The ordinary three-dimensional solenoidal space for the mean inverse #
This is the actual Lebesgue L² space on R³. Its solenoidal subspace is defined by orthogonality to genuine compactly supported smooth gradients, and the weak divergence test characterization is proved. The projected coefficient inverse below acts on this space, rather than on the lifted cylinder used by the oscillatory correction construction.
L²: an abbreviation for MeasureTheory.Lp Space 2 (volume : Measure Space).
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Test gradient, given by (gradient_memLp hc hs).toLp (gradient φ).
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- EulerMeanSolenoidal.testGradient φ hc hs = MeasureTheory.MemLp.toLp (gradient φ) ⋯
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Gradient space, given by (Submodule.span ℝ gradientGenerators).topologicalClosure.
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Solenoidal space, given by gradientSpace.orthogonal instance : CompleteSpace solenoidalSpace := gradientSpace.isClosed_orthogonal.completeSpace_coe.
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Orthogonality is equivalent to the ordinary distributional divergence test.
Solenoidal projection, given by solenoidalSpace.starProjection.
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The pressure component of the ordinary Helmholtz decomposition.
Classical integration by parts against a compact smooth test, on R³.
A classical divergence-free L² field lies in the actual closed mean space.
In particular, every smooth L² curl is solenoidal in the ordinary space.
The concrete inverse of the projected ordinary-space coefficient multiplier.
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- One or more equations did not get rendered due to their size.
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A forcing in the ambient L² space has one solenoidal solution of the projected metric equation. No inverse or solution is supplied as an input.
The residual of the solved projected equation is a genuine weak gradient.