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The Quantum Gravity Dynamics of Near Extremal Black Holes

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arxiv 1809.08647 v3 pith:4CZLVVQA submitted 2018-09-23 hep-th gr-qc

classification hep-thgr-qc
keywords quantumgravityblackdynamicsholesnearwavefunctionbackgrounds
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We study the quantum effects of Near-Extremal black holes near their horizons. The gravitational dynamics in such backgrounds are closely connected to a particle in $AdS_2$ with constant electric field. We use this picture to solve the theory exactly. We will give a formula to calculate all correlation functions with quantum gravity backreactions as well as the exact Wheeler-DeWitt wavefunction. Using the WdW wavefunction, we investigate the complexity growth in quantum gravity.

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Forward citations

Cited by 8 Pith papers

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

  1. JT gravity on the worldline

    hep-th 2026-07 conditional novelty 7.0 of 10

    Coupling a worldline observer to JT gravity replaces its evolution operator by an exactly computed average over fluctuating Euclidean times; the fluctuations are small in the disk but large on the double trumpet.

  2. Exact Schwarzian Metric Factor and Holographic Wilson-Loop Screening

    hep-th 2026-07 accept novelty 7.0 of 10

    Exact Schwarzian averaging yields a completely monotone metric factor with no confining minimum, so the Wilson-loop potential screens as E(L) ~ -κ_IR/L² rather than confining.

  3. Evaporating Black Hole Interior and Complexity Evolution

    hep-th 2026-05 unverdicted novelty 7.0 of 10

    In JT gravity with an end-of-the-world brane, the renormalized interior length — read as subsystem complexity — grows linearly, peaks around the Page time, and then decays exponentially, with growing relative fluctuat...

  4. York time in JT gravity

    hep-th 2025-05 conditional novelty 7.0 of 10

    In JT gravity, the Hartle-Hawking wavefunction satisfies a Schrodinger equation in York time with a Hermitian squeezing Hamiltonian, and York time evolution is a unitary change of the length basis rather than physical...

  5. Falling through the horizon of a quantum black hole

    hep-th 2026-07 conditional novelty 6.5 of 10

    Gravitational dressing in JT gravity lets an infalling Unruh-DeWitt detector detect the horizon location and temperature locally, violating the equivalence principle without a firewall.

  6. Quantum gravity around ultracold black holes from DSSYK

    hep-th 2026-08 conditional novelty 6.0 of 10

    Ultracold Reissner-Nordström de Sitter black hole fluctuations are proposed to be described by a gauged near-flat dilaton gravity model with a Gaussian spectral density, yielding a finite partition function and dynami...

  7. Classical Unattainability of Extremality in non-BPS D-brane Systems

    hep-th 2026-01 conditional novelty 6.0 of 10

    For a non-BPS four-charge D-brane system in N=8 string theory, the worldline potential has no classical zero-energy minimum, so extremality is unattainable; entropy is proposed as the logarithm of the number of isolat...

  8. JT gravity and deformed CFTs

    hep-th 2025-07 conditional novelty 5.0 of 10

    Deformed CFTs on a strip with a stretched-horizon conformal boundary are proposed as UV completions of pure and matter-coupled JT gravity, reproducing its entropy and a Page-curve-like saturation.

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