OAI/Analysis/Mahler/SourceRadiusFlux.lean
5 declarations, 0 contain sorry, 0 declared as axioms
- lemma
OAI.Mahler.continuousOn_sourceFluxForm_sphereline 12 - theorem
OAI.Mahler.sphereFlux_pos_eq_coordinateFluxline 19Source documentation
Positive dilation of the coordinate integral uses the tangential degree 2k+1, with no change in the outward orientation.
theorem sphereFlux_pos_eq_coordinateFlux {k : ℕ} {r : ℝ} (hr : 0 < r) (B : ComplexEuclidean (k+1) → ComplexEuclidean (k+1) [⋀^Fin (2*k+1)]→L[ℝ] ℂ) (hB : ContinuousOn B (sphere 0 r)) : MahlerStokes.sphereFlux r (fluxPullback B) = r^(2*k+1) * sphereFlux k (fun x => (B (r • x)).toAlternatingMap) := by …Mentions: OAI.Mahler.ComplexEuclidean, OAI.MahlerStokes.sphereFlux, OAI.Mahler.fluxPullback, OAI.Mahler.sphereFlux
- theorem
OAI.Mahler.sourceCoordinateFlux_eq_radiusSphereFluxline 37Source documentation
The coordinate Stokes flux equals the real part of the radius-sphere area integral. C3 is required only at the radius sphere.
theorem sourceCoordinateFlux_eq_radiusSphereFlux {k : ℕ} {u : ComplexEuclidean (k+1) → ℂ} {r : ℝ} (hr : 0 < r) (hu : ∀ z ∈ sphere (0 : ComplexEuclidean (k+1)) r, ContDiffAt ℝ 3 u z) : MahlerStokes.sphereFlux r (sourceCoordinateForm (sourceCoordinates k) u k) = (radiusSphereFlux k u r).re := by …Mentions: OAI.Mahler.ComplexEuclidean, OAI.MahlerStokes.sphereFlux, OAI.Mahler.sourceCoordinateForm, OAI.Mahler.sourceCoordinates, OAI.Mahler.radiusSphereFlux
- theorem
OAI.Mahler.MassHypotheses.sourceCoordinateFlux_eq_radiusSphereFluxline 81Source documentation
The mass hypotheses supply every regularity premise. Only the positive radius and inclusion of its sphere in the source domain remain.
theorem MassHypotheses.sourceCoordinateFlux_eq_radiusSphereFlux {k N m : ℕ} {U : Set (ComplexEuclidean (k+1))} {f : Fin N → ComplexEuclidean (k+1) → ℂ} {G : Fin N → MvPolynomial (Fin (k+1)) ℂ} (h : MassHypotheses (k+1) N m U f G) {r : ℝ} (hr : 0 < r) (hSU : sphere (0 : ComplexEuclidean (k+1)) r ⊆ U) : MahlerStokes.sphereFlux r (sourceCoordinateForm (sourceCoordinates k) (logTau f) k) = (radiusSphereFlux k (logTau f) r).re := by …Mentions: OAI.Mahler.ComplexEuclidean, OAI.Mahler.MassHypotheses, OAI.MahlerStokes.sphereFlux, OAI.Mahler.sourceCoordinateForm, OAI.Mahler.sourceCoordinates, OAI.Mahler.logTau, OAI.Mahler.radiusSphereFlux
- theorem
OAI.Mahler.MassHypotheses.sourceCoordinateFlux_limitline 96Source documentation
The coordinate small-sphere limit, with no flux-bridge premise.
theorem MassHypotheses.sourceCoordinateFlux_limit {k N m : ℕ} {U : Set (ComplexEuclidean (k+1))} {f : Fin N → ComplexEuclidean (k+1) → ℂ} {G : Fin N → MvPolynomial (Fin (k+1)) ℂ} (h : MassHypotheses (k+1) N m U f G) : Tendsto (fun r => MahlerStokes.sphereFlux r (sourceCoordinateForm (sourceCoordinates k) (logTau f) k)) (𝓝[>] 0) (𝓝 (homogeneousSphereFlux k N G)) := by …Mentions: OAI.Mahler.ComplexEuclidean, OAI.Mahler.MassHypotheses, OAI.MahlerStokes.sphereFlux, OAI.Mahler.sourceCoordinateForm, OAI.Mahler.sourceCoordinates, OAI.Mahler.logTau, OAI.Mahler.homogeneousSphereFlux