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Anti-de Sitter Geometry and the Conformal Boundary

Anti-de Sitter space is the maximally symmetric Lorentzian spacetime of constant negative curvature. Its conformal boundary is timelike, so bulk evolution is not specified by Cauchy data alone. The curvature radius LL, boundary conformal class, covering space, and boundary condition are therefore physical entries in a holographic dictionary, not disposable coordinate choices Aharony et al. 2000, §2.

Required background. Smooth manifolds, tangent spaces, and tensors supplies induced metrics and curvature tensors. Helpful background. Conformal geometry and compactification supplies the boundary action of SO(d,2)SO(d,2), while timelike AdS boundaries develops the general evolution problem.

Constant negative curvature from the embedding

Section titled “Constant negative curvature from the embedding”

Use the site-wide Lorentzian signature (+,,,)(+,-,\ldots,-) and curvature convention [M,N]VP=RPQMNVQ[\nabla_M,\nabla_N]V^P=R^P{}_{QMN}V^Q. Embed AdSd+1_{d+1} in R2,d\mathbb R^{2,d} with ambient quadratic form

X12+X02i=1dXi2=L2.X_{-1}^2+X_0^2-\sum_{i=1}^{d}X_i^2=L^2.

The normal is proportional to XAX^A, and the Gauss equation immediately gives

RMNPQ=1L2(gMPgNQgMQgNP),R_{MNPQ}=-\frac{1}{L^2} \left(g_{MP}g_{NQ}-g_{MQ}g_{NP}\right),

so that

RMN=dL2gMN,R=d(d+1)L2.R_{MN}=-\frac d{L^2}g_{MN}, \qquad R=-\frac{d(d+1)}{L^2}.

In vacuum Einstein gravity this solves RMN12RgMN+ΛgMN=0R_{MN}-\tfrac12Rg_{MN}+\Lambda g_{MN}=0 with Λ=d(d1)/(2L2)\Lambda=-d(d-1)/(2L^2). These signs are correlated. Flipping the Riemann convention reverses the displayed curvature tensors but cannot change invariant statements such as negative sectional curvature or the isometry group.

Global coordinates

X1=Lcoshρcosτ,X0=Lcoshρsinτ,Xi=LsinhρniX_{-1}=L\cosh\rho\cos\tau, \quad X_0=L\cosh\rho\sin\tau, \quad X_i=L\sinh\rho\,n_i

give

ds2=L2(cosh2ρdτ2dρ2sinh2ρdΩd12).\mathrm ds^2=L^2\left(\cosh^2\rho\,\mathrm d\tau^2-\mathrm d\rho^2 -\sinh^2\rho\,\mathrm d\Omega_{d-1}^2\right).

The hyperboloid itself has closed timelike curves because τ\tau is periodic. Physical AdS normally means its universal cover, τR\tau\in\mathbb R. This global choice is distinct from any local curvature statement.

Conformal compactification and causal travel time

Section titled “Conformal compactification and causal travel time”

Set tanχ=sinhρ\tan\chi=\sinh\rho, with 0χ<π/20\leq\chi<\pi/2. Then

ds2=L2cos2χ(dτ2dχ2sin2χdΩd12).\mathrm ds^2=\frac{L^2}{\cos^2\chi} \left(\mathrm d\tau^2-\mathrm d\chi^2-\sin^2\chi\,\mathrm d\Omega_{d-1}^2\right).

Removing the divergent Weyl factor produces the Einstein static cylinder. The boundary at χ=π/2\chi=\pi/2 has conformal metric

ds2=dτ2dΩd12.\mathrm ds_{\partial}^2=\mathrm d\tau^2-\mathrm d\Omega_{d-1}^2.

It is timelike: radial null curves satisfy dτ=±dχ\mathrm d\tau=\pm\mathrm d\chi and reach the boundary in finite global time Δτ=π/2\Delta\tau=\pi/2. Signals can therefore leave the bulk unless a boundary rule returns them or an explicitly enlarged exterior system receives them. This is the geometric origin of the AdS initial-boundary value problem emphasized by Ishibashi and Wald 2004, §3.

Only the conformal class [g(0)][g_{(0)}] is intrinsic at the boundary. Choosing a representative fixes a scale and hence a particular boundary Hamiltonian. On the cylinder, global time translations are generated by the CFT dilatation operator after the flat-space-to-cylinder map.

