The initial induction state is completely constructed from the compact β-family. A single positive time and a single label constant work for the family, with actual low-order guards and pressure sign.
Actual constant coefficient towers for the ordinary Euler correction equation: identity pressure metric, zero lower-order coefficients, spatial scale one and angular direction zero. No solution is included in the data.
Cache the standard NormedAddCommGroup (Space →L[ℝ] Space) instance to shorten typeclass
synthesis.
Instances For
Cache the standard NormedSpace ℝ (Space →L[ℝ] Space) instance to shorten typeclass
synthesis.
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Cache the standard NormedAddCommGroup (LiftTangent →L[ℝ] Space →L[ℝ] Space) instance to
shorten typeclass synthesis.
Instances For
Cache the standard NormedSpace ℝ (LiftTangent →L[ℝ] Space →L[ℝ] Space) instance to shorten
typeclass synthesis.
Instances For
Cache the standard NormedAddCommGroup (LiftTangent →L[ℝ] LiftTangent →L[ℝ] Space →L[ℝ] Space) instance to shorten typeclass synthesis.
Instances For
Cache the standard NormedSpace ℝ (LiftTangent →L[ℝ] LiftTangent →L[ℝ] Space →L[ℝ] Space)
instance to shorten typeclass synthesis.
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Coefficient, bundling coefficient, smooth, bound, norm_bound and the required
compatibility proofs.
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Jet used in constant correction data.
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- EulerConstantCorrection.jet P A 0 = EulerSpatialSobolevInverse.CoefficientJet.zero (EulerConstantCorrection.coefficient P A)
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Tower, bundling coefficient, jet, continuous.
Equations
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Data, bundling κ, direction, scale_bound, direction_bound and the required
compatibility proofs.
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Metric budget, bundling metric, continuous, derivative, hasDeriv and the required
compatibility proofs.
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Pressure bound, given by 9^729.
Equations
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The literal spatial convection of a small smooth cylinder field has a quadratic residual envelope at every Sobolev order. No residual estimate or differential equation is postulated.
Residual cost, given by 1+108*productBlockConstant P*C^2*R.
Equations
- EulerSmallCorrection.residualCost P C R = 1 + 108 * EulerCylinderPathProduct.productBlockConstant P * C ^ 2 * R
Instances For
Residual, given by (G.smul ε).spatialTransport (G.smul ε).
Equations
- EulerSmallCorrection.residual G ε = (G.smul ε).spatialTransport (G.smul ε)
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Input, given by data P (G.smul ε).toFieldTower (residual G ε).toFieldTower.
Equations
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An actual exact lifted Euler solution is constructed from any genuine smooth solenoidal L² datum with factorial derivative bounds. The amplitude is an explicit function of the supplied bounds and does not depend on the particular datum realizing them.
A genuine all-order correction budget for small smooth data with the identity metric. Every field and coefficient estimate is derived from the given datum's actual word bound; the amplitude is chosen explicitly.
An explicit positive amplitude puts any finite Gevrey datum and quadratic residual envelope in the all-order correction regime. The growth constant belongs to the identity-metric equation, not to an assumed solution.
Initial radius, given by 1/(2*(R+1)).
Equations
- EulerSmallCorrection.initialRadius R = 1 / (2 * (R + 1))
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These are scalar smallness inequalities, obtained explicitly below.
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Spatial budget, bundling Rc, M, B, B0 and the required compatibility proofs.
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Drift budget, bundling full, drift, drift_nonneg, drift_bound and the required
compatibility proofs.
Equations
- EulerSmallCorrection.driftBudget G hG hC hR S q hq = { full := EulerSmallCorrection.spatialBudget G hG hC hR S q hq, drift := 8 * S.value * C, drift_nonneg := ⋯, drift_bound := ⋯ }
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Budget, bundling metric, radius, growthCoefficient, delta and the required
compatibility proofs.
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No scalar guard is required of the input: the amplitude is explicitly chosen from its finite actual Gevrey constants.
