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We develop a new test that provides a necessary condition for a quantum state to be smooth in the vicinity of a null surface: near-horizon modes that can be defined locally near any patch of the null surface must be correctly entangled with each other and with their counterparts across the surface.
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1999
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E. Keski-Vakkuri, Bulk and boundary dynamics in BTZ black holes , Phys. Rev. D59
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2016
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M. Dafermos and Y. Shlapentokh-Rothman, Rough initial data and the strength of the blue-shift instability on cosmological black holes with λ \lambda ¿ 0 , Classical and Quantum Gravity 35
2018
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2018
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2018
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2018
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2018
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2018
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O. Sela, Quantum effects near the Cauchy horizon of a Reissner-Nordström black hole , Phys. Rev. D98
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2019
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2019
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