OAI.Mahler.MassHypotheses.homogeneous_flux_endpoints: intermediate lemma from OpenAI, The symmetric Mahler conjecture and its equality cases
ProvedOAI.Mahler.MassHypotheses.homogeneous_flux_endpointsAn intermediate lemma of the split of OpenAI's proof of OAI.SymmetricMahler.symmetric_mahler, carved from OpenAI's openai/math development for this platform. The statement and its proof are OpenAI's (OpenAI, The symmetric Mahler conjecture and its equality cases, OpenAI Math Release, September 22, 2026, result family 87, github.com/openai/math, Apache License 2.0); in Lean it is the declaration OAI.Mahler.MassHypotheses.homogeneous_flux_endpoints of lean/OAI/Analysis/Mahler/Mahler/HomogeneousEndpoint.lean at commit adc7f12, ported to Lean 4.33.1 and Mathlib 0df444a.
The statement, as published (namespace OAI.Mahler, with open Set Filter Metric, open scoped Topology):
theorem MassHypotheses.homogeneous_flux_endpoints {k N m : ℕ}
{U : Set (ComplexEuclidean (k+2))} {f : Fin N → ComplexEuclidean (k+2) → ℂ}
{G : Fin N → MvPolynomial (Fin (k+2)) ℂ} (h : MassHypotheses (k+2) N m U f G) :
homogeneousSphereFlux (k+1) N G = (Real.pi*(m:ℝ))^(k+2) ∧
Tendsto (fun r => (radiusSphereFlux (k+1) (logTau f) r).re)
(𝓝[>] (0:ℝ)) (𝓝 ((Real.pi*(m:ℝ))^(k+2)))
Definitions. The statement is written with OAI.Mahler.ComplexEuclidean, OAI.Mahler.MassHypotheses, OAI.Mahler.homogeneousSphereFlux, OAI.Mahler.logTau and OAI.Mahler.radiusSphereFlux (definitions bundle OAISMh000 of this split).
Used by. The proof of OAI.Mahler.MassHypotheses.homogeneousSphereFlux_value of this split imports it.
import Mathlib import Definitions.Def_OAISMh000
section
attribute [-instance] _root_.OAI.Mahler.finiteDimensional_continuousAlternatingMap
set_option linter.all false
set_option linter.unusedVariables false
set_option linter.unusedTactic false
set_option linter.unreachableTactic false
namespace OAI
noncomputable section
open Set Filter Metric
open scoped Topology
namespace Mahler
theorem MassHypotheses.homogeneous_flux_endpoints {k N m : ℕ}
{U : Set (ComplexEuclidean (k+2))} {f : Fin N → ComplexEuclidean (k+2) → ℂ}
{G : Fin N → MvPolynomial (Fin (k+2)) ℂ} (h : MassHypotheses (k+2) N m U f G) :
homogeneousSphereFlux (k+1) N G = (Real.pi*(m:ℝ))^(k+2) ∧
Tendsto (fun r => (radiusSphereFlux (k+1) (logTau f) r).re)
(𝓝[>] (0:ℝ)) (𝓝 ((Real.pi*(m:ℝ))^(k+2))) := by
sorry
end Mahler
end
end OAI
end