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This is equivalent to adding the term−βg µν to the deWitt metric, setting all scalar potentials apart fromψ, ϕto zero

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hep-th 1

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2026 1

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UNVERDICTED 1

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Stochastic modes in postquantum classical gravity

hep-th · 2026-05-06 · 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.

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  • Stochastic modes in postquantum classical gravity hep-th · 2026-05-06 · unverdicted · none · ref 63

    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.