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Shadow Theory

Bulk horizon geometry and the counting cutoff

Recover the same time normalization in the AdS wedge, then distinguish the stationary entropy density and regulator from the algebraic aperture.

4. Bulk realization and horizon entropy

Assume a classical AdS dual of radius LL for the boundary vacuum. Choose the boundary frame through the bulk defining function, and assume the thermal entropy of the dual saddle is its stationary horizon entropy at leading bulk semiclassical order. Write h=ρ2−L2h=\sqrt{\rho^2-L^2} for ρ>L\rho>L.

The hyperbolic chart maps to Poincaré coordinates by

Q=ρcosh⁡u+hcosh⁡(τ/R),zP=RLQ,t=Rhsinh⁡(τ/R)Q,r=Rρsinh⁡uQ.Q=\rho\cosh u+h\cosh(\tau/R),\qquad z_P=\frac{RL}{Q},\qquad t=\frac{Rh\sinh(\tau/R)}{Q},\qquad r=\frac{R\rho\sinh u}{Q}.

Substitution into L2zP−2(dzP2−dt2+dr2+r2dΩd−22)L^2z_P^{-2}(dz_P^2-dt^2+dr^2+r^2d\Omega_{d-2}^2) gives

ds2=dρ2f(ρ)−f(ρ) dτ~ 2+ρ2dHd−12,f(ρ)=ρ2L2−1,τ~=LτR.ds^2=\frac{d\rho^2}{f(\rho)}-f(\rho)\,d\widetilde{\tau}^{\,2}+\rho^2dH_{d-1}^2,\qquad f(\rho)=\frac{\rho^2}{L^2}-1,\qquad \widetilde{\tau}=\frac{L\tau}{R}.

As ρ→∞\rho\to\infty the map recovers the boundary conformal map. The inverse radial relation is

ρ2−L2=L24R2zP2[(R−t)2−r2−zP2][(R+t)2−r2−zP2].\rho^2-L^2=\frac{L^2}{4R^2z_P^2} \left[(R-t)^2-r^2-z_P^2\right]\left[(R+t)^2-r^2-z_P^2\right].

Both factors are positive on the exterior connected to the boundary diamond. Its null boundaries meet on t=0, r2+zP2=R2t=0,\ r^2+z_P^2=R^2. The chart therefore reads a wedge of the same pure AdS geometry. The bulk Killing generator restricts to the same future boundary flow, with the zP∂zPz_P\partial_{z_P} term included before restriction. Euclidean smoothness requires period 4π/f′(L)=2πL4\pi/f'(L)=2\pi L in τ~\widetilde{\tau}, giving 2πR2\pi R in τ\tau. Independently, the surface gravity for ∂τ\partial_\tau is 1/R1/R.

Stationary entropy density

For a local Lagrangian scalar L(g,Rabcd)\mathcal L(g,R_{abcd}), the stationary prescription is 8

S=−2π∫Σγ ∂L∂Rabcdϵabϵcd,ϵabϵab=−2.S=-2\pi\int_\Sigma\sqrt{\gamma}\,\frac{\partial\mathcal L}{\partial R_{abcd}}\epsilon_{ab}\epsilon_{cd}, \qquad \epsilon_{ab}\epsilon^{ab}=-2.

In Einstein gravity the contraction is −1/(8πG)-1/(8\pi G), giving area divided by 4G4G, in agreement with the spherical Ryu–Takayanagi surface 9. In Gauss–Bonnet gravity with coefficient λL02/[(d−2)(d−3)]\lambda L_0^2/[(d-2)(d-3)] inside the Einstein normalization, take d≥4d\ge4, f∞=L02/L2f_\infty=L_0^2/L^2 and 1−f∞+λf∞2=01-f_\infty+\lambda f_\infty^2=0. The induced section has scalar curvature −(d−1)(d−2)/L2-(d-1)(d-2)/L^2. The stationary entropy density is 1/(4G)1/(4G) times 1+2λL02RΣ/[(d−2)(d−3)]1+2\lambda L_0^2\mathcal R_\Sigma/[(d-2)(d-3)] 10. Hence

ad∗=πd/2Ld−18πGΓ(d/2)(1−2(d−1)λf∞d−3).a_d^*=\frac{\pi^{d/2}L^{d-1}}{8\pi G\Gamma(d/2)} \left(1-\frac{2(d-1)\lambda f_\infty}{d-3}\right).

The independent curvature contraction agrees with this density. Identifying it with the definition through the on-shell AdS Lagrangian uses the vacuum equation. The calculation concerns stationary spherical horizons. It makes no general claim about entropy functionals on arbitrary entangling surfaces.

5. Counting and matching the cutoffs

At the bifurcation surface, zP=R/cosh⁡uz_P=R/\cosh u. Thus zP=δz_P=\delta gives cosh⁡ubulk=R/δ\cosh u_{\mathrm{bulk}}=R/\delta. At boundary time τ=0\tau=0, the map gives r=Rtanh⁡(u/2)r=R\tanh(u/2), so the sharp radius r=R−δr=R-\delta gives e−uCFT=δ/(2R−δ)e^{-u_{\mathrm{CFT}}}=\delta/(2R-\delta). Write ε=δ/R\varepsilon=\delta/R. In the common variable X=sinh⁡umax⁡X=\sinh u_{\max},

Xbulk=ε−11−ε2,XCFT=ε−12(1−ε)2−ε.X_{\mathrm{bulk}}=\varepsilon^{-1}\sqrt{1-\varepsilon^2},\qquad X_{\mathrm{CFT}}=\varepsilon^{-1}\frac{2(1-\varepsilon)}{2-\varepsilon}.

Both give e−umax⁡∼ε/2e^{-u_{\max}}\sim\varepsilon/2. In that variable the bulk prescription minus the CFT prescription is −ε2/4+O(ε4)-\varepsilon^2/4+O(\varepsilon^4).

The tube and the algebra it generates

The spatial cutoff applied for every τ\tau defines a timelike tube UU in the diamond. It contains the entire open axis segment r=0, ∣t∣<Rr=0,\ |t|<R. A point (t0,r0)(t_0,r_0) is spacelike to that segment precisely when r0≥R+∣t0∣r_0\ge R+|t_0|, with the usual open-region convention for causal complements. By inclusion, the double causal complement of the tube has interior DD.

The timelike envelope can also be found directly. For each p=(t,x)∈Dp=(t,x)\in D, take two axis points in UU, one strictly to its timelike past and one strictly to its timelike future. The line segments through pp give a piecewise timelike curve. Contracting the spatial component linearly to the axis keeps the endpoints fixed and preserves timelikeness. Smooth the corners within the open timelike cones. This puts pp in the timelike envelope of UU. Conversely, a future timelike curve between points of UU remains in the causally convex diamond.

Under the hypotheses of the applicable timelike-tube theorem 7, this gives A(U)=A(D)\mathcal A(U)=\mathcal A(D). The smaller diamond of radius R−δR-\delta shares the tube's spatial section at τ=0\tau=0, but its full image under conformal transport has finite time extent. The shared section does not identify their spacetime apertures or specify regulated traces. Even the smaller diamond's algebra remains type III under the same net hypothesis.

Published source: Modular Transport and Spherical Holographic Entanglement Entropy in a Source–Readout Architecture. Read the original PDF alongside the web treatment.