5. Metric perturbations invisible to restricted families
All radii and centers on one slice give exactly when there. The slice proof shows why this condition does not control time derivatives or the other components of . For example, a spatial perturbation proportional to can vanish with its first time derivative at 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 fix a spatial point strictly inside the bulk slice. In the static metric with , vary only by a smooth compactly supported . Choose and in an orthonormal horizontal frame. A mixed quadratic multiplied by a bump equal to one near gives such an . The tangent 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
as follows from substituting the mixed time connection coefficients. Its off-diagonal variation at is . The trace and cosmological terms contribute zero to that component, so . 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 and use the symmetric off-diagonal perturbation
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 . In (2) the area integrand is odd separately in and , so the area variation vanishes directly. The boundary time-time charge also vanishes.
Inside the Fefferman–Graham conformal factor, the dimensionless perturbation is
The transverse, trace-free equation for is
Substitution cancels the term with no derivatives on . After removing the common factor , the transverse equation for the profile becomes
The profile above instead gives residual . 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 , . Its asymptotic charge vanishes. Formula (2) gives
Integrating the cosine series against the polynomial weight proves the second equality; the standard integral representation of gives it as well. Any positive zero at gives a nonzero perturbation invisible to every center at the one radius . This uses the admissible class with no horizontal decay condition. Replacing the cosine by 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 solves the equation for 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.