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Ernst and self-dual curvature data in the AIK convention

Definition

For the AIK perturbative GR/SBS package, let U=M~ be the open neighborhood of Σ0∩E‾ constructed in AIK §2.1. Use the normalized smooth Ernst potential σ=f+iψ on U, with f=−g(T,T), dσ=2ιTF and σ→1 at infinity. Here Fab=∇aTb=12(dT♭)ab, F=F+i⋆gF, F2=FabFab uses complex bilinear contraction, and the spacetime orientation fixes ϵ and ⋆g. Existence on U is imported explicitly in External input; the definition of a potential alone asserts no existence.

For normalization, designate the product end Uend=Φ0(I×E2R1)⊂U, where I=(−ε0,ε0) and R1,ε0 are from the AIK §2.1 construction. In its source coordinates (t,x), put y=x when dt∧dx1∧dx2∧dx3 is positive for the given spacetime orientation; otherwise put y=(−x1,x2,x3). Use (t,y) as the designated normalization chart, so dt∧dy1∧dy2∧dy3 is positive, ∣y∣=∣x∣ and T=∂t. The GR/SBS source chart and its component hypotheses remain the original (t,x) chart.

Write R(X,Y)Z=∇X∇YZ−∇Y∇XZ−∇[X,Y]Z for the stationary-data curvature operator. Define the source covariant array by RAIK(X,Y,Z,W)=g(X,R(Z,W)Y),RabcdAIK=gaeRebcd. This fixes all four slots and the sign explicitly; its identification with the AIK convention uses the curvature formula in §5.1 after (5.10), rather than (2.16) or a contraction with T alone. Define Rabcd=RabcdAIK+i2ϵcdefRabefAIK,Iabcd=14(gacgbd−gadgbc+iϵabcd). Thus the Hodge operation on curvature is in its last alternating pair, all raised indices use this g, and I is the displayed covariant four-tensor. The source identity (2.20), ∇μFab=TνRνμab, is an imported identity in this convention, not a definition of the full curvature array or a locally proved differential identity. No conversion to a different curvature convention is asserted.

Facts & Assumptions

[F1]

AIK perturbative global regularity and bifurcation package specifies the GR/SBS source hypotheses and background geometry. Stationary Lorentzian data and tensor conventions provides the connection, curvature operator, metric duality and tensor types.

[F2]

Killing two-form and normalized Ernst notation gives the Killing two-form, Ernst equation and normalized-potential terminology, and Complex self-dual forms and metric-dependent contraction gives the complex-linear Hodge star and complex bilinear contractions. Neither definition supplies potential existence.

[F3]

Import the neighborhood potential, its slice normalization and the stationary product end of the neighborhood construction from AIK §2.1 and §2.3, under exactly the GR/SBS hypotheses in [F1], as specified by the first statement-bearing source record and External input.

[F4]

Import the source curvature convention from the unnumbered formula after AIK (5.10), and (2.20) in that convention, from AIK §5.1 and §2.3, with the precise hypotheses in the second statement-bearing source record.

Justification

Given: The GR/SBS data, the declared mathematical conventions and the two explicit source inputs.

Goal: Establish the displayed constructions and their compatibility with the source convention.

1.1 Since F is alternating and the connection is torsion-free, (dT♭)ab=∇aTb−∇bTa=2Fab. The GR/SBS data meet the hypotheses of the imported neighborhood-potential input [F3], so σ is a supplied smooth function on U, with the stated real part, differential and slice normalization. The same source construction supplies Uend=Φ0(I×E2R1)⊂U with T=∂t. This end is connected, so the nowhere-zero form dt∧dx1∧dx2∧dx3 has constant orientation sign there. In the negative case the fixed reflection in the Definition multiplies that form by −1; in the positive case the chart is unchanged. Both choices are smooth coordinate diffeomorphisms onto I×E2R1, preserve the radius and t, and give the positive coordinate volume form required by [F2]. This changes only the designated coordinates, not the spacetime orientation, Hodge star or potential. By alternation, Ta∇aσ=2TaTbFba=0. Since T=∂t on this product end, σ(t,y)=σ(0,y) for every t∈I. For any δ>0, the imported slice limit gives R>2R1 such that ∣σ(0,x)−1∣<δ whenever ∣x∣>R. The equality of radii and the independence of t therefore give ∣σ(t,y)−1∣<δ for every t∈I and ∣y∣>R, exactly the uniform end normalization of [F2]. This uses the imported existence result, without claiming a local topological or potential-existence proof. [F1, F2, F3, algebra]

1.2 For any smooth local frame (va), substitution of the curvature operator of [F1] into the covariant array gives g(va,(∇vc∇vd−∇vd∇vc−∇[vc,vd])vb), exactly the source convention in [F4]. Thus this identification fixes every slot without inferring the full array from a contraction with T. The array is a smooth covariant tensor and is alternating in its last two slots because R(Z,W)=−R(W,Z) directly from its definition. Applying the smooth Hodge operation to those two slots is therefore intrinsic and well defined. [F1, F2, F4, algebra]

2.1 Metric tensor products, the oriented metric volume form, contractions and constant complex linear combinations preserve tensor type and smoothness. Hence the displayed R and I are smooth covariant four-tensors independent of the frame, and the displayed scalar contraction has precisely the complex bilinear meaning of [F2]. Together with the supplied smooth potential this proves well-definedness of the package. Identity (2.20) retains its imported status [F4]; it is not used to infer its own curvature convention or to prove potential existence. [F1, F2, F4, step 1.1, step 1.2] ∎

External input

The first statement-bearing AIK source record supplies the neighborhood potential, its normalization and the stationary product end in the neighborhood construction under GR/SBS. Its source argument is accepted as an external input; no local potential-existence proof is claimed.

