The paper argues that black hole interiors, Rindler horizons, and de Sitter horizons all emerge from coarse-graining soft modes of low-energy fields, selected by the Born rule.
The Black Hole Interior in Quantum Gravity
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abstract
We discuss the interior of a black hole in quantum gravity, in which black holes form and evaporate unitarily. The interior spacetime appears in the sense of complementarity because of special features revealed by the microscopic degrees of freedom when viewed from a semiclassical standpoint. The relation between quantum mechanics and the equivalence principle is subtle, but they are still consistent.
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Spacetime and Universal Soft Modes --- Black Holes and Beyond
The paper argues that black hole interiors, Rindler horizons, and de Sitter horizons all emerge from coarse-graining soft modes of low-energy fields, selected by the Born rule.