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Asymptotically flat positive-q ends and cylindrical limit
PDF p. 6: §1.4; PDF p. 12: equation (3.1)
Statement
Work in the inherited ZFC setting, including the Axiom of Choice. Adopt the stationary vacuum model and regular stationary spacetime data with a mass-one stationary Cartesian end , , and . Assume also that the original smooth spacelike maximal exterior section is supplied, with end coordinates and an ADM mass limit that exists and equals one, as required by the mass-one normalization. Use the supplied normalized Ernst potential , pole with , and Harrison one-form family with the radial choice required by the component estimates. Put and , and use the corresponding transformed metric for on the sufficiently distant end.
For every set , and . In these coordinates, with index denoting , Here means that spatial Cartesian derivatives of order are bounded by . For any fixed , the constants and one end radius can be chosen uniformly for ; they may depend on . The region is exactly , and therefore recedes in the original coordinates as for fixed . These component bounds express asymptotic flatness in the stated stationary end chart.
At , the induced metric on each constant- section of the distant end is asymptotic to in the coordinates and : its components and their derivatives through order five in and smooth angular charts differ from those of this product by . Here is the unit round metric induced by the Euclidean inner product on . Thus these sections have a cylindrical end, rather than an asymptotically Euclidean end, and the areas of their coordinate spheres tend to .
For this comparison, an asymptotically Euclidean spatial end means a neighborhood of the same infinity admitting an exterior chart , , in which uniformly in angle as . This metric condition is necessary, in particular, for a fixed-chart asymptotically Euclidean ADM end; no ADM mass convergence or special leading expansion is asserted here.
For an additional positive-parameter case, assume also that the specified exterior section of the regular-spacetime data is maximal for the original metric . This maximality is a hypothesis on that specified physical section; no identification with the supplied maximal section above is assumed. Replace the radial-choice requirement above by the smooth global primitive supplied by Closedness, periods and smooth global choice of W0, with its pole and normalization and under its additional standing hypothesis . Then the same positive- normalized component estimates, uniformity on every and recession statement hold. This additional positive-parameter conclusion requires only its spatial bounds , not equality with the exact radial integral. The zero-parameter cylindrical conclusions above retain the radial-choice hypotheses already stated.
Statement references
Stationary vacuum model and asymptotic normalization
Regular non-degenerate stationary vacuum spacetime
Mass-one convention and Harrison denominator
Single-potential construction of the Harrison one-form family
Stationary Harrison one-form and metric
Killing two-form and normalized Ernst notation
The exterior derivative by the invariant vector-field formula
Differentiated asymptotic bounds and parameter uniformity
Uniform denominator and one-form estimates
Uniform transformed component estimates
Surface area and flux on a sphere, with scalar integrals on a hemisphere
Riemannian volume is the radon measure of the riemannian density
Riemannian distance on a connected manifold
A specified asymptotically Euclidean ADM end
The pullback of a covariant tensor field
The chain rule for total derivatives: D(g∘ f)(a)=Dg(f(a))∘ Df(a)
Sum, product, quotient, and chain rules from difference quotients
A closed three-dimensional ball of radius r≥0 has volume 4π r³/3
Facts & Assumptions
The regular data are formulated in ZFC, so the Axiom of Choice and hence Countable Choice are available for the round-sphere and volume-measure interfaces below. The Axiom of Choice The stated model and regular data supply the mass-one stationary end and the specified stationary chart; the normalization and one-form definitions specify the conditional potential, pole, denominator and selected family. Stationary vacuum model and asymptotic normalization Regular non-degenerate stationary vacuum spacetime Mass-one convention and Harrison denominator Single-potential construction of the Harrison one-form family
The original smooth spacelike maximal exterior section is supplied, and the ADM mass limit of its end in the stated coordinates exists and equals one. These are assumed section and normalization data, not existence or mass-convergence conclusions. Mass-one convention and Harrison denominator Uniform transformed component estimates
For the stated data and radial choice, the denominator estimate gives bounded above and below by positive constants uniformly on , and on a common sufficiently distant end. Uniform denominator and one-form estimates
On that end, with and , the component estimates give , , and , uniformly for . The weighted derivative notation is the one specified in the supplier. Uniform transformed component estimates Differentiated asymptotic bounds and parameter uniformity
The unit round sphere is the compact sphere with its induced Euclidean metric; it has diameter , and its area is . The round-sphere supplier's Countable Choice premise follows from [A1]. Round sphere model geometry Surface area and flux on a sphere, with scalar integrals on a hemisphere
A positive-definite metric has coordinate density ; this gives surface area when and volume when . Under the inherited Countable Choice, its Riemannian volume measure is the Radon measure of this density, and metric balls are Borel. Riemannian length integrates along piecewise curves, and intrinsic distance is the infimum of these lengths with the curves confined to the specified connected end. Riemannian volume density Riemannian volume is the radon measure of the riemannian density Riemannian speed and length Riemannian distance on a connected manifold
