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Harrison electromagnetic form
PDF p. 6: §1.4; PDF p. 8: (2.6)
Definition
Use stationary Lorentzian data and a supplied normalized Ernst potential on an open set , with , Killing two-form , complex two-form , and . Here is the one-form , and the Hodge star uses the supplied orientation. Fix , put and , and use the Harrison one-form data on an open subset where . In particular, is the supplied real one-form, , and is the supplied Lorentzian metric. The pullback is fiberwise: .
Define the complex Harrison electromagnetic two-form and its real part by
With the same orientation used for as for , the associated identity is . No Maxwell equation or existence of is asserted by this definition.
Definition references
Facts & Assumptions
The normalized Ernst data supply the smooth complex two-form , the relation , and the identity . Killing two-form and normalized Ernst notation Complex self-dual forms and metric-dependent contraction
The Harrison data give on , , , the invertible map , and . Stationary Harrison one-form and metric Mass-one convention and Harrison denominator
The oriented metric Hodge map is characterized by and extends complex linearly. Geometric electrovacuum equations and charge convention Complex self-dual forms and metric-dependent contraction
Justification
Given: The data, parameter and restrictions in the Definition.
Goal: Establish well-definedness, the wedge formula, and the Hodge identity.
1.1 Since , the denominator is nonzero, and all coefficients are smooth; is a real constant, including at the endpoints. Expanding the two arguments of the alternating form gives : the term with two copies of vanishes. Substitution of proves the second expression and shows that and are smooth two-forms. [given, F1, F2, algebra]
2.1 At each point, the rank-one determinant identity gives ; thus preserves the specified orientation. Put . For real two-forms , the defining Hodge pairing, , and four-dimensional volume scaling yield and . Pulling back the defining wedge identity therefore gives ; nondegeneracy of the wedge pairing gives uniqueness. Complex linearity and imply . Writing with real , comparison of real parts gives . [given, F1, F2, F3, step 1.1, algebra] ∎
Source notes
The cited article attributes the formulas. The justification uses the supplied geometric definitions and pointwise algebra, and does not use the article's assertion as a premise.
Depends on
Used by · 14
- Positivity of the Harrison denominator and horizon bound
- Proposition 2.1: Einstein–Maxwell equations and regularity
- Proposition 2.1: electric and magnetic fluxes
- Mean-curvature linearization, weighted regularity and fixed-boundary graph map
- Horizon null frame, flux densities and stability operator notation
- Nonnegative principal eigenvalue of the horizon stability operator
- Stable-horizon flux-energy and area-charge inequalities
- Theorem 4.2: charged horizon area lower bound
- Boost invariance and limiting Maxwell normal form
- Inverse Harrison relation and Killing-scalar identity
- Harrison equation residuals are continuous functions of stationary two-jets
- Positive-parameter Harrison charge limits in the original end chart
- The zero Harrison parameter follows from continuity on one fixed sphere
- Weak original data furnish the one recovery family and pole
Dependency tree · 2 levels
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Sources
- The uniqueness of smooth stationary black holes · PDF page 6, section 1.4; page 8, equation (2.6) and the following displayed formula