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Complex self-dual forms and metric-dependent contraction
Definition
Assume the Axiom of Countable Choice : every countable family of nonempty sets has a choice function.
Let be a smooth, oriented and time-oriented Lorentzian four-manifold of signature . A real two-form is a smooth section of ; a complex two-form is a section of its complexification and can be written uniquely as with real two-forms . Extend the metric Hodge star complex linearly by . In this convention a complex two-form is called self-dual when .
For a real two-form , define its complex self-dual form by . Raise both indices using the inverse metric and define the complex bilinear contraction , with summation over both indices and without complex conjugation or a factor of one half.
Let be a smooth fiberwise invertible real-linear bundle map over the identity. Its algebraic pullbacks are the covariant two-tensors and for . The latter is again a real two-form. This pullback is defined fiberwise and need not be the differential of a diffeomorphism.
Definition references
Oriented Lorentzian fields, observers and coordinate conventions
Lorentzian exterior calculus and Hodge star
The inverse metric, musical isomorphisms and index raising
The direct-sum model V⊕ iV of a complexification
Smooth vector bundles, rank, fibres, and trivial bundles
Smooth sections, local sections, and support
Facts & Assumptions
Assume the Axiom of Countable Choice : every countable family of nonempty sets has a choice function, as defined in The Axiom of Countable Choice (AC_ω). This is the background assumption of the geometric suppliers used in [F1] and [F2].
The oriented, time-oriented Lorentzian data and real differential forms are as in Oriented Lorentzian fields, observers and coordinate conventions.
The metric Hodge star is a smooth real-linear bundle map and satisfies on real two-forms. Lorentzian exterior calculus and Hodge star
The nondegenerate metric has an inverse, which raises tensor indices. The inverse metric, musical isomorphisms and index raising
For a real vector space , the direct-sum complexification has underlying pairs , written , with . The direct-sum model V⊕ iV of a complexification
Smooth real vector bundles are described by fibrewise linear local trivializations; a smooth section is a smooth right inverse to the bundle projection. A bundle map over the identity is a smooth map preserving the projection and linear on each fibre. Smooth vector bundles, rank, fibres, and trivial bundles, Smooth sections, local sections, and support, Vector bundle maps over a smooth base map
The intrinsic exterior pairing on real two-forms has component expression . Lorentzian exterior calculus and Hodge star
The inertia of a finite-dimensional real symmetric bilinear form is independent of its diagonalizing basis, so invertible real congruence preserves the numbers of positive, negative and zero entries. Sylvester's law of inertia: every real symmetric form is congruent to diag(Iₚ,-I_q,0ᵣ), and (p,q,r) is unique
Justification
Here is the smooth complexification construction used in the Definition. Put . As a set over , take with projection , and equip each fibre with the scalar operations of [F4]. Each real local trivialization of gives coordinates on this set. If the real transition matrix is , the pair transition is . It is smooth with smooth inverse given by the inverse transition matrix; the identity and cocycle relations are inherited from those of . Identifying with , this transition is complex-linear by [F4]. Thus these coordinates give the smooth complex vector bundle meant here, with underlying real bundle of rank twelve in the sense of [F5]. A section is smooth exactly when its two component sections are smooth, since both projection to the pair components and formation of the pair are smooth in these coordinates. Consequently every smooth complex two-form has unique globally defined real and imaginary smooth two-forms .
For any smooth real-linear bundle map , define . Uniqueness of the pair makes this well defined. Real linearity gives , so it is complex-linear. In the pair coordinates its matrix is the same smooth matrix of on both components, so it is smooth. Apply this construction to the map of [F2]. By [F2], , so the stated name agrees with the chosen eigenvalue convention.
For real two-forms , use the inverse metric of [F3] in each covector slot to form . By [F6], the full contraction equals , so it is intrinsically defined and independent of the frame. Extend this real bilinear pairing complex bilinearly, using the unique real and imaginary parts just constructed. In particular . Its component expression is exactly the full sum in the Definition, with no conjugation and no factor of one half, so that expression is well defined in every frame.
