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Stationary end normalization from quotient compactification

Statement

Work in ZFC. Let a smooth stationary Ricci-flat four-end have T=∂t, g00=−1+2M/r+O6(r−2), g0i=O6(r−2), gij=δij+O6(r−1), with M>0. Choose the far tail where T is future timelike. There is a stationary end chart (t′,y) for the same field T with R=∣y∣, g00=−1+2M/R+O∞(R−2), gij=δij+O∞(R−1), and g0i=−2ϵijkSjyk/R3+O∞(R−3) for a fixed vector S. Here O∞ means every finite differentiated order. Relative to the original end this is a spatial end diffeomorphism and an exact stationary time change. The coefficient S is the ADM spin in the sign convention k=−g(∇n,⋅) and normalization (8π)−1∫(k−tr⁡k h)(A×y,ν). No new slice maximality is asserted.

The spatial chart can be chosen as y=ξ/∣ξ∣2, where ξ are orthonormal normal coordinates centered at the added point i for the analytic compactified quotient metric γ=ΩD2hˉ. Here V=g(T,T), hquot=g−g(T,⋅)⊗g(T,⋅)/V on the orbit space, hˉ=(−V)hquot, and ΩD is the potential-defined factor (17) of Dain. This factor and metric satisfy (18)–(19), with ΩD∈C2,α and γ∈C4,α for some 0<α<1, before applying the analytic compactification theorem; γ and ΩD are then analytic in ξ. These properties hold for the same chart (t′,y) asserted above.

Facts & Assumptions

[F2]

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

[F3]

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.

[F4]

A smooth embedded spacelike hypersurface in a time-oriented Lorentzian four-manifold has a unique smooth future unit normal n, a smooth induced metric h and the smooth symmetric second fundamental form K(U,W)=g(∇Un,W). The Statement uses the opposite convention k=−K. The future unit normal, induced metric and second fundamental form of a spacelike hypersurface

[F5]

Ricci-flatness means that the Ricci tensor of the metric-selected connection vanishes. Orthonormal normal coordinates for the compactified Riemannian quotient metric at i are the inverse exponential map expressed in an ordered orthonormal basis of the tangent space at i; 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.

1.1F1F2F3F5

Put V=g(T,T), ai=g0i/V, hij=gij−g0ig0j/V, and hˉ=(−V)h. The given bounds yield a=O6(r−2), h=δ+O6(r−1) and V+1=O6(r−1). The stationary vacuum twist equation gives a normalized twist with twice-differentiated decay on this spherical tail: its derivative is a contraction of T,∇T and the volume form, hence O(r−3); its additive limit is set to zero. Thus the local-at-infinity hypotheses of source 0 hold with any 1/2<α<1. Import its arbitrary finite-order expansions and Cm conformal quotient compactification, choosing m sufficiently large.

2.1F3F5step 1.1

In the inverted compact coordinates let ρ=1/r, rescaled potentials ΦM,ΦS and Q=ΦM2+ΦS2. The source mass coefficient is nonzero, so Q(i)>0. Dain's potential-defined factor is ΩD=ρ2 2Q/[B02(1+4ρ2Q+1)], with B02=Q(i). Its ratio to ρ2 is Cm, positive and one at i. It therefore preserves Cm compactified regularity and the conformal Hessian normalization. This supplies Dain's actual C4,α/C2,α hypotheses, rather than merely assuming them. Import source 1 Theorem2.1 to obtain analytic quotient fields and use its orthonormal normal coordinates x=ξ. In this notation γ=ΩD2hˉ, with hˉ=(−V)hquot 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.

3.1F1F3step 2.1

Source 1 Lemma2.5 constructs the convergent radial connection βi=ϵijkf1j(x)xk+ρ−1ϵijkf2j(x)xk. Set C0=f2(0) and invert to y=x/ρ2. The leading covector is radial-orthogonal, so the reflection part of the inversion differential leaves it unchanged; its physical components are βi=ϵijkC0jyk/R3+O∞(R−3). The convergent radial/angular expansions justify every finite derivative bound. Converting the source +−−− convention to −+++ gives g0i=−λβi, with λ=1+O∞(R−1). Define S=C0/2 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 D2y=O(r−2). Integrating radially and comparing angles yields y=Q0xold+O(log⁡r), Dy=Q0+O(r−1), with Q0 orthogonal. Thus R/r→1. The scalar limit r(V+1)/2=M identifies the new leading mass with the old one; convergence of the new radial expansion supplies its O∞(R−2) remainder.

4.1F1F2F3F4step 3.1

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 T. The new section Σ={t′=0} is a smooth embedded hypersurface because it is a coordinate slice. Hereafter hij=gij∣Σ denotes its induced metric, rather than the quotient metric in step 1.1. Step 3.1 gives hij=δij+O∞(R−1). Increase the tail radius until ∥h−δ∥op≤1/2 in Euclidean coordinates. Then hijvivj≥∣v∣2/2 for every tangent vector v, so Σ is spacelike. The ambient tail is smooth and time-oriented, with T future timelike; hence all hypotheses of [F4] hold. It supplies the smooth future unit normal n and second fundamental form K, and the Statement's k is −K. Put Xi=g0i, Xi=hijXj and N=(−g00+hijXiXj)1/2. These fields are smooth, N=1+O∞(R−1)>0, and n=N−1(T−Xi∂yi): this vector is unit, orthogonal to the slice, and future directed since g(T,n)=−N<0.

5.1F1F4step 3.1step 4.1∎

Let DUW be the tangential projection of ∇UW. Ambient metric compatibility and torsion freedom imply the same properties for D with respect to h, so D is the induced metric connection. Expanding LTg=0 by metric compatibility and torsion freedom and substituting T=Nn+X gives 0=2NKij+DiXj+DjXi on tangential pairs; derivatives of N multiply n and pair to zero. Thus kij=−Kij=(DiXj+DjXi)/(2N) in exactly the Statement's convention. By steps 3.1 and 4.1 its leading term is 3[(S×y)iyj+(S×y)jyi]/R5, with O∞(R−4) remainder, and its leading trace vanishes. Pair k−tr⁡hk h with A×y and the outward h-unit normal to a coordinate sphere and integrate using its h-area measure. Writing ω=y/R, the identity ∫S2ωiωj dω=(4π/3)δij gives ADM angular momentum A⋅S after multiplication by (8π)−1. The normal and area corrections are relative O(R−1), and the O(R−4) tensor remainder contributes O(R−1), so all errors vanish in the limit. This fixes the physical spin coefficient and the exact AIK factor two.

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External dependencies

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

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.

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

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