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A divergence-free current with nonzero face-flux density: J=x^1∂_2 in flat space
Example
Let carry the identity chart, the flat metric , the time orientation and the chart orientation, with metric-selected connection and volume form (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model, Oriented smooth manifolds and oriented charts, The metric volume form, current flux through 3-faces and finite-chain charges). Let
be the smooth vector field of A smooth vector field is a smooth section of the tangent bundle. Then:
- : the current is divergence-free.
- The current -form is , and identically, consistently with clause (a) of Divergence, Stokes flux balance and the non-null face formula for a Lorentzian current.
- The pointwise flux density of through a non-null face with adapted unit normal is ; for the coordinate directions this is Thus the divergence-free current has nonzero flux density through the faces normal to : vanishing divergence does not mean vanishing flux through every face, and the flux balance of clause (b) of Divergence, Stokes flux balance and the non-null face formula for a Lorentzian current controls the side boundary genuinely.
Facts & Assumptions
Given: The flat Lorentzian four-manifold with identity chart, , metric-selected connection , volume form and the vector field .
, , and on the identity chart (The metric volume form, current flux through 3-faces and finite-chain charges, The derivative of the metric density and the chart formula for the divergence of a vector field, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields).
and is obtained by multiplying the -insertion by the component (Interior product of a form by a vector field, The wedge product of differential forms).
On a non-null face with velocity basis and adapted unit normal , and the pullback of on is (Divergence, Stokes flux balance and the non-null face formula for a Lorentzian current clause (c), Chart independence of the metric volume form, its value on orthonormal frames, and the unit normal and density of a non-null hyperplane).
Verification
(Divergence.) By [L1], .
(Current form.) By [L2] and , . Its exterior derivative is , because occurs twice; consistently, [L3] and step 1.1 give .
(Flux densities.) At a point of a face with adapted unit normal (so and for a coordinate face), [L4] gives the flux density ; for it is . For , ; for , . This is the displayed list of values. Since on the open set , the flux density through the faces normal to is nonzero there although the divergence of vanishes identically, which completes the verification.
Remarks
- Reading. The example isolates the pointwise flux density: a divergence-free current can have nonzero density through faces normal to . The flux-balance theorem concerns integrals over oriented chains and states exactly how the slice fluxes differ by the side flux; whether a whole side-chain flux vanishes depends on that chain and its orientation.
Depends on
The metric volume form, current flux through 3-faces and finite-chain charges
Chart independence of the metric volume form, its value on orthonormal frames, and the unit normal and density of a non-null hyperplane
Divergence, Stokes flux balance and the non-null face formula for a Lorentzian current
The derivative of the metric density and the chart formula for the divergence of a vector field
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
Metric compatibility, torsion freedom and the metric-selected connection class
Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields
Oriented smooth manifolds and oriented charts
Interior product of a form by a vector field
The wedge product of differential forms
A smooth vector field is a smooth section of the tangent bundle
Dependency tree · 2 levels
Sources
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), section 4.5.5 with figures 40-41: the charge balance with the timelike boundary B and the requirement of vanishing flux through B, printed pp. 187-189 (PDF pp. 194-196)
- H. S. Reall, Part III General Relativity (Cambridge, October 12, 2022 revision), section 8.7: Stokes' theorem with the side boundary, printed pp. 109-110 (PDF pp. 110-111)