Spatial Partial Congr Space Time Set #
Supporting results for the Constantin–Ignatova–Vicol axisymmetric regularity theorem.
theorem
CIV.spatialPartial_congr_of_eqOn_spaceTimeSet
{v u : CKN.Foundation.Parabolic.ParabolicPoint → ℝ}
{Ω : Set CKN.Foundation.Parabolic.Vec3}
{I : Set ℝ}
(hΩ : IsOpen Ω)
(hI : IsOpen I)
(h : ∀ w ∈ CKN.spaceTimeSet Ω I, v w = u w)
{z : CKN.Foundation.Parabolic.ParabolicPoint}
(hz : z ∈ CKN.spaceTimeSet Ω I)
(j : Fin 3)
:
Pointwise agreement of two scalar fields on an open space-time cylinder transports a
spatial partial derivative. These lemmas generalize CIV.spatialPartial_congr_of_eqOn
(CIV/Reduction/AveragedClassical.lean) from the unit cylinder to an arbitrary open
cylinder spaceTimeSet Ω I, needed to differentiate the momentum equation of a classical
solution on the general cylinder that thm:analytic:interior is stated on.
theorem
CIV.timePartial_congr_of_eqOn_spaceTimeSet
{v u : CKN.Foundation.Parabolic.ParabolicPoint → ℝ}
{Ω : Set CKN.Foundation.Parabolic.Vec3}
{I : Set ℝ}
(hΩ : IsOpen Ω)
(hI : IsOpen I)
(h : ∀ w ∈ CKN.spaceTimeSet Ω I, v w = u w)
{z : CKN.Foundation.Parabolic.ParabolicPoint}
(hz : z ∈ CKN.spaceTimeSet Ω I)
:
Pointwise agreement of two scalar fields on an open space-time cylinder transports the time partial derivative.
theorem
CIV.spatialSecondPartial_congr_of_eqOn_spaceTimeSet
{v u : CKN.Foundation.Parabolic.ParabolicPoint → ℝ}
{Ω : Set CKN.Foundation.Parabolic.Vec3}
{I : Set ℝ}
(hΩ : IsOpen Ω)
(hI : IsOpen I)
(h : ∀ w ∈ CKN.spaceTimeSet Ω I, v w = u w)
{z : CKN.Foundation.Parabolic.ParabolicPoint}
(hz : z ∈ CKN.spaceTimeSet Ω I)
(i j : Fin 3)
:
Pointwise agreement of two scalar fields on an open space-time cylinder transports a second spatial partial derivative.