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Asymptotic maximal graph equation and coefficients
PDF p. 14: §3.2.1, divergence equation and L
Statement
Fix and take the family of candidate sections and normalized stationary end coordinates in the uniform asymptotic slope result. In particular, the sections are assumed to exist, are smooth and spacelike and have zero mean curvature; the differentiated end and graph-slope estimates there hold uniformly for . Write , , , and let indices range over in the coordinates . Then, on a common sufficiently distant end, satisfies Moreover this equation can be written , where , , and , uniformly for . These estimates mean bounds by constants independent of on a common end; the constants and radius may depend on . The function in this equation is distinct from the stationary norm .
Statement references
Facts & Assumptions
In the normalized stationary coordinates, the graph is and the spacelike graph has zero mean curvature. With the supplied sign convention, the mean curvature is . Stationary maximal graphs and normalized graph heights Spacelike sections, maximality and lapse–shift data Stationary Lorentzian data and tensor conventions
Uniformly on a common end, , , and ; the subscript means that each spatial derivative through order five gains the corresponding inverse power of . Asymptotically flat positive-q ends and cylindrical limit
Uniformly on a common end, and the graph is spacelike. Uniform asymptotic slope bound
On a smooth time-oriented Lorentzian four-manifold with its Levi–Civita connection, the metric density gives for a smooth vector field in a smooth chart. The derivative of the metric density and the chart formula for the divergence of a vector field
If is continuously differentiable on an open interval containing , then . The fundamental theorem of calculus and integration by parts
If is totally differentiable at and is totally differentiable at , then . The chain rule for total derivatives: D(g∘ f)(a)=Dg(f(a))∘ Df(a)
Let and . If are continuous and for and every , then satisfies for . Leibniz's rule on a compact rectangle: an interior parameter derivative with a continuous extension may be passed through a Riemann integral
The inherited stationary graph data supply an original stationary Lorentzian metric , normalized Ernst potential, pole with , and smooth stationary Harrison one-form with on a domain containing the exterior; the transformed metric is . For these data the Harrison Lorentzian-algebra result gives and . The graph coordinates have and , with and constant in spacetime. Stationary maximal graphs and normalized graph heights Invertibility, Lorentz signature and stationary norm
Proof
Given: The candidate family and normalized end coordinates in the Statement.
Goal: Derive the divergence equation and the stated uniform coefficient bounds.
By [F8], the Harrison stationarity result applies to the supplied data on the end and gives . The local flow of translates with the spatial coordinates fixed, so the flow definition of the metric Lie derivative makes every component of independent of . Since , the components in the normalized coordinates are independent of as well. Set and . The spacelike graph has timelike normal covector , so . Its future unit normal has components . Extend this normal off the graph using the same formula and the time-independent function . The mean curvature vanishes exactly when : differentiating shows the normal-normal contribution to the ambient divergence vanishes. Applying [F4] to the smooth extended normal gives . Time independence removes the time derivative, and . This proves the displayed divergence equation.
Write and define and . The metric estimates and matrix inversion give , , , and . For , , the slope bound implies uniformly; hence it is bounded away from zero on a common larger end. Direct differentiation of the displayed rational expression, holding fixed for spatial derivatives, gives and uniformly on this segment. Also and . These estimates use only the first spatial derivatives of the metric bounds and the explicit factors , with .
Define . By step 2.1, for each fixed and , the curve is smooth on an open interval containing . The chain rule [F6] gives its derivative as . Applying [F5] componentwise gives . The same identity holds for nearby wherever the segment has .
Fix on the common end and . For each spatial index , hold the other coordinates and fixed. Positivity of for and smoothness give a sufficiently small closed interval containing in its interior on which for every . On this rectangle the integrand and its derivative are continuous, so [F7] applies with integration interval . Consequently, with held fixed, . The uniform pointwise bound in step 2.1 makes this after summing over ; the auxiliary interval need not be uniform in .
Apply the chain rule [F6] to . The divergence equation becomes , with the second derivative holding fixed. Differentiating the identity in step 3.1 at fixed and using step 4.1 yields , with , with held fixed in that derivative, and . Steps 2.1 and 4.1 give , and , uniformly in . This specifies one admissible choice of the coefficients; the divergence equation itself is independent of that choice.
Source notes
The article citation attributes the original equation and estimates. The proof uses the declared end and slope results and the displayed coordinate calculation, without using the article's claim as a premise.
Depends on
- Uniform asymptotic slope bound
- Asymptotically flat positive-q ends and cylindrical limit
- Invertibility, Lorentz signature and stationary norm
- Stationary maximal graphs and normalized graph heights
- Spacelike sections, maximality and lapse–shift data
- Stationary Lorentzian data and tensor conventions
- The derivative of the metric density and the chart formula for the divergence of a vector field
- The fundamental theorem of calculus and integration by parts
- The chain rule for total derivatives: D(g∘ f)(a)=Dg(f(a))∘ Df(a)
- Leibniz's rule on a compact rectangle: an interior parameter derivative with a continuous extension may be passed through a Riemann integral
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Sources
- The uniqueness of smooth stationary black holes · PDF page 14, §3.2.1, divergence equation and L