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AdS/CFT Foundations

AdS/CFT is a surprising claim with a simple shape: a quantum theory of gravity in Anti-de Sitter spacetime can be exactly equivalent to an ordinary quantum field theory living on the boundary.

That sentence sounds almost too good to be true. This course is about making it precise.

If you are a senior undergraduate who has seen quantum field theory and general relativity, this course is meant to give you a real foothold. If you are a graduate student entering holography, it is meant to become your main spine. If you are a researcher from a nearby area, it is meant to be a reliable map of the assumptions, calculations, and modern language behind AdS/CFT.

The slogan is short:

gravity in asymptotically AdS spacetimequantum field theory on the boundary.\text{gravity in asymptotically AdS spacetime} \quad\longleftrightarrow\quad \text{quantum field theory on the boundary}.

The course is the long version of that slogan: why it is plausible, what it actually means, how to calculate with it, and where it stops being under control.

A good first encounter with AdS/CFT should not begin with ten-dimensional supergravity or a forest of indices. It should begin with three questions.

Why should gravity know about a lower-dimensional quantum theory? Black-hole entropy, large-NN gauge theory, and string theory all point toward the same strange idea: the fundamental variables of a gravitational system need not look local in the bulk.

Why Anti-de Sitter space? AdS has a timelike conformal boundary, a large symmetry group, and a natural relation between radial position and energy scale. These features make it the cleanest laboratory for holography.

What can I compute? Boundary correlators, thermal free energies, transport coefficients, Wilson loops, entanglement entropies, black-hole thermodynamics, and aspects of quantum gravity can all be translated into bulk problems.

For a gentle first week, read:

  1. Why Holography?
  2. What the Duality Claims
  3. Conformal Symmetry Minimum
  4. AdS as a Spacetime
  5. Statement of the Correspondence
  6. GKPW Prescription

Do not worry if the string-theory pages look unfamiliar on the first pass. The course introduces only the string theory needed to understand where the canonical example comes from.

The course assumes working familiarity with:

  • path integrals, sources, and correlation functions;
  • Yang–Mills theory and basic gauge invariance;
  • metrics, curvature, geodesics, horizons, and variational principles in general relativity;
  • comfort with learning new mathematical notation as needed.

It does not assume that you already know conformal field theory, supersymmetry, or string theory. Those topics appear, but the course develops the parts needed for AdS/CFT instead of asking you to master three separate subjects first.

A senior undergraduate can read the conceptual flow and many derivations. A graduate student should work through the exercises and reproduce the central calculations. A researcher should use the course map and appendices as a reference spine.

The canonical example is

N=4  SU(N)  super-Yang–Mills theory in four dimensionstype IIB string theory on AdS5×S5.\mathcal N=4\; SU(N)\;\text{super-Yang–Mills theory in four dimensions} \quad\longleftrightarrow\quad \text{type IIB string theory on }\mathrm{AdS}_5\times S^5 .

The field theory is a conformal gauge theory. The bulk theory is a quantum theory of closed strings, containing gravity. In a special large-NN, strong-coupling regime, the string theory simplifies to classical supergravity on a weakly curved spacetime.

The most useful parameter map is

λ=gYM2N,L4α2λ,gsλN.\lambda = g_{\mathrm{YM}}^2 N, \qquad \frac{L^4}{\alpha'^2} \sim \lambda, \qquad g_s \sim \frac{\lambda}{N}.

Here LL is the AdS radius, α\alpha' is the string length squared, gsg_s is the string coupling, and λ\lambda is the ‘t Hooft coupling. The interpretation is:

  • large NN suppresses quantum loops in the bulk;
  • large λ\lambda suppresses stringy corrections;
  • finite NN probes quantum gravity;
  • finite λ\lambda probes stringy physics.

Classical Einstein gravity is therefore not the full duality. It is a powerful and controlled corner of a larger equivalence.

The basic working form of the correspondence is the relation between boundary generating functionals and bulk partition functions:

ZCFT[ϕ(0)]=Zbulk ⁣[ϕϕ(0)].Z_{\mathrm{CFT}}[\phi_{(0)}] = Z_{\mathrm{bulk}}\!\left[\phi \to \phi_{(0)}\right].

In the classical Euclidean gravity approximation,

Zbulk ⁣[ϕϕ(0)]exp ⁣(Sren,on-shell[ϕ(0)]),Z_{\mathrm{bulk}}\!\left[\phi \to \phi_{(0)}\right] \approx \exp\!\left(-S_{\text{ren,on-shell}}[\phi_{(0)}]\right),

so that

WCFT[ϕ(0)]Sren,on-shell[ϕ(0)].W_{\mathrm{CFT}}[\phi_{(0)}] \approx -S_{\text{ren,on-shell}}[\phi_{(0)}].

