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Papers.AnsariRockelSteinmassl2026RhoGamma.ElementaryArc

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The elementary boundary arc and the exact half-shift regime #

The source's polynomial elementary arc, with d equal to half the corner length.

Corollary 2.1's radical formula at every elementary-arc parameter.

Every gamma below the first contact, apart from W, has a half-shift parameter.

Corollary 2.1: the closed formula on the whole elementary gamma interval.

theorem Papers.AnsariRockelSteinmassl2026RhoGamma.halfShift_not_optimal {s : ℝ} (hs : 0 < s) (hs1 : s < 1) :
∃ (C : ProbabilityTheory.Copula 2), ∫ (x : Fin 2 → ↑unitInterval), (↑(x 0) - ↑(x 1)) ^ 2 - s * |↑(x 0) - ↑(x 1)| ∂C.toMeasure < ∫ (x : Fin 2 → ↑unitInterval), (↑(x 0) - ↑(x 1)) ^ 2 - s * |↑(x 0) - ↑(x 1)| ∂ProbabilityTheory.Copula.RankRegion.RhoFootrule.halfTurn.toMeasure

An explicit competing copula improves the half-shift cost whenever 0<s<1.

theorem Papers.AnsariRockelSteinmassl2026RhoGamma.halfShift_optimal_iff {s : ℝ} (hs : 0 < s) :
(∀ (C : ProbabilityTheory.Copula 2), ∫ (x : Fin 2 → ↑unitInterval), (↑(x 0) - ↑(x 1)) ^ 2 - s * |↑(x 0) - ↑(x 1)| ∂ProbabilityTheory.Copula.RankRegion.RhoFootrule.halfTurn.toMeasure ≤ ∫ (x : Fin 2 → ↑unitInterval), (↑(x 0) - ↑(x 1)) ^ 2 - s * |↑(x 0) - ↑(x 1)| ∂C.toMeasure) ↔ 1 ≤ s

Lemma 3.6 in both directions, with s=1/theta.