Equations
- EulerSmallCorrection.smallBudget G hG hC hR hdiv = EulerSmallCorrection.budget G hG hC hR (EulerSmallCorrection.scale P C R (EulerSmallCorrection.residualCost P C R) hC hR ⋯) hdiv
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A genuine smooth spatial L² field, embedded as a time-independent, angle-independent cylinder field. Tensor bounds give a fixed mixed Sobolev word bound, and classical divergence zero gives the actual lifted constraint.
Spatial orbit, given by EulerLpTranslation.translation a.1 u.toLp.
Equations
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Field, constructed using Field.ofLifted.
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For a static approximation the prescribed residual is exactly its spatial convection, at every finite Sobolev order. This verifies the equation input to the correction theorem rather than assuming it.
Approximation residual, bundling pressure, gradient, equation, let and the required
compatibility proofs.
Equations
- EulerSmallCorrection.approximationResidual G hT ε hstatic = { pressure := (EulerPacketCylinderField.Field.zero P T).toFieldTower, gradient := ⋯, equation := ⋯ }
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Scales, given by scale P _ _ _ (mixedAmplitude_nonneg P C R hC hR) (mixedRadius_nonneg R hR) (residualCost_pos P _ _ (mixedRadius_nonneg R hR)).
Equations
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Input data, given by input (EulerStaticCylinder.field P 1 u) (amplitude P C R hC hR).
Equations
- EulerStaticEuler.inputData P u C R hC hR = EulerSmallCorrection.input (EulerStaticCylinder.field P 1 u) (EulerStaticEuler.amplitude P C R hC hR)
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Correction budget, constructed using budget.
Equations
- EulerStaticEuler.correctionBudget P u C R hC hR hu hdiv = EulerSmallCorrection.budget (EulerStaticCylinder.field P 1 u) ⋯ ⋯ ⋯ (EulerStaticEuler.scales P C R hC hR) ⋯
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Exact packet, constructed using exactPacketOfResidual.
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With spatial scale one and angular direction zero, the zero-angle slice of the actual exact lifted solution solves ordinary three-dimensional Euler. The scalar pressure is the canonical normalized graph potential.
Cache the standard NormedAddCommGroup Space instance to shorten typeclass synthesis.
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Cache the standard NormedSpace ℝ Space instance to shorten typeclass synthesis.
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Cache the standard NormedAddCommGroup LiftTangent instance to shorten typeclass synthesis.
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Cache the standard NormedSpace ℝ LiftTangent instance to shorten typeclass synthesis.
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Inclusion, given by (ContinuousLinearMap.id ℝ ℝ).prodMap (ContinuousLinearMap.inl ℝ Space ℝ).
Equations
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Velocity, given by S.rawVelocity (q.1,(q.2,0)).
Equations
- EulerConstantEuler.velocity S q = S.rawVelocity (q.1, q.2, 0)
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Pressure, given by S.rawGraphPotential 1 q.
Equations
- EulerConstantEuler.pressure S q = S.rawGraphPotential 1 q
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Force, given by S.rawPressure (q.1,(q.2,0)).
Equations
- EulerConstantEuler.force S q = S.rawPressure (q.1, q.2, 0)
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Field, bundling field, smooth, integrable.
Equations
- EulerConstantEuler.field S t = { field := S.velocity.physicalPointField 1 0 t, smooth := ⋯, integrable := ⋯ }
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The genuine Euler time/amplitude scaling. A solution starting from ε u₀ on [0,1] gives a solution starting from u₀ on [0,ε].
Coordinates, given by ((ε⁻¹ • ContinuousLinearMap.id ℝ ℝ).comp (fst ℝ ℝ E)).prod (snd ℝ ℝ E).
Equations
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Velocity, given by ε⁻¹ • u (coordinates ε q).