The boundary value ϕ(0)\phi_{(0)} of a bulk field ϕ\phi acts as a source for a boundary operator O\mathcal O:

ZCFT[ϕ(0)]=exp ⁣(AdSϕ(0)O).Z_{\mathrm{CFT}}[\phi_{(0)}] = \left\langle \exp\!\left( \int_{\partial\mathrm{AdS}} \phi_{(0)}\mathcal O \right) \right\rangle.

This formula is schematic until one specifies boundary conditions, counterterms, Lorentzian versus Euclidean signature, and normalization conventions. Much of the course is devoted to turning this compact equation into a dependable computational method.

By the end of the core path, you should be able to:

  1. explain why large-NN gauge theories naturally resemble weakly coupled bulk theories;

  2. derive the emergence of AdS5×S5\mathrm{AdS}_5\times S^5 from the near-horizon limit of D3-branes;

  3. compute simple CFT correlators from bulk on-shell actions;

  4. derive the scalar mass-dimension relation

    m2L2=Δ(Δd);m^2L^2=\Delta(\Delta-d);
  5. distinguish sources, responses, normalizable modes, and expectation values;

  6. carry out the basic steps of holographic renormalization;

  7. relate black branes to thermal CFT states;

  8. understand why quasinormal modes are poles of retarded Green functions;

  9. use RT/HRT surfaces to compute and interpret entanglement entropy;

  10. recognize which claims are exact, which are semiclassical, and which are phenomenological models.

The point is not to memorize a dictionary. The point is to learn how the dictionary is built.

This path is for readers who want the big picture before the technical machinery:

  1. Why Holography?
  2. What the Duality Claims
  3. Conformal Symmetry Minimum
  4. AdS as a Spacetime
  5. Global AdS and the Cylinder
  6. D3-Branes: Two Descriptions
  7. Statement of the Correspondence
  8. Ryu–Takayanagi formula

Skip long derivations on the first pass; return to them when the conceptual map is stable.

This path gives the calculational foundation:

  1. QFT Data and Generating Functionals
  2. Large N Gauge Theory
  3. Fields in AdS
  4. GKPW Prescription
  5. Scalar Two-Point Functions
  6. Mass-Dimension Relation
  7. Counterterms and Renormalized Action
  8. Practical Recipe

After the basic dictionary:

  1. Witten Diagrams
  2. Three-Point Functions and Bulk Couplings
  3. Four-Point Functions and Bulk Locality
  4. Wilson Loops
  5. Probe Branes and Flavor

For thermal field theory, transport, and response:

  1. Black Branes and Thermal CFTs
  2. Hawking–Page transition
  3. Euclidean Gravity and Free Energy
  4. Real-Time Prescription
  5. Retarded Green Functions
  6. Quasinormal Modes
  7. Hydrodynamics from Gravity
  8. Shear Viscosity

For quantum information and emergent spacetime:

  1. Entanglement Entropy in QFT
  2. Ryu–Takayanagi formula
  3. Covariant HRT formula
  4. Entanglement Wedges
  5. Relative Entropy and Linearized Gravity
  6. Quantum Extremal Surfaces
  7. Islands and Information

For bulk emergence, reconstruction, and black-hole information:

