Pathfinder and decoherence bounds.