Pulling back a covariant tensor evaluates it on the differentials of the coordinate map. The total-derivative chain rule and the coordinate-line product and quotient rules apply repeatedly to the smooth coordinate maps and component functions used below. The pullback of a covariant tensor field The chain rule for total derivatives: D(g∘ f)(a)=Dg(f(a))∘ Df(a) Sum, product, quotient, and chain rules from difference quotients
The published fixed-chart ADM-end definition requires , with constant and , as well as a separate condition on . Its metric therefore satisfies the weaker metric condition specified in the Statement. The argument below excludes even that weaker condition in every chart representing this same infinity; it does not infer the stronger ADM expansion from the positive- estimates. A specified asymptotically Euclidean ADM end
A Euclidean three-ball of radius has volume . A closed three-dimensional ball of radius r≥0 has volume 4π r³/3
The supplied normalized primitive satisfies and , and its family is . The family definition's local contraction calculation gives . Single-potential construction of the Harrison one-form family The Ernst interface uses the torsion-free metric-compatible connection, , and ; its local justification gives antisymmetry of and . Killing two-form and normalized Ernst notation
For a smooth one-form , exterior differentiation is . The exterior derivative by the invariant vector-field formula The Harrison one-form interface requires stationarity, , and . Its corresponding metric is on . Stationary Harrison one-form and metric
For the additional case, the specified exterior section of the regular-spacetime data is assumed maximal for ; this does not identify it with . Together with the regular stationary vacuum model, mass one and , this matches the hypotheses of the global primitive theorem. Use that theorem's supplied pole and normalization, in the unchanged original stationary chart. It supplies one smooth stationary with and the normalized contraction. Closedness, periods and smooth global choice of W0 The mass-one Ernst estimate gives and , independently of which primitive is chosen. Mass-one Ernst and radial primitive asymptotics For a supplied Harrison one-form the exact original-chart metric components are those of the component-identity theorem; no radial-gauge condition is imposed by that theorem. Coordinate components of the transformed metric
Proof
Given: The model, end, supplied original maximal exterior section and its existing ADM mass-one limit, pole, potential, selected one-form and transformed metrics in the Statement. In the additional case also assume maximality of the specified exterior section, as stated in [F10].
Goal: Prove the normalized positive- bounds and the zero- cylindrical spatial limit.
First verify the one-form hypotheses needed for the component estimates from the supplied primitive. Taking real and imaginary parts in [F8] gives and . Since , it follows that . In the stationary end chart the coordinate fields commute. With , [F9] therefore gives . Also gives . Thus is stationary there. The Killing condition makes the components of independent of , so the constant-coefficient family in [F8] is stationary for every fixed .
The torsion-free metric-compatible connection in [F8] satisfies . Expanding [F9] for consequently gives . The same exterior-derivative formula is real-linear in the one-form. For fixed its coefficients are constant, so . The contraction identity is already established in [F8]. Together with step 1.1 these are exactly the conditions in [F9]; the corresponding transformed metric in the Statement is the metric specified there. The positivity domain is supplied by [F1]. Thus the one-form hypotheses of the component supplier are established before its estimates are used below, while the given radial choice and section data are retained.
Fix . For , the factors , and their spatial derivatives have bounds controlled by , with each derivative gaining one power of . Since , [F2] gives , , and , with a common radius and constants depending on . For example, has the required differentiated bound.
At , [F2] gives . The error is smaller than the positive leading form for sufficiently large , so a constant- section is spacelike there. With and , . Indeed , and follows by differentiating , so the leading form is exactly the product with the induced round metric in [F3]. On relatively compact angular charts in a finite cover of the sphere, every required derivative of is . Each transformed error component has two coordinate-Jacobian factors. After at most five further derivatives, the chain and product rules express every term as a Cartesian derivative of order of the error, bounded by , times factors bounded by . Thus all these terms are . This proves the cylindrical metric assertion.
For the additional global-choice conclusion fix . The regular model in [A1], mass-one data in [A2], and maximality of the specified exterior section and in [F10] match the global primitive theorem's hypotheses. Apply it with its supplied pole and normalization in the original chart, as in [F10]. The primitive in F10 and its constant-coefficient family in F8 satisfy the one-form conditions by the local calculations in steps 1.1 and 2.1, which use no radial identity. For , the Ernst bounds in F10 give , uniformly in . On a common larger end . Repeated product and reciprocal differentiation using F5 gives . Also uniformly. At the fixed pole, , so and its reciprocal are bounded on . Substitute these estimates into the exact identities in F10. They give , and for this same global primitive. Every derivative assertion follows by the finite coordinate product and reciprocal rules; constants may depend on .
