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Proposition 5.1: recovery of Ionescu–Klainerman conditions
PDF p. 28: Proposition 5.1; (5.1); PDF p. 29: Proposition 5.1; proof
Statement
Adopt the stationary vacuum model and regular non-degenerate stationary construction, with original exterior section spacelike and maximal, ADM mass one, and stationary Killing field not identically zero on the bifurcation sphere . Use the supplied normalized Ernst potential , the single regular Harrison family, and its chosen pole , as in the two recovery suppliers. Here is the common pole of the local Hawking and axial fields supplied under these hypotheses: , , , has least positive common period , and has positive normal boost rate in the future/outward normal basis. The Harrison family uses this same pole. Here and is real. Define and , where and are the original metric's Levi–Civita connection and oriented Hodge star. Contract complex bilinearly, without conjugation or a factor of one half, and raise both indices using the original metric .
Then everywhere on , and .
Statement references
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
Killing two-form and normalized Ernst notation
Complex self-dual forms and metric-dependent contraction
Local Hawking and axial fields, boost and pole
Facts & Assumptions
The stationary vacuum model, regular construction, maximal original exterior section, mass-one normalization, nontriviality of on , supplied potential, Harrison family and pole are those in the Statement. 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
The normalized Ernst and complex-form conventions give the displayed definitions of , and , with the original metric used to raise indices and a complex bilinear contraction. Killing two-form and normalized Ernst notation Complex self-dual forms and metric-dependent contraction
Under the stated construction hypotheses, the inverse Harrison contraction gives on . Inverse Harrison relation and Killing-scalar identity
With the local fields and common pole in [F4], the same normalized potential and regular Harrison family, and , axial averaging gives ; in particular the displayed reciprocal is defined. Axial averaging and positive boost at the pole
The regular stationary vacuum data, maximal original exterior section and supply local commuting Killing fields with , , a circle action of least positive common period , a common pole with , and a constant positive normal boost rate for in the future/outward normal basis. These are the fields and pole used for the stated single Harrison family. Local Hawking and axial fields, boost and pole
Proof
Given: The model, construction and conventions in the Statement.
Goal: Establish the two displayed conditions on and at .
The regular stationary vacuum data, maximal original exterior section and nontriviality of in [A1] match [F4]. Use its local fields and common pole , with the normalized circle action and positive future/outward boost. By the stated family choice this is the same pole used throughout the two recovery suppliers, rather than a separately chosen zero of .
The construction hypotheses and original-metric contraction convention match [F2] for this family. Multiplying its equality by gives at every point of .
At the common pole, gives , so and . Together with the local fields, circle normalization and positive boost from step 1.1 and the same potential and family, this verifies the premises of [F3]. Adding one to its strict inequality and dividing by the positive number two gives . Together with step 2.1 this proves both conditions.
Source notes
The article is cited for attribution of Proposition 5.1. The deduction above uses the declared local-field and recovery suppliers. The article's assertion is not a proof 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
- Killing two-form and normalized Ernst notation
- Complex self-dual forms and metric-dependent contraction
- Inverse Harrison relation and Killing-scalar identity
- Axial averaging and positive boost at the pole
- Local Hawking and axial fields, boost and pole
Dependency tree · 2 levels
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Sources
- The uniqueness of smooth stationary black holes · PDF pages 28–29, Proposition 5.1 and its proof