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A Nonperturbative Toolkit for Quantum Gravity

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arxiv 2504.16986 v4 pith:25SXUVMP submitted 2025-04-23 hep-th gr-qc

classification hep-thgr-qc
keywords gravityquantumbasisgeometriesmethodovercompletepathapproximation
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We propose a method for demonstrating equivalences beyond the saddlepoint approximation between quantities in quantum gravity that are defined by the Euclidean path integral, without assumptions about holographic duality. The method involves three ingredients: (1) a way of resolving the identity with an overcomplete basis of microstates that is under semiclassical control, (2) a drastic simplification of the sum over topologies in the limit where the basis is infinitely overcomplete, and (3) a way of cutting and splicing geometries to demonstrate equality between two different gravitational path integrals even if neither can be explicitly computed. We illustrate our methods by giving a general argument that the thermal partition function of quantum gravity with two boundaries factorises. One implication of our results is that universes containing a horizon can sometimes be understood as superpositions of horizonless geometries entangled with a closed universe.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. How to Count States in Gravity

    hep-th 2025-06 conditional novelty 6.0 of 10

    The Gibbons-Hawking Euclidean gravity path integral with periodic time equals an explicit thermal trace over the single-boundary quantum gravity Hilbert space.

  2. Nonperturbative Quantum Gravity in a Closed Lorentzian Universe

    hep-th 2025-05 conditional novelty 6.0 of 10

    In a closed universe with a one-dimensional Hilbert space per alpha-microstate, tracing out unobserved environmental degrees of freedom yields robust, einselected probabilities with errors exponentially suppressed by ...

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