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Stable-horizon flux-energy and area-charge inequalities
PDF p. 27: Proof of Theorem 4.2; proof of Corollary 4.1
Statement
Assume the regular non-degenerate stationary vacuum model, with original exterior section maximal, ADM mass normalized to one and stationary Killing field nontrivial on its bifurcation sphere . Fix and an individually admissible smooth spacelike maximal section as in Nonnegative principal eigenvalue of the horizon stability operator, with a smooth spacelike extension and outward normal-graph tube as in Horizon expansion variation and Einstein–Maxwell curvature. Work in ZFC. Let be the Harrison metric and electromagnetic two-form, and let and be the induced metric and oriented area form. Define electric and magnetic flux densities by and . Then Here . In particular, both inequalities hold for sufficiently small positive under the same hypotheses. The second inequality follows directly from the same stability equation and Gauss–Bonnet.
Facts & Assumptions
Given: The model, parameter, admissible section, extension and graph data in the Statement.
Goal: Prove the two displayed inequalities.
The regularity and normalization conventions and the meaning of a spacelike maximal section are those of Regular non-degenerate stationary vacuum spacetime, Mass-one convention and Harrison denominator and Spacelike sections, maximality and lapse–shift data, in the conditional model Stationary vacuum model and asymptotic normalization. Work in ZFC. The Axiom of Choice
The horizon and surface-data definitions supply the smooth positive surface measure, null gauge, flux densities and intrinsic gradient, divergence, Laplacian and Gauss curvature. Horizon null frame, flux densities and stability operator notation Surface measure, flux densities and null normal gauge
For the stated section, is a connected closed two-sphere and the outward graph stability operator has nonnegative principal eigenvalue . The principal-eigenvalue theorem supplies a smooth eigenfunction with . Nonnegative principal eigenvalue of the horizon stability operator Principal eigenfunctions and MOTS spectral stability
In this gauge the operator is , with all surface operations taken for . Horizon expansion variation and Einstein–Maxwell curvature
On the closed oriented surface, the integral of the divergence of a smooth vector field is zero. Gauss–Bonnet gives ; a tetrahedral triangulation of the two-sphere has Euler characteristic . Riemannian divergence theorem Global Gauss-Bonnet for closed oriented surfaces
Cauchy–Schwarz applies to square-integrable functions for the finite surface measure. Cauchy-Schwarz inequality for L²
The construction in Proposition 2.1: Einstein–Maxwell equations and regularity applies under [A1] and supplies the normalized smooth Ernst potential and a stationary one-form family satisfying the defining curl and contraction identities, with at a zero of , on the exterior and an open neighborhood of where . The symbols denote the resulting smooth Lorentzian metric and real two-form of Stationary Harrison one-form and metric and Harrison electromagnetic form, using the same fields, spacetime orientation and time orientation in [F1]–[F3].
Proof
Set and let be the surface metric-dual vector field. Dividing the eigenvalue equation in [F3] by and using gives . The positive eigenfunction makes smooth. Integrating, applying [F4], and using yields .
Smoothness and compactness put and the constant function in . By [F5], . Since , step 1.1 bounds the last integral by . Dividing by gives the area–charge inequality. This also proves its derivation from the same stability equation and Gauss–Bonnet. The fixed was arbitrary in , so the asserted sufficiently-small-positive-parameter case follows.
Source notes
The article reference records attribution. The proof uses the listed suppliers; it does not use the article's assertion as a premise.
Depends on
- Stationary vacuum model and asymptotic normalization
- Regular non-degenerate stationary vacuum spacetime
- Spacelike sections, maximality and lapse–shift data
- Mass-one convention and Harrison denominator
- Stationary Harrison one-form and metric
- Harrison electromagnetic form
- Proposition 2.1: Einstein–Maxwell equations and regularity
- Horizon null frame, flux densities and stability operator notation
- Surface measure, flux densities and null normal gauge
- Nonnegative principal eigenvalue of the horizon stability operator
- Horizon expansion variation and Einstein–Maxwell curvature
- Principal eigenfunctions and MOTS spectral stability
- Riemannian divergence theorem
- Global Gauss-Bonnet for closed oriented surfaces
- Cauchy-Schwarz inequality for L²
- The Axiom of Choice
Dependency tree · 2 levels
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Sources
- The uniqueness of smooth stationary black holes · PDF p. 27, proof of Theorem 4.2 and proof of Corollary 4.1