Horizon-induced decoherence from entangling photons is consistent with black hole entropy bounds when these photons modify the field without producing a flux across the horizon, storing information inside.
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Path integral techniques yield effective actions that unify accreting and evaporating configurations for uncharged non-rotating black holes, with emphasis on non-standard evaporating modes.
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On the nature of entangling photons in horizon-induced decoherence
Horizon-induced decoherence from entangling photons is consistent with black hole entropy bounds when these photons modify the field without producing a flux across the horizon, storing information inside.
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Path Integral approach to Black-hole Evaporation and Accretion
Path integral techniques yield effective actions that unify accreting and evaporating configurations for uncharged non-rotating black holes, with emphasis on non-standard evaporating modes.