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Solvable Models of Quantum Black Holes: A Review on Jackiw-Teitelboim Gravity
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We review recent developments in Jackiw-Teitelboim (JT) gravity. This is a simple solvable model of quantum gravity in two dimensions (that arises e.g. from the s-wave sector of higher dimensional gravity systems with spherical symmetry). Due to its solvability, it has proven to be a fruitful toy model to analyze important questions such as the relation between black holes and chaos, the role of wormholes in black hole physics and holography, and the way in which information that falls into a black hole can be recovered.
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Cited by 39 Pith papers
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The evaporation of black holes in supergravity
Near-BPS black holes in N=2 supergravity emit a discrete spectral line when transitioning to BPS states, and their radiation and absorption spectra deviate strongly from semiclassical black-body predictions.
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Exact Schwarzian Metric Factor and Holographic Wilson-Loop Screening
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.
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Wormholes and the imaginary distance bound
Wormhole solutions with imaginary scalars set an Imaginary Distance Bound on analytic continuation of couplings, enforced by stringy effects that coincide with WGC and KSW in special cases.
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Entanglement Revivals and Scrambling for Evaporating Black Holes
Increasing black hole scrambling time in JT and RST evaporating geometries suppresses and eliminates late-time entanglement revivals in 2d CFT mutual information for disjoint intervals, interpolating between quasipart...
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Quantum Fluctuations and Newton-Cartan Geometry for Non-Relativistic de Sitter space
The one-loop partition function of the Galilean-de Sitter boundary theory is Z(β) = (2/πβ²) exp(4π²c₀/β), whose β⁻² prefactor matches the four generators of the EdS-G algebra; the matching bulk is a Newton-Cartan geom...
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Schwarzian quantum corrections to shear correlators of the near-extremal Reissner-Nordstr\"om-AdS black hole
Schwarzian quantum fluctuations raise the shear viscosity of near-extremal Reissner-Nordström-AdS4 black holes above s/4π by a positive O(1/(CT)^2) correction and are argued to lift the classical T=0 gapless shear mode.
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The Effects of Near-AdS$_2$ Backreaction on Matter Fields
Backreaction of near-AdS2 geometry gives a temperature correction to scalar correlators that for massive fields needs metric backreaction, matches BTZ, and corrects the standard prescription.
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Towards the super Virasoro minimal string
The authors derive the timelike super Liouville structure constants from crossing symmetry and construct a tentative Type 0A/0B super Virasoro minimal string whose sphere three-point functions vanish only after sign c...
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de Sitter JT gravity from double-scaled SYK
The upper edge of the DSSYK spectrum, in a triple scaling limit, exactly reproduces the matrix model of two-dimensional de Sitter JT gravity.
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Accidental Symmetry Near Extreme Spinning Black Holes
A new accidental symmetry of the NHEK near-horizon geometry maps extreme to near-extreme Kerr perturbations and embeds with SL(2,R) into a Virasoro algebra.
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Twisted times, the Schwarzian and its deformations in DSSYK
The soft modes of double-scaled SYK are reparametrizations of twisted time coordinates; their effective action is the nonlinear Schwarzian, and deformations yield multi-field Liouville theories with computable low-ene...
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Angle of Null Energy Condition Lines in Critical Spacetimes
In Choptuik critical collapse, the null energy condition saturation lines meet at the center with a universal angle α=2 arccot(D−1), numerically α≈0.64 in four dimensions.
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Chaos and the Emergence of the Cosmological Horizon
Finite-mass observers in dS2 have non-commuting type I algebras, and their OTOC shows a Lyapunov exponent 4π/β_dS, twice the de Sitter bound.
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Quantum corrections to the near-extremal thermodynamics of (warped) BTZ black holes
Near-extremal BTZ and warped BTZ in TMG receive log-T corrections from Schwarzian and rotational zero modes whose full-geometry eigenvalues match the throat after non-normalizable eigenfunction corrections and BC spec...
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Falling through the horizon of a quantum black hole
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.
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The quadratic growth of Krylov spread complexity in the BTZ black hole
Krylov spread complexity of the BTZ thermofield-double state departs from pure quadratic growth at intermediate times and appears to return to quadratic pre-saturation growth, with a bulk dual constructed from an infi...
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Three-loop onset of the wormhole length in DSSYK
The wormhole-length onset L0 in DSSYK is derived in closed form through three loops, with new two- and three-loop coefficients from a new exact recursion.
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Quantum gravity around ultracold black holes from DSSYK
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...
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Flavour current correlators and the non-Abelian hydrodynamic approximation: the charged sector
Isospin-imbalanced strongly coupled dense matter is shown, via holography, to obey non-Abelian hydrodynamic predictions for current correlators up to the chemical-potential scale, beyond the standard ω,k ≪ T regime.
