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Ernst sublevels and the Mars–Simon tensor interface
Definition
Use the stationary Lorentzian data, metric connection and index conventions, together with the complex self-dual-form conventions. Let , , and without conjugation. For a complex two-form with real , use the interior product extended complex linearly: , so .
As normalization data, choose and a smooth embedding . Its image is the chosen parametrized spatial end, with radial coordinate . This end datum specifies where the limit is taken and imposes no metric decay conditions. For this interface an Ernst potential is a supplied smooth complex scalar satisfying , normalized by along this end. Precisely, for every there is such that for all , uniformly in angular direction. Existence of the end datum and of such a potential is supplied, not proved here.
On the open set define and . Write for the oriented metric volume tensor: in every positively oriented coordinate chart, . Use the same orientation for this tensor and the Hodge star. Write for the curvature convention used in the cited source; let and . The Mars–Simon tensor in the IK convention is . Curvature and orientation conventions must be transported together when applying this formula.
Definition references
Justification
The Killing equation makes alternating, using Stationary Lorentzian data and tensor conventions. The supplied self-dual-form interface Complex self-dual forms and metric-dependent contraction defines the complex contractions. The real interior product in Interior product of a form by a vector field is smooth and inserts into the first slot; its complex-linear extension is well defined because the real and imaginary parts are unique. The end embedding, in the sense of Smooth embeddings, makes a specified function on a Euclidean exterior; the quantified limit is therefore a predicate on the supplied data, rather than an assertion that stationary geometry provides an end or a normalized potential.
Clause (a) of The metric volume form, current flux through 3-faces and finite-chain charges supplies the smooth normalized metric volume form on an oriented Lorentzian four-manifold. Raising its indices uses the given inverse metric. On the smooth nonzero denominator permits the reciprocal and tensor formula, so they define smooth fields there. This construction does not assert a wave equation, vanishing or a Kerr characterization.
Appendix A.3 of Ionescu–Klainerman, printed p. 54, fixes . This is the curvature operator of Stationary Lorentzian data and tensor conventions with its output index lowered: in a coordinate frame . Thus the imported convention agrees with that supplier without a sign reversal or slot permutation.
External input
Ionescu–Klainerman supplies the displayed definition formulas in §4.2–§4.3, printed pp. 22–24, and the reciprocal potential in §7, equation (7.3), printed p. 35. Appendix A.3, printed p. 54, supplies the curvature convention compared above. Its normalization is at infinity along the chosen section. The embedding and quantified angularly uniform limit above specify that convention locally. Only definitions are adopted from the source's vacuum setting; no potential-existence or analytic theorem is inferred.
Depends on
- Stationary Lorentzian data and tensor conventions
- Complex self-dual forms and metric-dependent contraction
- Interior product of a form by a vector field
- The metric volume form, current flux through 3-faces and finite-chain charges
- Smooth embeddings
- Ionescu–Klainerman, On the uniqueness of smooth, stationary black holes in vacuum · §4.2, (4.11), (4.15), (4.17) and the normalization paragraph after (4.18), printed pp. 22–23; §4.3, (4.19)–(4.21), (4.27), Definition 4.3 (4.29), printed pp. 23–24; §7, (7.3), printed p. 35; Appendix A.3, opening curvature-component formula, printed p. 54 (PDF p. 54).
Used by · 10
- Ionescu–Klainerman local Kerr criterion with full interface
- Local Kerr rigidity and conditional global identification
- Conditional horizon recovery and Kerr implications
- Pathwise exhaustion by anchored Ernst sublevels
- Stationary transport of vanishing from a section
- Normalized Ernst data and zero Mars–Simon survive stationary gauges
- AIK global Kerr identification under the full GR/SBS/PK contract
- The IK continuation also fixes one global reciprocal invariant
- A smooth radial primitive can be returned to a weak end gauge
- Equivariant global Harrison primitive under weak original data
Dependency tree · 2 levels
Each result is drawn at its shortest distance from this item. Arrows run from prerequisites to the items that use them; this item has a heavier outline. External source nodes link directly to the cited text. The view shows up to two dependency steps; open a prerequisite to continue.
External dependencies
Definitions of the Killing two-form, complex self-dual form, Ernst differential, normalized potential, reciprocal potential and Mars–Simon tensor, and the Riemann curvature sign and slot convention used in these formulas.
Hypotheses: The cited development assumes a smooth oriented four-dimensional vacuum spacetime, a Killing field and an existing Ernst potential; 1−σ is nonzero on the reciprocal/tensor domain. Only the displayed definitions are adopted here for stationary Lorentzian data with a supplied potential; no vacuum identity or existence theorem is imported.
Reading limits: Read the PDF text at the listed definition equations and normalization paragraph, including (7.3), and the opening curvature formula of Appendix A.3 on printed p. 54. Compared that formula with the stationary-data supplier. The end parametrization, quantified limit and complex-linear extension are local formulation details. No PDF image inspection, analytic proof reconstruction or independent proof review is claimed.
Sources
- Ionescu–Klainerman, On the uniqueness of smooth, stationary black holes in vacuum · §4.2, (4.11), (4.15), (4.17) and the normalization paragraph after (4.18), printed pp. 22–23; §4.3, (4.19)–(4.21), (4.27), Definition 4.3 (4.29), printed pp. 23–24; §7, (7.3), printed p. 35; Appendix A.3, opening curvature-component formula, printed p. 54 (PDF p. 54).