Quasilocal probability flux at black hole horizons produces non-Hermitian ringdown dynamics yielding correlated multi-mode deviations, weak amplitude dependence, and damping-energy mismatch as a low-dimensional discriminator from modified gravity.
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Gravity renders probability quasilocal in quantum theory on curved backgrounds by converting global unitarity into local flux balance laws at boundaries while preserving overall conservation.
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Smoking Gun Signatures of Quasilocal Probability in Black Hole Ringdowns
Quasilocal probability flux at black hole horizons produces non-Hermitian ringdown dynamics yielding correlated multi-mode deviations, weak amplitude dependence, and damping-energy mismatch as a low-dimensional discriminator from modified gravity.
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Does Gravity Render Probability Quasilocal?
Gravity renders probability quasilocal in quantum theory on curved backgrounds by converting global unitarity into local flux balance laws at boundaries while preserving overall conservation.