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Positive smooth horizon area and the exact degenerate angular-momentum test
Statement
Work in ZFC. Let be a nonempty compact smooth spacelike horizon cross-section, let be its induced Riemannian metric, and define its intrinsic area by , where is the Riemannian volume density. Then . For any supplied real scalar , the equality implies . In the degenerate stationary axisymmetric vacuum application, vacuum means near the section. Supply the axial generator with angle parameter of period , an ambient orientation and an orientation of . In geometric units , the component charge is the finite-section Komar functional , where is inclusion and ; take in the assumed equality. These application data do not restrict the arbitrary-scalar implication. This is a componentwise test: it does not require the total angular momentum of all components to be nonzero and puts no condition on nondegenerate components.
Facts & Assumptions
Work in ZFC with The Axiom of Choice. In particular The Axiom of Countable Choice (AC_ω) holds: apply choice to the family of nonempty sets in a sequence and compose the choice function with that sequence. Countable choice is the inherited hypothesis of the chart-partition integration in [F2] and [F3].
Horizon, stationarity, axisymmetry and degeneracy terminology is that of Staticity, axisymmetry and black-hole regularity hypotheses. Smoothness, compactness, nonemptiness and spacelikeness of the two-dimensional cross-section are explicit hypotheses here. Its smooth induced positive-definite tensor is a Riemannian metric in Riemannian metric and riemannian manifold.
The density Riemannian volume density is in a surface chart. By The riemannian volume density is coordinate independent these formulas glue to a positive smooth density independent of the chart.
Use Riemannian volume of a compactly supported smooth density with on the compact surface to define . Under [A1], Orientation-free density integration and its properties makes this integral independent of charts and partition, nonnegative, and strictly positive for every nonzero nonnegative smooth density. The compact-support construction is a finite sum of finite chart integrals and requires no orientation.
For the second assertion, the extra data are a specified real scalar attached to this component and the assumed equality , with defined in [F3]. In the intended degenerate stationary axisymmetric vacuum application, take the charge defined in [F5] for this same section, with the equality in that normalization supplied independently. The lemma uses only this scalar-data contract and the equality; the area–angular-momentum relation remains a premise.
For the application terminology, vacuum is the geometric predicate near , with the Ricci tensor of The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors. Use the chosen axial generator of Staticity, axisymmetry and black-hole regularity hypotheses. Specify an orientation of its Lorentzian neighborhood and an orientation of for this charge. Metric duality The inverse metric, musical isomorphisms and index raising gives , and Lorentzian exterior calculus and Hodge star gives the smooth two-form . With inclusion , define using Integration on an oriented embedded submanifold. Reall (8.25) fixes the integrand and factor in units ; the finite-section functional is defined here. Its orientations and axial scale are supplied data. No equality to a charge at infinity, independence of cross-section, or derivation of the area relation is asserted by this definition.
Proof
Given: A nonempty compact smooth spacelike cross-section with its induced positive metric, [A1] and [F1]–[F3]; for the second assertion also the real component charge and equality in [F4]; for the geometric application, additionally the data in [F5].
Goal: Verify intrinsic finite positive area and the exact componentwise nonvanishing consequence.
By [F1] and [F2], is a positive smooth density on the nonempty surface, hence is nonzero. Compactness makes its support compact, and is smooth with compact support. Thus the integral construction in [F3] applies under [A1] and gives a finite real value : only finitely many partition-weighted, compactly supported chart coefficients contribute, each with finite integral. Strict positivity in [F3] applies to the nonzero positive density, so . Choice is used only through the inherited chart-partition construction.
For the application data in [F5], the Ricci tensor is defined on the specified smooth Lorentzian neighborhood, so its vanishing is a definite predicate. The specified smooth axial field has a smooth metric dual, exterior derivative and Hodge dual. Pullback gives a smooth real top form on oriented ; its support is compact because is compact. The submanifold integration supplier therefore gives a finite real . Thus the application supplies a scalar of the type required by [F4], without a physical postulate or a conservation assertion.
If , the supplied equality in [F4] gives , contradicting step 1.1. Therefore . Apply this implication separately to each degenerate component for which the scalar charge and equality are supplied. It uses no sum of component charges and imposes no condition on a nondegenerate component.
External input
The cited Komar definition supplies the normalization recorded in the source contract. The finite-section functional in [F5] is a local definition using the declared mathematical suppliers; the proof establishes its finiteness. The area–angular-momentum equality remains an independently supplied premise.
Depends on
- Staticity, axisymmetry and black-hole regularity hypotheses
- Riemannian metric and riemannian manifold
- The Axiom of Choice
- The Axiom of Countable Choice (AC_ω)
- Riemannian volume density
- The riemannian volume density is coordinate independent
- Riemannian volume of a compactly supported smooth density
- Orientation-free density integration and its properties
- The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
- The inverse metric, musical isomorphisms and index raising
- Lorentzian exterior calculus and Hodge star
- Integration on an oriented embedded submanifold
- H. S. Reall, Black Holes, Part III lecture notes, 15 March 2024 · Conventions, printed p.1; section 8.2, equation (8.25), printed p.109 (PDF page 110).
Dependency tree · 2 levels
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External dependencies
In units G=c=1, Komar angular momentum at an axisymmetric asymptotically flat end is (16 pi)^(-1) times the large-sphere limit of the integral of star d(m-flat), where m generates axial rotations.
Hypotheses: The cited definition assumes an axisymmetric asymptotically flat end and an existing limit. Only its integrand and numerical normalization are adopted here; the finite-section functional is defined locally, with a specified 2 pi axial generator and orientations. No asymptotic or horizon-transport equality is imported.
Reading limits: Read browser-extracted PDF text at Conventions and section 8.2 through (8.25). No visual inspection, convergence proof, conservation theorem or area equality was checked or imported.
Sources
- H. S. Reall, Black Holes, Part III lecture notes, 15 March 2024 · Conventions, printed p.1; section 8.2, equation (8.25), printed p.109 (PDF page 110).