The bundle map has the meaning in [F5], with base map . In any local frame its matrix entries are smooth, since they are components of the smooth map applied to the local basis sections. The pullback components are and , hence smooth. The defining fibrewise evaluations are intrinsically bilinear, symmetric for and alternating for , so these local expressions agree on overlaps and the latter defines a real two-form. If for every , surjectivity of implies for every , whence and then . Thus is nondegenerate. Its matrix is , an invertible congruence, so [F7] gives the same signature as . This reasoning uses only the fibrewise bundle map, with no assumption that it is a differential.
External input
The Hodge definition and square formula in Carroll's Lecture Notes on General Relativity, §1, equations (1.87)–(1.88), PDF p. 30, provide independent background for the chosen convention. Only those equations and the accompanying signature explanation were consulted. The smooth Hodge map and its square used above are supplied by [F2]; the complex bundle, extension, contraction application and pullback justification are local constructions from [F1]–[F7].
Depends on
- Oriented Lorentzian fields, observers and coordinate conventions
- Lorentzian exterior calculus and Hodge star
- The inverse metric, musical isomorphisms and index raising
- The direct-sum model V⊕ iV of a complexification
- Smooth vector bundles, rank, fibres, and trivial bundles
- Smooth sections, local sections, and support
- Vector bundle maps over a smooth base map
- Sylvester's law of inertia: every real symmetric form is congruent to diag(Iₚ,-I_q,0ᵣ), and (p,q,r) is unique
- The Axiom of Countable Choice (AC_ω)
- Lecture Notes on General Relativity · §1, equations (1.87)–(1.88), PDF p. 30
Used by · 33
- Vacuum Killing and Ernst differential identities
- Smooth invariant Harrison primitive near the horizon and at infinity
- Regular Harrison Einstein–Maxwell family
- Rank-one tangent changes, signature and Hodge transfer
- Ionescu–Klainerman local Kerr criterion with full interface
- Killing two-form and normalized Ernst notation
- Stationary Harrison one-form and metric
- Harrison electromagnetic form
- Single-potential construction of the Harrison one-form family
- Mass-one Ernst and radial primitive asymptotics
- Closedness, periods and smooth global choice of W0
- Proposition 2.1: Einstein–Maxwell equations and regularity
- Horizon null frame, flux densities and stability operator notation
- Boost invariance and limiting Maxwell normal form
- Inverse Harrison relation and Killing-scalar identity
- Pole identities and the Ernst scalar inequality reduction
- Proposition 5.1: recovery of Ionescu–Klainerman conditions
- Vanishing divergence implies closed Hodge dual
- Killing flow preserves its complex two-form
- Closed Ernst contraction and the real potential
- Lifting a normalized stationary primitive to the Harrison parameter
- Regular Lorentzian metric from the normalized rank-one map
- Smooth Maxwell tensor formula without division by the stationary norm
- Ernst sublevels and the Mars–Simon tensor interface
- Fixing the Ernst constant by integrable asymptotic twist
- A common positive Harrison domain across the compact sphere
- Harrison equation residuals are continuous functions of stationary two-jets
- Passing a local Harrison identity through compatible stationary jets
- Ernst and self-dual curvature data in the AIK convention
- Mars–Simon tensor and its smooth weighted extension
- Harrison spatial two-form differs from the seed by an integrable tail
- A smooth radial primitive can be returned to a weak end gauge
- Equivariant global Harrison primitive under weak original data
Dependency tree · 2 levels
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External dependencies
The Hodge star maps p-forms to (n-p)-forms and its square is given by the metric-signature formula.
Hypotheses: An oriented nondegenerate metric and the stated form degree and dimension.
Reading limits: Consulted only §1, equations (1.87)–(1.88) and the accompanying signature explanation on PDF p. 30. This is background for the Hodge convention; the bundle construction, complex extension and applications below are local arguments using the declared mathematical suppliers.
Sources
- Lecture Notes on General Relativity · §1, equations (1.87)–(1.88), PDF p. 30