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Radial barrier, absorption and height decay
PDF p. 14: §3.2.1; (3.6)–(3.7); PDF p. 15: §3.2.1; (3.6)–(3.7)
Statement
Fix and . Assume the candidate family, normalized Cartesian ends and uniform estimates of Asymptotic maximal graph equation and coefficients and Uniform asymptotic slope bound. In particular, each normalized graph height tends to zero as , uniformly in direction for that fixed ; the sections are assumed to exist. Write , using the coefficients supplied by the graph equation, evaluated on the given graph.
There are and , independent of , such that for . Fix any and put . There is a constant independent of and such that, for , . If is a uniform constant in , then . Consequently, for a fixed sufficiently large , on , with independent of .
Facts & Assumptions
On a common end the graph equation is , with , and uniformly in . The principal coefficient is uniformly positive definite on a sufficiently distant common end. Asymptotic maximal graph equation and coefficients
On a common end the normalized slope satisfies uniformly in . Uniform asymptotic slope bound
The normalized end uses , and the graph-height normalization requires convergence to zero uniformly in angle for each fixed parameter. Stationary maximal graphs and normalized graph heights
Proof
Given: The family and hypotheses in the Statement.
Goal: Establish the radial barrier, comparison, absorption inequality and uniform height decay.
In three Cartesian spatial dimensions, direct differentiation gives , while and . The coefficient errors in [F1] therefore contribute at most . Since , increasing the common radius gives the claimed strictly negative bound, uniformly in .
Fix beyond that radius and choose , with from [F1]. Set . Then for : indeed is strictly greater than because and . At the inner sphere . For each fixed , [F3] and imply that on a sufficiently distant outer sphere this difference is at most any prescribed . On the closed intervening annulus it cannot attain a positive interior maximum exceeding : at such a maximum the gradient vanishes and the Hessian is negative semidefinite, so positive definiteness of gives , a contradiction. Letting the outer radius tend to infinity and then proves the comparison bound.
Along each radial segment from radius to , [F2] bounds the height change by . Taking the maximum over directions and applying step 2.1 at radius yields the stated absorption inequality.
Since , the inequality in step 3.1 gives a bound on independent of once the common is fixed. Substitution into step 2.1 gives the asserted bound.
Source notes
The article reference attributes the original estimates. The proof does not use that reference as a premise; the comparison argument is given on bounded annuli and uses each individual graph's end limit, not a uniform rate of convergence in .
Depends on
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Sources
- The uniqueness of smooth stationary black holes · PDF pages 14–15, §3.2.1, equations (3.5)–(3.7)