Equations
- EulerTimeRescaling.velocity ε u q = ε⁻¹ • u ((EulerTimeRescaling.coordinates ε) q)
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Pressure, given by (ε⁻¹)^2*p (coordinates ε q).
Equations
- EulerTimeRescaling.pressure ε p q = ε⁻¹ ^ 2 * p ((EulerTimeRescaling.coordinates ε) q)
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A positive-time classical Euler solution constructed from a genuine solenoidal Gevrey datum. The initial velocity is the original datum, not its small multiple. All spatial derivative tensors remain continuous L² paths after the actual Euler time/amplitude rescaling.
Local velocity, given by EulerTimeRescaling.velocity (amplitude P C R hC hR) (EulerConstantEuler.velocity (exactPacket P u C R hC hR hu hdiv)).
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Local pressure, given by EulerTimeRescaling.pressure (amplitude P C R hC hR) (EulerConstantEuler.pressure (exactPacket P u C R hC hR hu hdiv)).
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Local force as an element of Space.
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Local field, constructed using SmoothL2Field.mapField.
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The locally constructed ordinary Euler solution supplies a concrete first parent, its label budget and its genuine particle inverse. All constants and the positive common horizon depend only on the input Gevrey envelope, not on the particular initial datum.
Actual smooth coefficient paths and their true time derivatives under the Euler amplitude/time scaling. The time interval is shortened by the same positive amplitude used to normalize the initial velocity.
Coefficient, given by (A.compTime (timeMap ε hε)).map (ε⁻¹ • ContinuousLinearMap.id ℝ V).
Equations
- EulerTimeRescaling.coefficient ε hε A = SmoothTimeField.map (ε⁻¹ • ContinuousLinearMap.id ℝ V) (A.compTime (EulerTimeRescaling.timeMap ε hε))
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Derivative coefficient, given by (A.compTime (timeMap ε hε)).map ((ε⁻¹)^2 • ContinuousLinearMap.id ℝ V).
Equations
- EulerTimeRescaling.derivativeCoefficient ε hε A = SmoothTimeField.map (ε⁻¹ ^ 2 • ContinuousLinearMap.id ℝ V) (A.compTime (EulerTimeRescaling.timeMap ε hε))
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The constructed static-datum solution and its actual time derivative have smooth bounded spatial jets continuous in time. This includes the one-sided derivatives at both endpoints.
Unit velocity coefficient as an element of SmoothTimeField (Icc (0 : ℝ) 1) Space Space.
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Unit derivative coefficient as an element of SmoothTimeField (Icc (0 : ℝ) 1) Space Space.
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Unit force coefficient, given by (exactPacket P u C R hC hR hu hdiv).pressure.toSmoothTimeField.precompLinear (ContinuousLinearMap.inl ℝ Space ℝ).
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Velocity coefficient, given by EulerTimeRescaling.coefficient (amplitude P C R hC hR) (amplitude_pos P C R hC hR) (unitVelocityCoefficient P u C R hC hR hu hdiv).
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Derivative coefficient, constructed using EulerTimeRescaling.derivativeCoefficient.
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Force coefficient, constructed using EulerTimeRescaling.derivativeCoefficient.
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Uniform source-only Gevrey bounds for the actual local Euler solution and its genuine time derivative. The same spatial radius works for sup and ordinary L² norms. All constants depend only on P,C,R, not on the particular solenoidal datum realizing the input bounds.
Explicit bounds for the constructed small-data solution. All constants are functions of the datum's supplied Gevrey bounds and the fixed period; none depends on which datum realizes those bounds.
A fixed positive radius retained by the actual correction.
Equations
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Base error factor, given by metricAmplification 1/2.
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Static source cost, given by sourceBound P 1 1 0 0 1 baseErrorFactor ((8/EulerSmallCorrection.initialRadius (mixedRadius R))*baseErrorFactor).
Equations
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Static time cost, given by (1+2*pressureBound*(448*1+1))*staticSourceCost P R.
