Canonical pressure of the physical terminal heat tail #
The heat parameter is the physical time 1-t. The pressure is the actual
improper radial integral. Its regularity is obtained by separating the pure
heat tail from a compact taper correction.
The exponent of the physical angular heat amplitude.
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Derivatives with respect to the actual scaled heat parameter.
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- NavierStokes.TerminalPressure.heatJet h n ν v = (2 / v) ^ n * NavierStokes.RadialHeatProfile.profileJet (1 + h) n (2 * ν / v)
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Heat pressure jet, given by pressureWeight h v * ParametricHeatTail.jetProduct (fun i => heatJet h i ν v) (fun i => heatJet h i ν v) n.
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Dimensionless pure-heat pressure integral, including the zero-diffusion endpoint.
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- NavierStokes.TerminalPressure.heatPressureFactor h ν = ∫ (v : ℝ) in Set.Ioi 1, NavierStokes.TerminalPressure.pressureWeight h v * NavierStokes.RadialHeatProfile.profile (1 + h) (2 * ν / v) ^ 2
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Every derivative of the heat-only improper integral is dominated by an integrable power, uniformly all the way to zero diffusion.
The compact taper correction #
Heat density, given by pressureWeight h v * RadialHeatProfile.profile (1 + h) (2 * ν / v) ^ 2.
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- NavierStokes.TerminalPressure.heatDensity h ν v = NavierStokes.TerminalPressure.pressureWeight h v * NavierStokes.RadialHeatProfile.profile (1 + h) (2 * ν / v) ^ 2
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Tapered density, given by heatDensity h p.1 v * f (p.2 + Real.log v) ^ 2.
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- NavierStokes.TerminalPressure.taperedDensity h f p v = NavierStokes.TerminalPressure.heatDensity h p.1 v * f (p.2 + Real.log v) ^ 2
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Deficit density, given by heatDensity h p.1 v * (1 - f (p.2 + Real.log v) ^ 2).
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- NavierStokes.TerminalPressure.deficitDensity h f p v = NavierStokes.TerminalPressure.heatDensity h p.1 v * (1 - f (p.2 + Real.log v) ^ 2)
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Tapered pressure factor, given by ∫ v in Ioi (1 : ℝ), taperedDensity h f p v.
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- NavierStokes.TerminalPressure.taperedPressureFactor h f p = ∫ (v : ℝ) in Set.Ioi 1, NavierStokes.TerminalPressure.taperedDensity h f p v
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Compact deficit, given by (B - 1) * ∫ u in (0 : ℝ)..1, deficitDensity h f p (1 + (B - 1) * u).
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Genuine joint smoothness of the tapered improper integral. Only the compact taper correction depends on the logarithmic radial coordinate.
Actual differentiation in the logarithmic radial parameter #
Taper derivative density, given by heatDensity h p.1 v * f (p.2 + Real.log v) * deriv f (p.2 + Real.log v).
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- NavierStokes.TerminalPressure.taperDerivativeDensity h f p v = NavierStokes.TerminalPressure.heatDensity h p.1 v * f (p.2 + Real.log v) * deriv f (p.2 + Real.log v)
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Taper derivative integral, given by ∫ v in Ioi (1 : ℝ), taperDerivativeDensity h f p v.
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The derivative is obtained from the defining improper integral; the derivative integrand is compactly supported by the actual taper plateau.
Identification with the physical canonical pressure #
Pressure coordinates, given by ((1 - p.1) / p.2.1, Real.log (SimilarityProfile.X h p)).
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- NavierStokes.TerminalPressure.pressureCoordinates h p = ((1 - p.1) / p.2.1, Real.log (NavierStokes.SimilarityProfile.X h p))
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Scaling is performed in the physical radial integral. In particular the
argument of the heat profile is 2(1-t)/s, rather than a fixed diffusion parameter.
The actual canonical pressure is jointly smooth throughout the presingular, positive-radius domain. No differentiability of the pressure is an input.
The axial derivative of the physical pressure #
Log scale derivative, given by CoordinateAlgebra.qAxial (SimilarityProfile.q h p) h (SimilarityProfile.eta h p) / SimilarityProfile.q h p.
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Axial pressure integral as an element of ℝ.
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Exact axial derivative of the canonical pressure, including the dependence
of the heat profile on the physical time and of the taper on q(t,z).
Quantitative pressure estimates from monotonicity of the heat carrier #
The actual outgoing taper and its terminal edge estimate #
Outgoing taper, given by OutgoingTail.tailShape d (y - y0).
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Outgoing pressure, given by TerminalStress.canonicalPressure (TerminalStress.swirlCoefficient C d.h (outgoingTaper d y0)).
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Fully expanded formula for the actual pressure derivative needed in the
terminal edge chart. The integration coordinate is the physical s=r^2/2.
Compact support of the terminal forcing and its positive mass #
A positive lower bound for the actual backward angular stress. Every tail integrability hypothesis is discharged using the taper's genuine plateau.
The genuine backward axial pressure stress #
Since ds = r dr, this is the cylindrical backward primitive with weight
r. It uses the actual axial derivative of the canonical pressure.
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Coarse angular/axial tilt on a fixed terminal annulus #
Tilt constant, given by (2 / (1 - 2 * h)) * (Λ - 1) / Λ ^ (-amplitudeExponent h).
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Actual backward stresses satisfy the coarse tilt estimate on any fixed
annulus. The factor q^(1-D) K is subsequently bounded by the released amplitude.
Uniform smallness from the constructed release #
The normalization is exactly the physical carrier normalization in
ParametricHeatTail.physicalEdit_heat_carrier.
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The actual parametric heat edit agrees with this module's physical carrier. The diffusion identity is proved from the physical similarity coordinates.
The bound is uniform in spacetime, in the terminal scale K, and in the
distance to the edge. The released amplitude contributes the proved factor h^4.
Full physical residual formula after discharging the pressure regularity and improper-integral assumptions. The axial viscosity of the swirl is retained.
The backward axial primitive has the required cylindrical divergence, computed from actual derivatives of the canonical pressure.