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Mars–Simon tensor and its smooth weighted extension

Definition

Use the preceding AIK-convention tensor and potential data. On U′={σ≠1} define Qabcd=(1−σ)−1(FabFcd−13F2Iabcd),S=R+6Q. This S is the source's Mars–Simon tensor. Its weighted version is the globally smooth covariant four-tensor W=(1−σ)R+6(F⊗F−13F2I). On U′ it equals (1−σ)S. At points where σ=1, W is defined by this polynomial formula, not by dividing by zero. No vanishing, Kerr-characterization, Weyl-symmetry or propagation theorem is inferred from these formulas alone.

Facts & Assumptions

[F1]

Ernst and self-dual curvature data in the AIK convention supplies the smooth potential and source-convention tensors on their potential domain.

[F2]

Complex self-dual forms and metric-dependent contraction supplies complex two-forms, their real and imaginary parts, and the complex bilinear contraction convention.

[F3]

Tensor products and contractions of smooth tensor fields are smooth supplies tensor products and contractions of smooth real tensor fields and their smoothness. Apply these operations complex bilinearly, by taking real and imaginary parts as in [F2].

Justification

Given: The smooth potential and tensor fields of [F1], the complex convention of [F2], and the real tensor operations of [F3].

1.1 For smooth real tensor fields A,B,C,D, define the complex tensor product by (A+iB)⊗(C+iD)=(A⊗C−B⊗D)+i(A⊗D+B⊗C). Bilinearity of the real tensor product makes this intrinsic and complex bilinear; [F3] makes each real and imaginary component smooth. Contraction extends by the same real and imaginary decomposition. Smooth scalar multiplication and sums are smooth componentwise, so these operations apply to all products and contractions in the Definition. [F1, F2, F3, algebra]

2.1 The set U′ is open because σ is continuous. There (1−σ)−1 is smooth: for 1−σ=x+iy, its real and imaginary components are x/(x2+y2) and −y/(x2+y2), with nonzero denominator. Thus the displayed Q and S are smooth on U′. Multiplication by 1−σ gives exactly W. Its polynomial formula uses only smooth products, contractions and sums, so it defines a smooth covariant four-tensor throughout the potential domain, including σ=1. This proves the weighted identity and well-definedness without assuming any rigidity conclusion. [F1, F2, F3, step 1.1, algebra] ∎

Depends on

Used by · 3

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 2.3, equations (2.18)–(2.19), with (2.13), (2.16)–(2.17) and the weighted-smoothness sentence immediately after (2.19).

On $U\cap\{\sigma\ne1\}$, (2.18) defines $\mathcal Q=(1-\sigma)^{-1}(\mathcal F\otimes\mathcal F-\mathcal F^2\mathcal I/3)$ and (2.19) names $\mathcal S=\mathcal R+6\mathcal Q$ the Mars–Simon tensor; the next sentence asserts that $(1-\sigma)\mathcal S$ extends smoothly over $U=\widetilde M$.

Hypotheses: The source GR/SBS stationary Ricci-flat four-manifold and its smooth normalized Ernst potential on $U=\widetilde M$, supplied by def-author-ad064c44a1cc-ernst-curvature-package, with AIK Hodge, curvature and bilinear-contraction conventions. Division requires $\sigma\ne1$. PK smallness is unnecessary for these definitions and their weighted extension.

Reading limits: Read arXiv v1 HTML section 2.3, (2.13)–(2.19), the intervening potential-domain paragraph and the sentence following (2.19); checked section 1.1 GR/SBS and section 2.1 neighborhood construction. HTML renders the weighted sentence with a malformed tensor glyph. Formula coefficients are explicit in (2.18)–(2.19); smoothness is justified locally below. No PDF image inspection or rigidity-proof review is claimed.

Sources