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The Black Hole Interior in Quantum Gravity

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arxiv 1412.7539 v2 pith:5Y7GG242 submitted 2014-12-23 hep-th gr-qc

Yasunori Nomura , Fabio Sanches , Sean J. Weinberg This is my paper · ORCID
classification hep-thgr-qc
keywords blackinteriorquantumgravityholeappearsbecausecomplementarity
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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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  1. Spacetime and Universal Soft Modes --- Black Holes and Beyond

    hep-th 2019-08 conditional novelty 5.0 of 10

    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.

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