Equations
- EulerStaticEuler.staticTimeCost P R = (1 + 2 * EulerConstantCorrection.pressureBound * (448 * 1 + 1)) * EulerStaticEuler.staticSourceCost P R
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Quantitative spatial jet bounds under actual Euler time/amplitude rescaling. The constants are explicit and the spatial radius is unchanged.
Cache the standard NormedAddCommGroup (E [×n]→L[ℝ] V) instance to shorten typeclass
synthesis.
Instances For
Cache the standard NormedSpace ℝ (E [×n]→L[ℝ] V) instance to shorten typeclass synthesis.
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Cache the standard NormedAddCommGroup (E →ᵇ (E [×n]→L[ℝ] V)) instance to shorten typeclass
synthesis.
Instances For
Cache the standard NormedSpace ℝ (E →ᵇ (E [×n]→L[ℝ] V)) instance to shorten typeclass
synthesis.
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Cache the standard NormedAddCommGroup Space instance to shorten typeclass synthesis.
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Cache the standard NormedSpace ℝ Space instance to shorten typeclass synthesis.
Instances For
Cache the standard NormedAddCommGroup (Space [×n]→L[ℝ] Space) instance to shorten
typeclass synthesis.
Instances For
Cache the standard NormedSpace ℝ (Space [×n]→L[ℝ] Space) instance to shorten typeclass
synthesis.
Instances For
Cache the standard NormedAddCommGroup (Space →ᵇ (Space [×n]→L[ℝ] Space)) instance to
shorten typeclass synthesis.
Instances For
Cache the standard NormedSpace ℝ (Space →ᵇ (Space [×n]→L[ℝ] Space)) instance to shorten
typeclass synthesis.
Instances For
Cover radius, given by ‖coordinateEquiv.symm.toContinuousLinearMap‖*(retainedRadius R)⁻¹.
Equations
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Graph cost, given by 1+sobolevEmbeddingConstant P 3+Real.sqrt (2/P+2*P)*(1+coverRadius R).
Equations
- EulerStaticEuler.graphCost P R = 1 + EulerCylinderSobolevSpace.sobolevEmbeddingConstant P 3 + √(2 / P + 2 * P) * (1 + EulerStaticEuler.coverRadius R)
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Output derivative size, given by (amplitude P C R hC hR)⁻¹*graphCost P R*staticTimeCost P R.
Equations
- EulerStaticEuler.outputDerivativeSize P C R hC hR = (EulerStaticEuler.amplitude P C R hC hR)⁻¹ * EulerStaticEuler.graphCost P R * EulerStaticEuler.staticTimeCost P R
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Local derivative field, constructed using SmoothL2Field.mapField.
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The genuine ordinary flow of a smooth divergence-free velocity gives the first parent particle data. Its horizon can be shortened by an explicit positive amount before applying the uniform flow-jet estimate.
Cache the standard NormedAddCommGroup (Space [×n]→L[ℝ] Space) instance to shorten
typeclass synthesis.
Instances For
Cache the standard NormedSpace ℝ (Space [×n]→L[ℝ] Space) instance to shorten typeclass
synthesis.
Instances For
Cache the standard NormedAddCommGroup (Space →ᵇ (Space [×n]→L[ℝ] Space)) instance to
shorten typeclass synthesis.
Instances For
Cache the standard NormedSpace ℝ (Space →ᵇ (Space [×n]→L[ℝ] Space)) instance to shorten
typeclass synthesis.
Instances For
Input data, collecting T, T_pos, field, derivative, time_derivative, divergence
and their compatibility conditions.
