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Stationary end normalization from quotient compactification
Statement
Work in ZFC. Let a smooth stationary Ricci-flat four-end have , , , , with . Choose the far tail where is future timelike. There is a stationary end chart for the same field with , , , and for a fixed vector . Here means every finite differentiated order. Relative to the original end this is a spatial end diffeomorphism and an exact stationary time change. The coefficient is the ADM spin in the sign convention and normalization . No new slice maximality is asserted.
The spatial chart can be chosen as , where are orthonormal normal coordinates centered at the added point for the analytic compactified quotient metric . Here , on the orbit space, , and is the potential-defined factor (17) of Dain. This factor and metric satisfy (18)–(19), with and for some , before applying the analytic compactification theorem; and are then analytic in . These properties hold for the same chart asserted above.
Statement references
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
Killing fields of a Lorentzian metric
Metric compatibility, torsion freedom and the metric-selected connection class
Periods and primitives on a spherical exterior
Differentiated asymptotic bounds and parameter uniformity
The future unit normal, induced metric and second fundamental form of a spacelike hypersurface
The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
Facts & Assumptions
Lorentzian, Killing and connection conventions and differentiated end bounds are fixed. Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model Killing fields of a Lorentzian metric Metric compatibility, torsion freedom and the metric-selected connection class Differentiated asymptotic bounds and parameter uniformity
Work in ZFC; closed one-forms on a spherical tail are exact by the spherical-period interface. The Axiom of Choice Periods and primitives on a spherical exterior
The independent Beig–Schmidt stationary connection–twist curl relation, multipole and conformal-compactification inputs are source 0, and Dain Theorem2.1 and Lemma2.5 are source 1, with their full stated hypotheses and reading limits.
A smooth embedded spacelike hypersurface in a time-oriented Lorentzian four-manifold has a unique smooth future unit normal , a smooth induced metric and the smooth symmetric second fundamental form . The Statement uses the opposite convention . The future unit normal, induced metric and second fundamental form of a spacelike hypersurface
Ricci-flatness means that the Ricci tensor of the metric-selected connection vanishes. Orthonormal normal coordinates for the compactified Riemannian quotient metric at are the inverse exponential map expressed in an ordered orthonormal basis of the tangent space at ; their Countable Choice assumption is included in ZFC. The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors Normal neighborhood and normal coordinate chart
Proof
**Given:**The full hypotheses in the Statement.
Goal: Establish the stated claim with its exact hypotheses.
Put , , , and . The given bounds yield , and . The stationary vacuum twist equation gives a normalized twist with twice-differentiated decay on this spherical tail: its derivative is a contraction of and the volume form, hence ; its additive limit is set to zero. Thus the local-at-infinity hypotheses of source 0 hold with any . Import its arbitrary finite-order expansions and conformal quotient compactification, choosing sufficiently large.
In the inverted compact coordinates let , rescaled potentials and . The source mass coefficient is nonzero, so . Dain's potential-defined factor is , with . Its ratio to is , positive and one at . It therefore preserves compactified regularity and the conformal Hessian normalization. This supplies Dain's actual hypotheses, rather than merely assuming them. Import source 1 Theorem2.1 to obtain analytic quotient fields and use its orthonormal normal coordinates . In this notation , with from step 1.1. The spatial chart is obtained by inversion of precisely these normal coordinates, so the compactification conditions and the chart identity in the Statement refer to the same constructed chart.
Source 1 Lemma2.5 constructs the convergent radial connection . Set and invert to . The leading covector is radial-orthogonal, so the reflection part of the inversion differential leaves it unchanged; its physical components are . The convergent radial/angular expansions justify every finite derivative bound. Converting the source convention to gives , with . Define to obtain the displayed coefficient, without equating differently normalized source spin symbols. The other reconstructed components have the asserted convergent expansions. Both old and new quotient metrics are asymptotically Euclidean, so their coordinate transition has bounded first derivative and inverse; the Christoffel transformation gives . Integrating radially and comparing angles yields , , with orthogonal. Thus . The scalar limit identifies the new leading mass with the old one; convergence of the new radial expansion supplies its remainder.
Both stationary connections reconstruct the same norm/twist/quotient fields. The stationary connection–twist relation in source 0, equations (2.36) and (2.70), therefore gives equal exterior derivatives, so their difference is closed. The spherical-tail exactness of [F2] gives the stationary time gauge; it preserves . The new section is a smooth embedded hypersurface because it is a coordinate slice. Hereafter denotes its induced metric, rather than the quotient metric in step 1.1. Step 3.1 gives . Increase the tail radius until in Euclidean coordinates. Then for every tangent vector , so is spacelike. The ambient tail is smooth and time-oriented, with future timelike; hence all hypotheses of [F4] hold. It supplies the smooth future unit normal and second fundamental form , and the Statement's is . Put , and . These fields are smooth, , and : this vector is unit, orthogonal to the slice, and future directed since .
