OAI/GroupTheory/Kervaire/SpectralLogarithm.lean

GitHub source file

7 declarations, 0 contain sorry, 0 declared as axioms

  1. theorem OAI.KervaireSpectral.exists_phaseOperator line 19
  2. def OAI.KervaireSpectral.vectorCLM line 107

    Source documentation

    The continuous vector functional on all bounded operators.

    def vectorCLM (ξ : H) : Operator H →L[ℂ] ℂ :=
    …

    Mentions: OAI.KervaireSpectral.Operator

  3. theorem OAI.KervaireSpectral.vectorCLM_apply line 111
  4. theorem OAI.KervaireSpectral.vectorCLM_star line 115

    Source documentation

    The vector functional respects the star, without a trace assumption.

    theorem vectorCLM_star (ξ : H) (T : Operator H) :
        vectorCLM ξ (star T) = star (vectorCLM ξ T) := by
    …

    Mentions: OAI.KervaireSpectral.Operator, OAI.KervaireSpectral.vectorCLM

  5. theorem OAI.KervaireSpectral.vectorCLM_complexify_real line 122

    Source documentation

    Real continuous spectral functions have real vector expectations.

    theorem vectorCLM_complexify_real (U : Operator H) [hU : IsStarNormal U] (ξ : H)
        (f : C(spectrum ℂ U, ℝ)) :
        (((vectorCLM ξ (cfcHom hU (complexify f))).re : ℝ) : ℂ) =
          vectorCLM ξ (cfcHom hU (complexify f)) := by
    …

    Mentions: OAI.KervaireSpectral.Operator, OAI.KervaireSpectral.vectorCLM, OAI.KervaireSpectral.complexify

  6. theorem OAI.KervaireSpectral.integrable_continuous_map line 134

    Source documentation

    Every continuous function on the compact spectral space is integrable.

    theorem integrable_continuous_map {E : Type*} [NormedAddCommGroup E]
        (U : Operator H) [IsStarNormal U] (ξ : H) (f : C(spectrum ℂ U, E)) :
        Integrable f (vectorMeasure U ξ) := by
    …

    Mentions: OAI.KervaireSpectral.Operator, OAI.KervaireSpectral.vectorMeasure

  7. theorem OAI.KervaireSpectral.integral_vectorMeasure_complex line 141

    Source documentation

    The scalar spectral measure integrates complex functions as well as real ones.

    theorem integral_vectorMeasure_complex (U : Operator H) [hU : IsStarNormal U] (ξ : H)
        (f : C(spectrum ℂ U, ℂ)) :
        ∫ z, f z ∂vectorMeasure U ξ = vectorCLM ξ (cfcHom hU f) := by
    …

    Mentions: OAI.KervaireSpectral.Operator, OAI.KervaireSpectral.vectorMeasure, OAI.KervaireSpectral.vectorCLM