- T : ℝ
Time horizon of
Input, of typeℝ. - field : SmoothTimeField (↑(Set.Icc 0 self.T)) EulerSmoothLimit.Space EulerSmoothLimit.Space
Underlying field of
Input, of typeSmoothTimeField (Icc (0 : ℝ) T) Space Space. - derivative : SmoothTimeField (↑(Set.Icc 0 self.T)) EulerSmoothLimit.Space EulerSmoothLimit.Space
Derivative field of
Input, of typeSmoothTimeField (Icc (0 : ℝ) T) Space Space. - time_derivative : SmoothTimeField.TimeDerivative self.T ⋯ self.field self.derivative
- divergence (t : ↑(Set.Icc 0 self.T)) (x : EulerSmoothLimit.Space) : EulerSmoothLimit.divergence (⇑(self.field.field t)) x = 0
- B : ℝ
Bound parameter of
Input, of typeℝ. - R : ℝ
Radius parameter of
Input, of typeℝ.
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Velocity, given by I.field.compDisplacement I.displacement.
Equations
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Acceleration, given by accelerationCoefficient I.T I.T_pos.le I.field I.B I.R I.B_nonneg I.R_pos I.small I.bound I.derivative.
Equations
- I.acceleration = EulerSmoothBanachFlow.accelerationCoefficient I.T ⋯ I.field I.B I.R ⋯ ⋯ ⋯ ⋯ I.derivative
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Particle inverse, bundling field, left_inverse, right_inverse, continuous and the
required compatibility proofs.
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Of interval, bundling T, T_pos, field, derivative and the required compatibility
proofs.
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The three actual base-flow fields satisfy the source's fixed-H6 label bound with one explicit constant, independent of derivative order.
Actual ordinary L² displacement, material velocity and acceleration for the base flow. The displacement estimate integrates the real spatial jets of the flow, and the other two estimates use volume preservation.
Cache the standard NormedAddCommGroup (Space [×n]→L[ℝ] Space) instance to shorten
typeclass synthesis.
Instances For
Cache the standard NormedSpace ℝ (Space [×n]→L[ℝ] Space) instance to shorten typeclass
synthesis.
Instances For
Cache the standard NormedAddCommGroup (Space →ᵇ (Space [×n]→L[ℝ] Space)) instance to
shorten typeclass synthesis.
Instances For
Cache the standard NormedSpace ℝ (Space →ᵇ (Space [×n]→L[ℝ] Space)) instance to shorten
typeclass synthesis.
Instances For
L² data, collecting velocity, derivative, velocity_match, derivative_match, C, S
and their compatibility conditions.
- velocity : ↑(Set.Icc 0 I.T) → EulerLpTranslation.SmoothL2Field EulerSmoothLimit.Space
- derivative : ↑(Set.Icc 0 I.T) → EulerLpTranslation.SmoothL2Field EulerSmoothLimit.Space
- derivative_match (t : ↑(Set.Icc 0 I.T)) (x : EulerSmoothLimit.Space) : (self.derivative t).field x = (I.derivative.field t) x
- C : ℝ
Bound coefficient of
L2Data, of typeℝ. - S : ℝ
- C₁ : ℝ
First-derivative bound coefficient of
L2Data, of typeℝ. - S₁ : ℝ
- derivative_bound (t : ↑(Set.Icc 0 I.T)) : (self.derivative t).HasJetBound self.C₁ self.S₁
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Velocity field, constructed using SmoothL2Field.composeField.
Equations
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Displacement field, bundling field, smooth, integrable.
Equations
- L.displacementField t = { field := ⇑(I.displacement.field t), smooth := ⋯, integrable := ⋯ }
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Acceleration product, constructed using SmoothL2Field.productField.
Equations
- L.accelerationProduct t = EulerLpTranslation.SmoothL2Field.productField (fderiv ℝ ⇑(I.field.field t)) ⋯ (L.velocity t) (I.B * I.R) L.C L.accelerationSourceRadius ⋯ ⋯ ⋯ ⋯ ⋯
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Acceleration source, given by SmoothL2Field.addField (L.derivative t) (L.accelerationProduct t).
Equations
- L.accelerationSource t = (L.derivative t).addField (L.accelerationProduct t)
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Acceleration radius, given by flowRadius I.B I.R I.T L.accelerationSourceRadius.