  1. Bulk Effective Field Theory
  2. Large N Factorization and Fock Space
  3. Bulk Reconstruction
  4. Quantum Error Correction
  5. Black-Hole Information in AdS/CFT
  6. Stringy and Quantum Corrections
  7. Open Problems and Research Map
PagePurpose
Why Holography?Motivation from quantum gravity, strongly coupled QFT, entropy, and black holes.
What the Duality ClaimsThe exact, semiclassical, and practical meanings of AdS/CFT.
Regimes of ValidityWhen the bulk is quantum string theory, classical string theory, supergravity, or Einstein gravity.
Conventions and UnitsCourse-wide signatures, dimensions, indices, Fourier conventions, and source normalizations.
RoadmapHow to navigate the course by interest and preparation.
PagePurpose
QFT Data and Generating FunctionalsSources, Z[J]Z[J], W[J]W[J], connected correlators, and Ward identities.
Conformal Symmetry MinimumThe CFT ingredients needed for holography.
Radial Quantization and the CylinderThe map from flat-space CFT to the cylinder Hilbert space.
Large N Gauge Theory’t Hooft counting, planar diagrams, and the string-genus expansion.
Single Trace and FactorizationSingle-particle/multiparticle bulk interpretation from CFT operators.
N=4\mathcal N=4 Super-Yang–MillsThe canonical boundary theory of AdS5_5/CFT4_4.
Thermal States and Density MatricesBoundary thermal field theory before black branes.
PagePurpose
AdS as a SpacetimeEmbedding, curvature, universal cover, and boundary intuition.
Coordinate SystemsGlobal, Poincare, Fefferman–Graham, black-brane, and EF coordinates.
Conformal BoundaryConformal compactification and boundary conformal classes.
Global AdS and the CylinderWhy global AdS talks to the CFT on R×Sd1\mathbb R\times S^{d-1}.
Isometries and Conformal SymmetryThe SO(2,d)SO(2,d) symmetry match.
Fields in AdSNear-boundary falloffs and the first source-response bridge.
Black Holes and Black BranesThe geometric side of thermal CFT states.
Euclidean AdS and Thermal CirclesSmooth Euclidean horizons and Hawking temperature.
PagePurpose
Open and Closed StringsThe minimal string ingredients behind gauge fields and gravitons.
D-Branes for Field TheoristsD-branes as open-string worlds, gauge theories, and closed-string sources.
D3-Branes: Two DescriptionsThe open-string SYM and closed-string geometry descriptions.
Near-Horizon GeometryHow the D3-brane throat becomes AdS5×S5\mathrm{AdS}_5\times S^5.
Decoupling LimitWhy the field theory and AdS throat decouple from flat-space gravity.
Parameter MapThe map between NN, λ\lambda, gsg_s, LL, α\alpha', and Newton constants.
Why Classical Gravity EmergesHow large NN and large gap/large λ\lambda produce classical bulk gravity.
PagePurpose
Statement of the CorrespondenceThe exact, semiclassical, and classical statements of the duality.
GKPW PrescriptionBoundary sources as bulk boundary values.
Scalar Two-Point FunctionsA complete first correlator computation.
Mass-Dimension RelationThe derivation of m2L2=Δ(Δd)m^2L^2=\Delta(\Delta-d).
Alternate Quantization and BF BoundStability, falloffs, and source-response exchange.
One-Point Functions and VEVsExtracting expectation values from renormalized variations.
Spin, Symmetry, and Conserved CurrentsScalars, spinors, gauge fields, currents, and symmetries.
Stress Tensor and the MetricThe boundary metric source and holographic stress tensor.
PagePurpose
Why Renormalization Is NeededInfinite AdS volume, UV/IR relation, and local counterterms.
Near-Boundary ExpansionThe asymptotic expansions for scalars, metrics, and gauge fields.
Counterterms and Renormalized ActionConstructing SrenS_{\rm ren} from regulated actions and counterterms.
One-Point Functions from VariationCanonical momenta and finite vevs.
Ward Identities and AnomaliesGauge, diffeomorphism, and Weyl identities from bulk constraints.
Radial Hamiltonian ViewpointHolographic renormalization as a Hamilton–Jacobi problem.
Practical RecipeA reusable checklist for calculations.
PagePurpose
Witten DiagramsThe AdS analogue of Feynman diagrams.
Three-Point Functions and Bulk CouplingsCubic couplings and CFT OPE coefficients.
Four-Point Functions and Bulk LocalityCross ratios, double-trace towers, Mellin amplitudes, and locality.
Heavy Operators and GeodesicsLarge-Δ\Delta operators as bulk particles.
Wilson LoopsFundamental strings ending on boundary loops.
Probe Branes and FlavorFlavor branes, mesons, and probe limits.
Bulk Causality and Boundary ConsistencyBoundary constraints on bulk effective interactions.
PagePurpose
Black Branes and Thermal CFTsPlanar horizons as homogeneous thermal states.
Hawking–Page transitionThermal AdS versus global AdS black holes.
Euclidean Gravity and Free EnergyComputing FF, EE, and SS from IEI_E.
Real-Time PrescriptionLorentzian AdS/CFT and infalling boundary conditions.
Retarded Green FunctionsPractical computation of GRG_R.
Quasinormal ModesQNM spectra as poles of retarded correlators.
Hydrodynamics from GravityFluid/gravity and long-wavelength black-brane dynamics.
Shear ViscosityThe Kubo calculation of η/s=1/(4π)\eta/s=1/(4\pi).
PagePurpose
Entanglement Entropy in QFTReduced density matrices, replica trick, and modular Hamiltonians.
Ryu–Takayanagi formulaStatic holographic entanglement from minimal surfaces.
