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Diffeomorphism Noether current identity and local charge
Statement
Let be an oriented smooth four-manifold, let be the chosen smooth field bundle, and let be a local Lagrangian four-form for its smooth sections, with a chosen first-variation decomposition . Let be a smooth spacetime vector field with local flow . Suppose there is a smooth local lift to fibre-preserving local diffeomorphisms of over , with and the local flow composition law. On the common domain define its induced pullback action on sections by Write the vertical field variation determined by this smooth family; at each it lies in , the tangent space to the fibre . In the tensor-field case where , it is the Lie derivative defined by the local-flow derivative. Assume the action preserves the chosen field domain, and assume covariance in the precise sense wherever both sides are defined; thus its derivative satisfies . Define the Noether current three-form
Then
Here a solution means a field configuration at which the Euler functional vanishes, that is, for every smooth variation in its domain. Thus is closed on solutions. For every chart whose open image is star-shaped, a solution has a local two-form with .
Statement references
Some Properties of Noether Charge, §4
Advanced Lectures on General Relativity, §1.3.3
Covariant phase space with boundaries, §§2.3–2.4
Covariant field families and variations
Covariant presymplectic current
Closed differential forms are exact on star-shaped coordinate domains
The Lie derivative of a differential form
The Lie derivative of a tensor field
Facts & Assumptions
Given: The selected first-variation decomposition, the local spacetime flow , its specified smooth lift and induced section action , and the stated covariance of .
and by the specified lifted action and covariance condition.
The first-variation decomposition is . Covariant presymplectic current
Cartan's identity is for every differential form . Cartan's magic formula
A closed smooth -form on an open star-shaped domain in has a primitive for each . Closed differential forms are exact on star-shaped coordinate domains
For a tensor field and the local flow of , . The Lie derivative of a tensor field
Pullback is defined by evaluation on the differential of the map, and for a smooth map and smooth form . The pullback of a differential form The exterior derivative commutes with pullback
Proof
Given: As in [A1] and [F1]–[F5].
By the tensor-flow definition [F4], is the derivative of the pullback of the spacetime four-form along . Since has top degree on a four-manifold, . Cartan's identity [F2] gives .
Apply [F1] to the variation supplied by [A1] and equate it with step 1.1: . Rearranging gives .
If , step 2.1 gives . For a chart as in the Statement, the form is closed on by [F5]. Apply [F3] with to obtain with . Set ; [F5] gives .
Remarks
The primitive is local. This proposition gives no global Noether charge without a separate cohomological argument. It asserts a classical identity only; it constructs no measure, Hilbert space, or anomaly-free quantization.
The current sign in the cited sources is not uniform. Iyer--Wald's equation (49) and Harlow--Wu's equation (2.44) use the current defined here. Compère--Fiorucci's equation (1.59) uses , which is in the tensor-field case; its on-shell current identity and local primitive therefore require the same sign conversion. The proof above uses only the explicit local hypotheses stated here.
Depends on
Covariant field families and variations
Covariant presymplectic current
Closed differential forms are exact on star-shaped coordinate domains
Cartan's magic formula
The Lie derivative of a differential form
The Lie derivative of a tensor field
The pullback of a differential form
The exterior derivative commutes with pullback
Dependency tree · 2 levels
Sources
- Vivek Iyer and Robert M. Wald, Some Properties of Noether Charge and a Proposal for Dynamical Black Hole Entropy, §4, equations (49)–(51)
- Geoffrey Compère and Adrien Fiorucci, Advanced Lectures on General Relativity, §1.3.3
- Daniel Harlow and Jie-qiang Wu, Covariant phase space with boundaries, §§2.3–2.4