Equations
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Acceleration field, constructed using SmoothL2Field.composeField.
Equations
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Label cost, constructed using 1.
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Label data, bundling K, K_one, displacement, velocity and the required compatibility
proofs.
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Odd initial velocity produces the actual odd local Euler velocity and odd pressure force. The scalar pressure, normalized at the origin, is even. These are consequences of correction uniqueness.
Odd static data give the genuine parity hypotheses of the constructed correction. In particular the actual convection residual is odd; this is proved from its derivative formula.
The actual local Euler velocity and pressure force agree with the constructed smooth coefficient paths. In particular the local velocity has a true one-sided time derivative at the initial and terminal times.
Oddness of the genuine base velocity propagates through its actual flow to the base parent, using ODE uniqueness.
Base time, given by EulerBaseEulerParent.horizon (amplitude P C R hC hR) (outputVelocitySize P C R) (outputRadius R).
Equations
- EulerStaticEuler.baseTime P C R hC hR = EulerBaseEulerParent.horizon (EulerStaticEuler.amplitude P C R hC hR) (EulerStaticEuler.outputVelocitySize P C R) (EulerStaticEuler.outputRadius R)
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Base inclusion, given by initialInclusion _ _ (baseTime_le P C R hC hR).
Equations
- EulerStaticEuler.baseInclusion P C R hC hR = EulerTimeIntervalRestriction.initialInclusion (EulerStaticEuler.amplitude P C R hC hR) (EulerStaticEuler.baseTime P C R hC hR) ⋯
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Base input, constructed using EulerBaseEulerParent.ofInterval.
Equations
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Base L² data, bundling velocity, derivative, velocity_match, derivative_match and
the required compatibility proofs.
Equations
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Base parent, given by (baseInput P u C R hC hR hu hdiv).parent ell hell hell1.
Equations
- EulerStaticEuler.baseParent P u C R hC hR hu hdiv ell hell hell1 = (EulerStaticEuler.baseInput P u C R hC hR hu hdiv).parent ell hell hell1
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Base label data, given by (baseL2Data P u C R hC hR hu hdiv).labelData ell hell hell1.
Equations
- EulerStaticEuler.baseLabelData P u C R hC hR hu hdiv ell hell hell1 = (EulerStaticEuler.baseL2Data P u C R hC hR hu hdiv).labelData ell hell hell1
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Base inverse, given by (baseInput P u C R hC hR hu hdiv).particleInverse ell hell hell1.
Equations
- EulerStaticEuler.baseInverse P u C R hC hR hu hdiv ell hell hell1 = (EulerStaticEuler.baseInput P u C R hC hR hu hdiv).particleInverse ell hell hell1
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Base evolution, bundling inverse, velocity, pressure, force and the required
compatibility proofs.
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The actual compact base datum has factorial bounds uniform in the small transverse parameter. All constants use the fixed cutoff only.
The compact initial velocity in the manuscript is constructed using the fixed factorial-bounded outer cutoff and the actual curl potential.
Potential, given by outerCutoff x*linearPotential L i x.
Equations
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Velocity, given by curl (potential L).
Equations
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Field, bundling field, smooth, integrable.
Equations
- EulerBaseDatum.field L = { field := EulerBaseDatum.velocity L, smooth := ⋯, integrable := ⋯ }
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Linear, given by (EuclideanSpace.proj 1).smulRight (EuclideanSpace.single 0 1+β • EuclideanSpace.single 2 1).
Equations
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Pointwise factorial estimates suffice when one factor has compact support. In particular polynomial factors need not be globally bounded.
Compact support turns actual uniform tensor bounds into the ordinary L² tensor bounds used in the label Sobolev estimates.
Cutoff amplitude, given by (9*(1+3/EulerGevreyCutoff.bumpMass)^2)^3.
Equations
- EulerBaseDatum.cutoffAmplitude = (9 * (1 + 3 / EulerGevreyCutoff.bumpMass) ^ 2) ^ 3
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Potential amplitude, given by 3*cutoffAmplitude*(24*‖L‖).