Covariant HRT formulaTime-dependent entanglement from extremal surfaces.
Entanglement WedgesSubregion duality and reconstructable bulk regions.
Relative Entropy and Linearized GravityHow entanglement first laws imply linearized Einstein equations.
Quantum Extremal SurfacesGeneralized entropy and bulk quantum corrections.
Islands and InformationPage curves, islands, and black-hole information.
PagePurpose
Why AdS3_3 Is SpecialNo local gravitons, boundary gravitons, and strong CFT2_2 control.
Brown–Henneaux central chargeThe derivation and meaning of c=3L/(2G3)c=3L/(2G_3).
BTZ Black HolesRotating BTZ geometry, thermodynamics, and CFT charges.
Cardy Formula and Black-Hole EntropyMatching BTZ entropy from Virasoro state counting.
Virasoro Symmetry and Boundary GravitonsPhysical large diffeomorphisms and the vacuum module.
Lessons for Higher-Dimensional HolographyWhat generalizes and what is special to three dimensions.
PagePurpose
What Counts as a Holographic CFT?Large NN, sparse spectrum, large gap, and local bulk EFT.
Other AdS BackgroundsABJM, M5, conifolds, D1-D5, quivers, and internal spaces.
RG Flows and Domain WallsRelevant deformations and radial evolution.
Confinement and Hard-Wall ModelsMass gaps, hard-wall AdS/QCD, and confinement diagnostics.
Finite Density and Bulk Gauge FieldsChemical potentials, charge density, and boundary conditions.
Reissner–Nordstrom AdSCharged black branes and finite-density states.
AdS2_2 Throats and IR CriticalityEmergent near-horizon scaling at extremality.
Holographic ConductivityKubo formulas, membrane paradigm, and transport caveats.
Holographic SuperconductorsCharged scalar hair and condensates.
Fermions and Spectral FunctionsBulk spinors, spectral densities, and holographic Fermi surfaces.
Bottom-Up ModelsHow to build useful phenomenological holographic models responsibly.
Limits of the DictionaryWhat is controlled, what is effective, and what is still speculative.
PagePurpose
Bulk Effective Field TheoryHow CFT data yields approximate local bulk EFT.
Large N Factorization and Fock SpaceMultiparticle bulk Hilbert spaces from multi-trace operators.
Bulk ReconstructionHKLL, subregion reconstruction, and gravitational dressing.
Quantum Error CorrectionRedundant encoding, code subspaces, and entanglement wedges.
Black-Hole Information in AdS/CFTBoundary unitarity, Page curves, islands, and interiors.
Stringy and Quantum Corrections1/N1/N, 1/λ1/\lambda, higher-derivative, KK, and nonperturbative corrections.
Open Problems and Research MapResearch directions after the course.
PagePurpose
NotationSymbols and conventions used throughout the course.
Differential Geometry CheatsheetCurvature, hypersurfaces, extrinsic curvature, and Brown–York data.
AdS Coordinate SystemsA reference atlas for common AdS metrics.
Variational Principles and Boundary TermsScalar, Maxwell, gravity, fermion, and mixed-boundary variations.
Green Functions CheatsheetEuclidean, retarded, Feynman, spectral, thermal, and SK correlators.
CFT CheatsheetConformal symmetry, OPEs, blocks, Ward identities, and CFT data.
String Theory CheatsheetStrings, branes, fluxes, parameter maps, and correction hierarchies.
Problem SetsCourse-wide exercises with solutions.
BibliographyAnnotated references and reading paths.
Boundary QFTBulk AdS description
spacetime where the QFT livesconformal boundary of AdS
energy scaleradial position
source ϕ(0)\phi_{(0)}boundary value of bulk field ϕ\phi
local operator O\mathcal Obulk field ϕ\phi
expectation value O\langle\mathcal O\ranglenormalizable response of ϕ\phi
stress tensor TijT_{ij}bulk metric gMNg_{MN}
conserved current JiJ^ibulk gauge field AMA_M
thermal stateAdS black hole or black brane
entropyhorizon area or extremal-surface area
large NNweak bulk quantum loops
large λ\lambda or large spectral gapweak stringy/higher-spin corrections

This table is only a first orientation. Every entry has qualifications, and many of the most important pages explain those qualifications.

Not quite. The AdS boundary is reached after conformal compactification. It is not an ordinary material surface at finite proper distance.

“The radial direction is just another spatial direction.”

Section titled ““The radial direction is just another spatial direction.””

From the bulk point of view, it is geometric. From the boundary point of view, it is tied to energy scale and renormalization.

Classical gravity is a limit of AdS/CFT. The full correspondence involves quantum string theory or M-theory.

“Every CFT has a simple Einstein-gravity dual.”

Section titled ““Every CFT has a simple Einstein-gravity dual.””

No. A simple local bulk EFT requires special CFT properties, especially large NN and a sparse light spectrum with a large gap.

A good first pass is to read for structure rather than mastery. Learn what each page is for, then return to the derivations when you need them. The appendices are designed to be opened constantly while reading the main course pages.

The exercises are intentionally mixed: some check definitions, some reproduce core derivations, and some point toward research-level questions. Work through the solved exercises actively; many contain the fastest route to understanding the dictionary.