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Copula.KendallDistribution

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Kendall distributions #

The Kendall distribution is the law of C(U) when U has copula C. It is defined in every finite dimension, including zero. Its CDF uses closed lower intervals, so an atom at zero is retained (as for countermonotonicity).

The probability law of the copula CDF evaluated at a draw from the copula.

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    noncomputable def ProbabilityTheory.Copula.kendallCDF {d : ℕ} (C : Copula d) :
    ℝ → ℝ

    Kendall's distribution function K_C(t) = P(C(U) ≤ t).

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    Instances For
      theorem ProbabilityTheory.Copula.kendallCDF_of_neg {d : ℕ} (C : Copula d) {t : ℝ} (ht : t < 0) :
      theorem ProbabilityTheory.Copula.kendallCDF_of_one_le {d : ℕ} (C : Copula d) {t : ℝ} (ht : 1 ≤ t) :
      theorem ProbabilityTheory.Copula.le_kendallCDF {d : ℕ} [NeZero d] (C : Copula d) (t : ↑unitInterval) :
      ↑t ≤ C.kendallCDF ↑t

      A nonempty copula's Kendall distribution stochastically lies below uniform.

      theorem ProbabilityTheory.Copula.integral_kendallDistribution {d : ℕ} (C : Copula d) (f : ℝ → ℝ) (hf : Measurable f) :
      ∫ (t : ℝ), f t ∂↑C.kendallDistribution = ∫ (x : Fin d → ↑unitInterval), f (C.cdf x) ∂C.toMeasure

      Integration against the Kendall law is integration of the CDF transform.

      @[simp]

      Dimension zero gives the constant CDF value one, rather than a uniform Kendall law.

      All natural moments of the independent copula's Kendall law, including dimension zero.

      @[simp]

      Countermonotonicity has an atom of mass one at zero, not K_W(0) = 0.