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On conformal symmetry in large-$N$ quiver mechanics
At large rank N, the fixed-point formula for the quiver superconformal index equals the Ω_uneq contribution to the microscopic scaling BPS index of Beaujard–Mondal–Pioline, a piece previously invisible on the Coulomb branch.
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Kink collisions in a two-dimensional gravity model
In a 2D dilaton-gravity model, stronger gravity shifts kink-antikink bounce windows to higher speeds and narrows them, leaves a lasting contraction of the conformal scale, and produces no curvature singularity in the ...
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Resolving Black Hole Singularities in Jackiw-Teitelboim Gravity
In JT gravity, the left confining potential required by spectral discreteness makes the wormhole length turn around and plateau, allowing boundary time to run past the would-be singularity and eliminating future horizons.
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Approaching a dynamical extreme black hole horizon
Explicit JT-gravity solutions give closed-form descriptions of the late-time approach to dynamical extreme Reissner-Nordström black holes with persistent Aretakis instability.
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Krylov Complexity of Supersymmetric SYK Models
In finite-size N=2 SYK, breaking supersymmetry with an irrelevant deformation pushes late-time Krylov complexity to roughly half the maximal Krylov-space bound, while a mass deformation leaves saturation complexity a ...
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Holography of K-complexity: Switchbacks and Shockwaves
Operator Krylov complexity in triple-scaled DSSYK matches JT-gravity geodesic lengths with shockwaves and exhibits the switchback effect when the Lanczos algorithm is perturbed by two-sided operator insertions.
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Tests of restricted Quantum Focusing and a new CFT bound
From rQFC, a new CFT bound follows that forbids the QNEC from saturating faster than O(Σ^{d−2}) in near-vacuum states, while rQFC is proven in JT gravity and explicit QFC counterexamples are constructed.
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Entanglement Entropy of Quantum Corners
For a two-dimensional corner symmetry algebra, coherent corner states give an entanglement entropy that scales with the area when mapped to near-extremal Reissner-Nordström black holes.
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Probing the singularity at the holographic screen via $q$-holography
The probe-regime two-point function of sinh dilaton gravity matches the q-deformed Ward identity correlator, indicating an emergent quantum hyperbolic disk with SLq(2) isometry near the holographic boundary.
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A revision to the QES prescription
The paper proposes a weighted-sum revision of the quantum extremal surface formula, but the weight is assumed rather than derived.
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Gravitational dynamics of near-extreme Kerr (Anti-)de Sitter black holes
Near-extremal Kerr-dS4 and Kerr-AdS4 black holes admit a sector of metric perturbations whose linearized dynamics is the JT equation, with a Schwarzian effective action for the AdS case.
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Operator K-complexity in DSSYK: Krylov complexity equals bulk length
In the semiclassical limit of double-scaled SYK, Krylov complexity of an operator insertion equals total chord number, i.e., bulk wormhole length.
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Sine-dilaton gravity vs double-scaled SYK: exploring one-loop quantum corrections
The one-loop gravitational path integral of sine-dilaton gravity reproduces the one-loop corrections of double-scaled SYK for the free energy (up to an ordering ambiguity) and exactly for the matter two-point function.
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Two types of quantum chaos: testing the limits of the Bohigas-Giannoni-Schmit conjecture
A Metropolis-modified k-local SYK Hamiltonian keeps its chaotic early-time dynamics but changes its level statistics away from random-matrix universality at finite N.
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JT gravity and deformed CFTs
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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Comments on firewalls in JT gravity with matter
A twist factor cutoff from eigenvalue branes reproduces the gray hole firewall probabilities in JT gravity, with matter loop corrections subleading at late times.
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Thermal Pseudo-Entropy
Thermal pseudo-entropy is the analytic continuation S(β+it) of thermal entropy, equals the pseudo-entropy of a Thermofield Double transition matrix, and its averaged real part tracks the spectral form factor.
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Correlation functions of von Neumann entropy
Two-point correlators of modular Hamiltonians obey entropy-like properties and equal the stress-tensor conformal block for spherical regions in CFT, including imaginary-time separations.
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Spacetime-curvature induced uncertainty principle: linking the large-structure global effects to the local black hole physics
The authors derive a black hole metric with a cosmological-constant-dependent effective mass and use EHT and VLBI data to put extremely weak bounds on a quantum parameter beta.
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Notes on solution phase space and BTZ black hole
A detailed worked example showing that the solution phase space method reproduces the known mass, angular momentum, entropy, first law, and Smarr relation for the BTZ black hole and three-dimensional Kerr-dS spacetime.
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