Let be the tangential projection of . Ambient metric compatibility and torsion freedom imply the same properties for with respect to , so is the induced metric connection. Expanding by metric compatibility and torsion freedom and substituting gives on tangential pairs; derivatives of multiply and pair to zero. Thus in exactly the Statement's convention. By steps 3.1 and 4.1 its leading term is , with remainder, and its leading trace vanishes. Pair with and the outward -unit normal to a coordinate sphere and integrate using its -area measure. Writing , the identity gives ADM angular momentum after multiplication by . The normal and area corrections are relative , and the tensor remainder contributes , so all errors vanish in the limit. This fixes the physical spin coefficient and the exact AIK factor two.
Depends on
- Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
- Killing fields of a Lorentzian metric
- Metric compatibility, torsion freedom and the metric-selected connection class
- Periods and primitives on a spherical exterior
- The Axiom of Choice
- Differentiated asymptotic bounds and parameter uniformity
- The future unit normal, induced metric and second fundamental form of a spacelike hypersurface
- The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
- Normal neighborhood and normal coordinate chart
- R. Beig and B. Schmidt, Time-Independent Gravitational Fields · §2.1 (2.33)–(2.38), p.7; §2.3 (2.70)–(2.72), pp.10–11; §3.1 (3.5), (3.15)–(3.25), pp.17–20; §3.2 (3.51)–(3.52), p.23
- S. Dain, Initial data for stationary space-times near space-like infinity · §2 (17)–(19) and Theorem2.1, p.4; (20), pp.5–6; Lemma2.5 and (36)–(43), pp.7–8
Used by · 5
- Local Kerr rigidity and conditional global identification
- Extending normalized end coordinates while preserving the section
- Mass-one end coordinates on the unchanged maximal section
- A smooth radial primitive can be returned to a weak end gauge
- Equivariant global Harrison primitive under weak original data
Dependency tree · 2 levels
Each result is drawn at its shortest distance from this item. Arrows run from prerequisites to the items that use them; this item has a heavier outline. External source nodes link directly to the cited text. The view shows up to two dependency steps; open a prerequisite to continue.
External dependencies
Stationary vacuum quotient fields on an AF three-end with O2(r^-alpha), 1/2<alpha<1, admit arbitrary finite-order multipole expansions with O-infinity remainders. Inversion and Omega=r^-2 give C^m compactified quotient metric and rescaled mass/twist potentials for arbitrarily high finite m. The stationary connection curl is determined by the twist; changing it by dF changes the stationary time coordinate.
Hypotheses: The use is local at spatial infinity, where the given stationary field is timelike and the quotient is R3 minus a ball. It does not assume a globally timelike field on the black-hole DOC.
Reading limits: Read the stated decomposition, twist, weak-decay, multipole-theorem and conformal-compactification passages in the retained full PDF. No reconstruction or independent review of the elliptic multipole theorem; the 1981 primary reference was not retrieved. The conformal conversion and gauge calculations below are local arguments, not falsely attributed verbatim to this source.
Under the specified potential-defined conformal factor with C2,alpha regularity, C4,alpha conformal quotient metric and Hessian normalization, the quotient fields are analytic. In analytic normal coordinates the radial stationary connection has beta_i=epsilon_ijk f1^j x^k+rho^-1 epsilon_ijk f2^j x^k, with analytic f1,f2.
Hypotheses: Stationary vacuum timelike quotient near spatial infinity; nonzero mass normalization B² and exactly the conformal conditions (17)–(19). The source signature is +--- and the new slice is not asserted maximal.
Reading limits: Read the exact hypotheses and Theorem2.1, fields/conformal formulas and Lemma2.5 in the retained PDF, plus the nonmaximal-slice qualification. The analytic existence theorems are imported; no proof reconstruction or primary Beig–Simon1981 reading is claimed. Target signature and spin normalization are converted explicitly below.
Sources
- R. Beig and B. Schmidt, Time-Independent Gravitational Fields · §2.1 (2.33)–(2.38), p.7; §2.3 (2.70)–(2.72), pp.10–11; §3.1 (3.5), (3.15)–(3.25), pp.17–20; §3.2 (3.51)–(3.52), p.23
- S. Dain, Initial data for stationary space-times near space-like infinity · §2 (17)–(19) and Theorem2.1, p.4; (20), pp.5–6; Lemma2.5 and (36)–(43), pp.7–8