Good points for the endpoint regularity argument #
The domains and energy in this file use the spatial and parabolic conventions
of def:good-point.
The open space-time cylinder used in def:good-point.
Equations
- ESS.goodPointPastCylinder x t r = CKN.Foundation.Parabolic.vec3Ball x r ×ˢ Set.Ioo (t - r ^ 2) t
Instances For
The open domain and its closed top face used in def:good-point.
Equations
Instances For
The unit past cylinder including its top time slice.
Equations
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noncomputable def
ESS.goodPointEnergy
(u : CKN.Foundation.Parabolic.ParabolicPoint → CKN.Foundation.Parabolic.Vec3)
(p : CKN.Foundation.Parabolic.ParabolicPoint → ℝ)
(x : CKN.Foundation.Parabolic.Vec3)
(t r : ℝ)
:
The nonnegative velocity and pressure energy on a past cylinder. The CKN cylinder includes its top slice, which is null for space-time volume.
Equations
- One or more equations did not get rendered due to their size.
Instances For
def
ESS.IsGoodPoint
(ε₀ : ℝ)
(u : CKN.Foundation.Parabolic.ParabolicPoint → CKN.Foundation.Parabolic.Vec3)
(p : CKN.Foundation.Parabolic.ParabolicPoint → ℝ)
(z : CKN.Foundation.Parabolic.ParabolicPoint)
:
A point is good when it has an admissible past cylinder with sufficiently small normalized velocity and pressure energy.
Equations
- One or more equations did not get rendered due to their size.
Instances For
theorem
ESS.goodPointEnergy_mono
{u : CKN.Foundation.Parabolic.ParabolicPoint → CKN.Foundation.Parabolic.Vec3}
{p : CKN.Foundation.Parabolic.ParabolicPoint → ℝ}
{x₁ x₂ : CKN.Foundation.Parabolic.Vec3}
{t₁ t₂ r₁ r₂ : ℝ}
(hsubset : CKN.Foundation.Parabolic.parabolicCylinder x₁ t₁ r₁ ⊆ CKN.Foundation.Parabolic.parabolicCylinder x₂ t₂ r₂)
:
The good-point energy is monotone in the cylinder.