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Shadow Theory

What fixed-slice balls miss

Construct non-gauge lapse and cross-mode perturbations that evade all rest-frame balls, and isolate the effects of fixing a radius or center.

5. Metric perturbations invisible to restricted families

All radii and centers on one slice give DB=0D_B=0 exactly when δR[q]=0\delta R[q]=0 there. The slice proof shows why this condition does not control time derivatives or the other components of hh. For example, a spatial perturbation proportional to (t−t0)2(t-t_0)^2 can vanish with its first time derivative at t0t_0 and still change the spatial evolution equations. The next two constructions are invisible to a larger family.

Keep the same regions and change the order of response. Second-Order Detection by Boundary Balls constructs a transverse AdS solution whose first-order area and energy both vanish on these fixed-slice balls, but whose bulk canonical energy is positive at every radius. The boundary relative-entropy interpretation of that energy needs the holographic dictionary and an admissible state family.

A compactly supported lapse perturbation

For d≥3d\geq3 fix a spatial point pp strictly inside the bulk slice. In the static metric −N2dt2+qˉ-N^2dt^2+\bar q with N=L/zN=L/z, vary only NN by a smooth compactly supported nn. Choose n(p)=Dn(p)=0n(p)=Dn(p)=0 and D1D2n(p)≠0D_1D_2 n(p)\ne0 in an orthonormal horizontal frame. A mixed quadratic multiplied by a bump equal to one near pp gives such an nn. The tangent htt=−2Nnh_{tt}=-2Nn has radial gauge and vanishes near the conformal boundary. The spatial metric is unchanged at every time. Consequently every rest-frame ball has zero area variation and zero boundary charge.

The spatial Ricci tensor of the static spacetime is

Ric⁡AB[qˉ]−N−1DADBN,\operatorname{Ric}_{AB}[\bar q]-N^{-1}D_AD_BN,

as follows from substituting the mixed time connection coefficients. Its off-diagonal variation at pp is −N−1D1D2n-N^{-1}D_1D_2n. The trace and cosmological terms contribute zero to that component, so E12≠0E_{12}\ne 0. A linearized diffeomorphism of an on-shell background has zero residual by covariance. This compactly supported example is therefore non-gauge, with vanishing boundary stress variation. It remains invisible under time translations in the same frame.

A nonzero Ward-compatible boundary tensor

In boundary dimension three, set h12=zH12h_{12}=zH_{12} and use the symmetric off-diagonal perturbation

h12=z(t2+z2/7+1/3)h_{12}=z(t^2+z^2/7+1/3)

with other independent components zero. The boundary tensor is nonzero, traceless and conserved: its only entries are spatial cross components independent of the spatial coordinates. On a rest slice the induced perturbation is trace free and divergence free in the hyperbolic background, hence δR=0\delta R=0. In (2) the area integrand is odd separately in y1y^1 and y2y^2, so the area variation vanishes directly. The boundary time-time charge also vanishes.

Inside the Fefferman–Graham conformal factor, the dimensionless perturbation is

γ12=z2h12L2=z3H12L2.\gamma_{12}=\frac{z^2h_{12}}{L^2}=\frac{z^3H_{12}}{L^2}.

The transverse, trace-free equation for γ12\gamma_{12} is

(∂z2−2z−1∂z−∂t2)γ12=0.(\partial_z^2-2z^{-1}\partial_z-\partial_t^2)\gamma_{12}=0.

Substitution cancels the term with no derivatives on H12H_{12}. After removing the common factor z3/L2z^3/L^2, the transverse equation for the profile becomes

(∂z2+4z−1∂z−∂t2)H12=0.(\partial_z^2+4z^{-1}\partial_z-\partial_t^2)H_{12}=0.

The profile above instead gives residual −4/7-4/7. The perturbation is off shell and non-gauge. A boost with velocity components along both spatial directions couples to the spatial cross residual and can detect it. Ward compatibility here is a property of the geometric boundary data; no corresponding CFT state is asserted.

Fixing the radius or the center

In three bulk dimensions take hxx=z4cos⁡(kx)h_{xx}=z^4\cos(kx), k>0k>0. Its asymptotic charge vanishes. Formula (2) gives

GD(R,x0)=cos⁡(kx0)8LR∫−RR(R2−y2)3cos⁡(ky) dy=cos⁡(kx0)8LRπ Γ(4)(2R/k)7/2J7/2(kR).\begin{aligned} GD(R,x_0) &=\frac{\cos(kx_0)}{8LR}\int_{-R}^R(R^2-y^2)^3\cos(ky)\,dy\\ &=\frac{\cos(kx_0)}{8LR}\sqrt\pi\,\Gamma(4)(2R/k)^{7/2}J_{7/2}(kR). \end{aligned}

Integrating the cosine series against the polynomial weight proves the second equality; the standard integral representation of JνJ_\nu gives it as well. Any positive zero at kR0kR_0 gives a nonzero perturbation invisible to every center at the one radius R0R_0. This uses the admissible class with no horizontal decay condition. Replacing the cosine by sin⁡(k(x−x0))\sin(k(x-x_0)) gives an odd integrand and a fixed-center kernel for every radius.

These examples concern the defect. Even on shell, the separate entropy data in one frame can miss components. The spatial cross profile H12=t2+z2/5+1/3H_{12}=t^2+z^2/5+1/3 solves the equation for H12H_{12} above, has the same boundary cross stress, and gives zero area variation for every rest-frame ball. Its nonzero boundary stress distinguishes it from a boundary-trivial gauge transformation.

Published source: Boundary Ball Readouts and Linearized Einstein Gravity in a Source–Readout Architecture. Read the original PDF alongside the web treatment.