Energy of compactly supported fields on Euclidean three-space #
All integrals in this module are the standard Lebesgue volume integrals on
ProblemStatement.Space. Compact support supplies integrability; no finite
replacement measure or convention about nonintegrable functions is used.
A scalar bound for the forced energy inequality #
The integrating factor controls an energy whose time derivative is bounded by the energy plus a constant. Only derivatives in the interior of the time interval are required.
The shifted energy has a nonincreasing integrating factor.
The scalar forced Gronwall estimate with zero initial energy.
A bound independent of the endpoint of an interval contained in [0, 1].
A uniform spatial square-integral bound for compactly supported forces #
Compact spacetime support gives one compact spatial set supporting all slices.
Continuity of the parameterized integral then supplies a finite bound on the
closed time interval [0, 1].
A continuous force of compact spacetime support has uniformly bounded spatial square integrals on the unit time interval.
Integration against a compactly supported vector field transfers a directional derivative to its divergence.
Divergence-free transport contributes zero to the whole-space energy.
The pressure need not have compact support: the compact velocity already makes every integration-by-parts product integrable.
The full squared spatial L2 norm with ordinary Euclidean volume.
Equations
Instances For
Energy rate, given by ∫ x : Space, 2 * ⟪u (t, x), temporalDerivative u t x⟫_ℝ.
Equations
- NavierStokesR3.CompactEnergy.energyRate u t = ∫ (x : NavierStokes.ProblemStatement.Space), 2 * inner ℝ (u (t, x)) (NavierStokes.ProblemStatement.temporalDerivative u t x)
Instances For
Dissipation, given by ∑ i : Fin 3, ∫ x : Space, ‖spatialPartial i (fun y => u (t, y)) x‖ ^ 2.
Equations
- One or more equations did not get rendered due to their size.
Instances For
The exact forced Navier--Stokes energy balance on all of Euclidean space.
Young's inequality controls the forcing by the two actual squared L2 norms. All terms are integrable before the integral is compared.
Differentiation under the ordinary whole-space energy integral follows from joint smoothness and fixed compact spatial support.
The exact energy identity, with the derivative justified and all spatial integrals taken against ordinary Lebesgue volume on R³.
A smooth compact force yields one uniform bound for the kinetic energy before time one. The proof includes square integrability at every time, then uses the PDE-derived energy inequality and a scalar integrating factor.