Isometries and boundary conformal transformations

Section titled “Isometries and boundary conformal transformations”

The ambient transformations preserving the quadratic form form SO(d,2)SO(d,2), up to connected components and global coverings. They act linearly on XAX^A and induce AdS isometries. Near the boundary the same transformations act as conformal transformations of the dd-dimensional boundary metric. Thus the equality of Lie algebras

isom(AdSd+1)so(d,2)conf(R1,d1)\mathfrak{isom}(\mathrm{AdS}_{d+1})\cong\mathfrak{so}(d,2) \cong\mathfrak{conf}(\mathbb R^{1,d-1})

is a geometric compatibility condition for the dictionary. It does not determine the boundary theory, its operator spectrum, its global conformal group, or the existence of a duality. The original GKPW construction uses precisely this conformal boundary structure while retaining separate dynamical assumptions Witten 1998, §§2–3.

First application: embedding, boundary, and symmetry

Section titled “First application: embedding, boundary, and symmetry”

The hyperboloid calculation supplies one internally checked package: the induced metric has curvature radius LL, compactification produces the cylinder conformal class, and the same ambient SO(d,2)SO(d,2) transformations become boundary conformal transformations. These three facts—not the embedding equation alone—are the geometric input used by the field/operator map.

Convention reversal as an adversarial check

Section titled “Convention reversal as an adversarial check”

Suppose a source uses the opposite Riemann sign while retaining mostly-minus signature. Its statement RMN=+dL2gMNR_{MN}=+dL^{-2}g_{MN} translates to the QFT.org convention by reversing the curvature tensor definition, not by changing Λ\Lambda physically. A consistent round trip must reproduce:

  • the scalar curvature radius R=d(d+1)/L2\lvert R\rvert=d(d+1)/L^2;
  • the SO(d,2)SO(d,2) Killing algebra;
  • the null travel time on the compactified cylinder;
  • the scalar mass–dimension invariant Δ(Δd)=m2L2\Delta(\Delta-d)=m^2L^2 once the wave-equation convention is translated.

If only one sign is flipped, these checks disagree. The strongest surviving claim is then merely that a coordinate metric was written, not that it realizes the stated AdS curvature convention.

This page establishes exact pure-AdS geometry on the universal cover; it does not select a quantum state, boundary condition, or dual CFT. Global, Poincaré, and AdS-Rindler Patches next restricts this geometry to observable-dependent coordinate domains, while Timelike-Boundary Causality and Boundary-Value Problems supplies the missing evolution data.

Show that a radial light ray emitted from the origin at τ=0\tau=0 reaches the boundary at τ=π/2\tau=\pi/2 and returns to the origin at τ=π\tau=\pi under reflecting boundary data.

Solution

For a radial null curve, dΩd1=0\mathrm d\Omega_{d-1}=0 and the compactified metric gives dτ=dχ\mathrm d\tau=\mathrm d\chi on the outgoing leg. Integrating from χ=0\chi=0 to π/2\pi/2 gives Δτ=π/2\Delta\tau=\pi/2. Reflection reverses the radial direction; a further interval π/2\pi/2 reaches the center along the opposite angular ray. The total is π\pi. The statement uses reflecting data—geometry alone does not specify the return.

The chapter overview contains the structure diagram and validity and failure diagram. They are embedded there once so that their shared chapter-level context is not repeated on every article.

For the chapter-wide comparison of assumptions, counterevidence, falsifiers, and claim ceilings, see the claim-domain table.

  • Aharony, Ofer, Steven S. Gubser, Juan Maldacena, Hirosi Ooguri, and Yaron Oz. “Large N Field Theories, String Theory and Gravity.” Physics Reports 323 (2000): 183–386. arXiv. DOI.
  • Ishibashi, Akihiro, and Robert M. Wald. “Dynamics in Non-Globally-Hyperbolic Static Spacetimes III: Anti-de Sitter Spacetime.” Classical and Quantum Gravity 21 (2004): 2981–3014. arXiv. DOI.
  • Witten, Edward. “Anti-de Sitter Space and Holography.” Advances in Theoretical and Mathematical Physics 2 (1998): 253–291. arXiv. DOI.