By [F1], , so the coordinate change is invertible. Its inverse Jacobian has and . Applying the tensor transformation law to step 3.1 gives the displayed leading coefficients. Each derivative contributes a factor , and ; all factors are uniformly bounded for . This proves the stated estimates on a common normalized end. The identity gives the region correspondence and its recession.
Restricting the metric in step 3.2 to gives in smooth angular charts. Relative to the positive round metric, the two eigenvalues are , uniformly over the compact sphere. By the determinant density in [F4], the area density is therefore . Integrating and using [F3] gives sphere area , proving the stated limit.
Write for the zero- spatial metric and . Choose so large that on the connected end one has . Fix any . For every piecewise path from to confined to , [F4] gives length at least . Thus its intrinsic ball lies in . The volume density is at most and , so . This proves the linear upper bound without assuming a minimizing curve exists.
Suppose the same infinity admitted the asymptotically Euclidean chart specified in the Statement. Truncate it to an end lying in , with there. Fix with . Any with can be reached from by a spherical arc at radius followed by a radial segment, all in . By [F3], the Euclidean spherical arc has length at most ; the radial segment has length at most . Its -length is at most . Consequently this annulus is contained in the intrinsic ball of centered at with radius , since all these paths are also allowed in . For the annulus contains the Euclidean ball of radius centered at in the chart. The density lower bound and [F7] give . This is a cubic lower bound for radii , contradicting step 4.3, which applies to every fixed center in .
Thus there is no asymptotically Euclidean chart at this infinity even in the weaker metric sense specified, and in particular no fixed-chart ADM end of [F6]. Together with steps 4.1, 3.2 and 4.2 this proves all the normalized positive- estimates, their uniformity and recession, and the cylindrical limit with area . The inherited choice premise is used only through the round-sphere and volume-measure suppliers, not to choose a family of curves in the comparison.
Apply and to the bounds in step 3.3. The tensor transformation law in F5 and give exactly the stated normalized bounds, uniformly on a common end for . The graph of the coordinate change has , so the same region correspondence and recession follow. This proves the additional positive-parameter conclusion for the actual smooth global family while preserving all radial-choice conclusions already proved. No zero-parameter assertion for a different gauge is inferred from this extension.
Source notes
Attribution only: The positive-q transformed ends are asymptotically flat in the normalized coordinates, while the zero-q spatial end is asymptotically cylindrical with limiting area 4π in the mass-one normalization. The proof uses the supplied component and denominator estimates and the declared mathematical interfaces; this article citation is not an imported premise.
Depends on
- Uniform transformed component estimates
- Uniform denominator and one-form estimates
- Mass-one convention and Harrison denominator
- Single-potential construction of the Harrison one-form family
- Regular non-degenerate stationary vacuum spacetime
- Stationary vacuum model and asymptotic normalization
- Differentiated asymptotic bounds and parameter uniformity
- Round sphere model geometry
- Surface area and flux on a sphere, with scalar integrals on a hemisphere
- Riemannian volume density
- Riemannian volume is the radon measure of the riemannian density
- Riemannian speed and length
- Riemannian distance on a connected manifold
- A specified asymptotically Euclidean ADM end
- The pullback of a covariant tensor field
- The chain rule for total derivatives: D(g∘ f)(a)=Dg(f(a))∘ Df(a)
- Sum, product, quotient, and chain rules from difference quotients
- A closed three-dimensional ball of radius r≥0 has volume 4π r³/3
- The Axiom of Choice
- Stationary Harrison one-form and metric
- Killing two-form and normalized Ernst notation
- The exterior derivative by the invariant vector-field formula
- Closedness, periods and smooth global choice of W0
- Mass-one Ernst and radial primitive asymptotics
- Coordinate components of the transformed metric
Used by · 10
- Mean-curvature linearization, weighted regularity and fixed-boundary graph map
- Uniform asymptotic slope bound
- Asymptotic maximal graph equation and coefficients
- Rescaled annular estimates through four derivatives
- Uniform compact graph and positive-lapse estimates
- Causal speed and finite-section-time escape estimates
- Lemma 4.3: localization of the causal cut near S
- Uniform end estimates indexed only by existing admissible slices
- Compact estimates for arbitrary sequences of individually existing slices
- Sequence closedness and completeness without an interval-family premise
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Sources
- The uniqueness of smooth stationary black holes · PDF page 6, Section 1.4; page 12, equation (3.1)