The actual finite pressure Hessian is its primary normal tensor plus a uniform inverse-frequency error. No derivative or remainder estimate is assumed for a solved field.
The initialized finite pressure has its actual leading angular force and a uniformly small covector remainder.
Initialized angular pressure, defined pointwise by (pressureJet (scalar τ hτ hτT B (initialData D δ hδ (α • ξ) hs)) z).2 angleDirection.
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Initialized covector remainder, given by covectorRemainder (N := N) (a := initializedProfiles M D τ hτ hτT B δ hδ ξ hs α) D.m₀ κ.
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- EulerPacketTerminalDatum.initializedCovectorRemainder M D τ hτ hτT B δ hδ ξ hs α N κ = EulerPacketPressure.covectorRemainder D.m₀ κ
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Initialized pressure budget, constructed using Classical.choice.
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- EulerPacketTerminalDatum.initializedPressureBudget M D hTime τ hτ hτT B δ hδ ξ hs α L H NB W LM WM BC hRc hcost hδ1 hα hR WP S hgrowth p = Classical.choice ⋯
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Initialized angular pressure field as an element of Field period D.T (fun z => initializedAngularPressure D τ hτ hτT B δ hδ ξ hs α z • D.m₀).
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Initialized covector remainder field as an element of Field period D.T (initializedCovectorRemainder M D τ hτ hτT B δ hδ ξ hs α N κ).
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The leading pressure tensor of the actual joined primary. Both angular derivatives below are derivatives of its constructed scalar pressure.
Coefficient, given by -(2*a*⟪D.normal.field t x, D.M.field t x (canonicalVelocity τ hτ hτT B ξ hs t x)⟫_ℝ)/‖D.normal.field t x‖^2.
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Physical pressure, given by k⁻¹^2 * scalar τ hτ hτT B (initialData D δ hδ (a • ξ) hs) (t,(Y x,k*⟪D.m₀,Y x⟫_ℝ)).
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Hessian remainder, given by lowerHessian (fun z => scalar τ hτ hτT B (initialData D δ hδ (a • ξ) hs) (t,z)) k D.m₀ Y (fun y => D.FInv.field t (Y y)) x.
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The leading term is the literal normal tensor in source (20); the remainder contains only terms with at least one factor of k⁻¹.
Initialized pressure hessian cost, constructed using fastHessianCost.
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