Equations
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Vector potential, given by ∑ i : Fin 3, potential L i x • EuclideanSpace.single i 1.
Equations
- EulerBaseDatum.vectorPotential L x = ∑ i : Fin 3, EulerBaseDatum.potential L i x • EuclideanSpace.single i 1
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Velocity amplitude, given by ‖curlOperator‖*(3*potentialAmplitude L*256).
Equations
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Volume factor, given by (volume (Metric.closedBall (0 : Space) 2)).toReal^(1/2 : ℝ).
Equations
- EulerBaseDatum.volumeFactor = (MeasureTheory.volume (Metric.closedBall 0 2)).toReal ^ (1 / 2)
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A single positive time and a single label bound work for every compact base datum with |β|≤1. The parent, inverse and Euler evolution below are the actual constructed objects.
A single factorial budget for every base datum with |β|≤1. In particular this covers β=x₀⁻² with x₀≥1, independently of the eventual frequency and iteration scales.
Uniform amplitude, given by 1+‖curlOperator‖*(3*(3*cutoffAmplitude*(24*2))*256).
Equations
- EulerBaseDatum.uniformAmplitude = 1 + ‖EulerPacketPiola.curlOperator‖ * (3 * (3 * EulerBaseDatum.cutoffAmplitude * (24 * 2)) * 256)
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Uniform L² amplitude, given by uniformAmplitude*volumeFactor.
Equations
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Uniform label bound, given by 1+sobolevCoefficientAmplitude (Fin 3) 6 1024 uniformL2Amplitude + sobolevCoefficientRadius (Fin 3) 1024.
Equations
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Solution time, given by EulerStaticEuler.baseTime 1 uniformL2Amplitude 1024 uniformL2Amplitude_nonneg (by norm_num).
Equations
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Solution label constant, given by EulerStaticEuler.baseLabelConstant 1 uniformL2Amplitude 1024 uniformL2Amplitude_nonneg (by norm_num).
Equations
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Solution parent, constructed using EulerStaticEuler.baseParent.
Equations
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Solution label data, constructed using EulerStaticEuler.baseLabelData.
Equations
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Solution inverse, constructed using EulerStaticEuler.baseInverse.
Equations
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Solution evolution, constructed using EulerStaticEuler.baseEvolution.
Equations
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The actual normalized Euler pressure force has smooth ordinary L² slices, with all derivative tensors continuous in time.
Local force field, constructed using SmoothL2Field.mapField.
Equations
- One or more equations did not get rendered due to their size.
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The concrete local base evolution has actual continuous L² jets for both velocity and pressure force. Consequently its Euler equation holds strongly in every finite Sobolev order, including endpoint derivatives.
Base sobolev data, bundling velocity, force, velocity_match, force_match and the
required compatibility proofs.
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Solution sobolev data, constructed using EulerStaticEuler.baseSobolevData.
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Initial parent, given by (solutionParent β hβ ell hell hell1).restrictTime initialTime initialTime_pos initialTime_le.
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Initial label data, given by (solutionLabelData β hβ ell hell hell1).restrictTime initialTime initialTime_pos initialTime_le.
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Initial inverse, given by (solutionInverse β hβ ell hell hell1).restrictTime initialTime initialTime_pos initialTime_le.
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Initial evolution, given by (solutionEvolution β hβ ell hell hell1).restrictTime initialTime initialTime_pos initialTime_le.
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Initial sobolev data, given by (solutionSobolevData β hβ ell hell hell1).restrictTime initialTime initialTime_pos initialTime_le.
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Initial low bounds, given by lowBounds (solutionLabelData β hβ ell hell hell1).
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- EulerBaseDatum.initialLowBounds β hβ ell hell hell1 = EulerBaseEulerGuards.lowBounds (EulerBaseDatum.solutionLabelData β hβ ell hell hell1)