4. Bulk realization and horizon entropy
Assume a classical AdS dual of radius 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 for .
The hyperbolic chart maps to Poincaré coordinates by
Substitution into gives
As the map recovers the boundary conformal map. The inverse radial relation is
Both factors are positive on the exterior connected to the boundary diamond. Its null boundaries meet on . 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 term included before restriction. Euclidean smoothness requires period in , giving in . Independently, the surface gravity for is .
Stationary entropy density
For a local Lagrangian scalar , the stationary prescription is 8
In Einstein gravity the contraction is , giving area divided by , in agreement with the spherical Ryu–Takayanagi surface 9. In Gauss–Bonnet gravity with coefficient inside the Einstein normalization, take , and . The induced section has scalar curvature . The stationary entropy density is times 10. Hence
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, . Thus gives . At boundary time , the map gives , so the sharp radius gives . Write . In the common variable ,
Both give . In that variable the bulk prescription minus the CFT prescription is .
The tube and the algebra it generates
The spatial cutoff applied for every defines a timelike tube in the diamond. It contains the entire open axis segment . A point is spacelike to that segment precisely when , with the usual open-region convention for causal complements. By inclusion, the double causal complement of the tube has interior .
The timelike envelope can also be found directly. For each , take two axis points in , one strictly to its timelike past and one strictly to its timelike future. The line segments through 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 in the timelike envelope of . Conversely, a future timelike curve between points of remains in the causally convex diamond.
Under the hypotheses of the applicable timelike-tube theorem 7, this gives . The smaller diamond of radius shares the tube's spatial section at , 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.