The second statement-bearing AIK source record supplies the explicit curvature convention and identity (2.20). The identification with the stationary-data operator and the well-definedness of the displayed constructions are justified locally above. This definition imports no global rigidity theorem.

Depends on

Used by · 2

Dependency tree · 2 levels

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External dependencies

S. Alexakis, A. D. Ionescu and S. Klainerman, Uniqueness of smooth stationary black holes in vacuum: small perturbations of the Kerr spaces · Section 1.1 setup and GR/SBS; section 2.1 neighborhood construction preceding (2.3); section 2.3, (2.13)–(2.15) and the potential-existence paragraph immediately before (2.16). PDF v1 pp. 4–7 and 8–9.

Under GR/SBS there is a smooth complex potential $\sigma$ on the section 2.1 neighborhood $\widetilde M$ of $\Sigma^0\cap\overline E$, satisfying $d\sigma=2\iota_T\mathcal F$, $\Re\sigma=-g(T,T)$, and $\sigma\to1$ at spatial infinity on $\Sigma^0$. In the section 2.1 construction, $\Phi_1:(-\varepsilon_0,\varepsilon_0)\times E_{1-\varepsilon_0}\to\widetilde M$ is a diffeomorphism and agrees with $\Phi_0$ on $(-\varepsilon_0,\varepsilon_0)\times E_{2R_1}$, where $T=\partial_t$.

Hypotheses: The smooth oriented time-oriented Ricci-flat four-dimensional stationary data, source partial Cauchy surface, stationary asymptotic end and GR/SBS conditions of def-author-ad064c44a1cc-perturbative-gr-sbs. Use the neighborhood constructed in section 2.1; PK and maximality are not required for this input.

Reading limits: Consulted the arXiv v1 HTML section 1.1 setup and GR/SBS, section 2.1 neighborhood construction, and section 2.3 (2.13)–(2.17) with the intervening existence paragraph; cross-checked that paragraph in the PDF text on p. 9. Import restricted to the neighborhood potential and slice normalization. The source also gives an exterior extension, which is not needed here. Its topology and potential-existence argument are accepted as an external input, not locally reconstructed; no rigidity proof was reviewed. For the present orientation repair, re-read the HTML section 2.1 construction between (2.2) and (2.3), including the product domain and agreement with the stationary end, and the section 2.3 potential paragraph before (2.16). The preceding PDF-reading statements are retained historical source metadata; no new PDF inspection or review of the source proof is claimed in this repair. The orientation-compatible coordinate choice is proved locally.

S. Alexakis, A. D. Ionescu and S. Klainerman, Uniqueness of smooth stationary black holes in vacuum: small perturbations of the Kerr spaces · Section 2.3, (2.13), (2.16)–(2.17), (2.20), PDF pp. 8–9; section 5.1, (5.9)–(5.10) and the immediately following unnumbered curvature formula, PDF p. 27.

The covariant curvature convention is $R^{\rm AIK}(X,Y,Z,W)=g(X,(\nabla_Z\nabla_W-\nabla_W\nabla_Z-\nabla_{[Z,W]})Y)$. Equations (2.16)–(2.17) set $\mathcal R_{ab cd}=R^{\rm AIK}_{ab cd}+\frac{i}{2}\epsilon_{cd}{}^{ef}R^{\rm AIK}_{ab ef}$ and $\mathcal I_{ab cd}=\frac14(g_{ac}g_{bd}-g_{ad}g_{bc}+i\epsilon_{abcd})$; in vacuum (2.20) states $\nabla_\mu\mathcal F_{ab}=T^\nu\mathcal R_{\nu\mu ab}$.

Hypotheses: For the curvature convention and algebraic definitions, a smooth oriented Lorentzian four-metric with its Levi–Civita connection; the covariant slots follow the arbitrary-frame convention displayed in section 5.1. For (2.20), require Ricci-flatness and a smooth Killing field, with the Hodge convention (2.13). These conditions hold in the declared GR/SBS package.

Reading limits: Read the indicated HTML equations and the defining first line of the unnumbered curvature formula in section 5.1 after (5.10); cross-checked the latter in the PDF text on p. 27. The PDF screenshot service failed, so no image inspection is claimed. This imports the convention and (2.20), without reconstructing the Ricci identity or reviewing the continuation argument around the curvature formula.

Sources