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Linear Dynamical Properties of Weighted Backward Shifts on Spaces of Real Analytic Functions Can Deha Karksz (joint work with late Pawe l Doma nski) Ozye gin University, Istanbul deha.kariksiz@ozyegin.edu.tr 03.07.2018


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Linear Dynamical Properties of Weighted Backward Shifts on Spaces of Real Analytic Functions

Can Deha Karıksız (joint work with late Pawe l Doma´ nski)

¨ Ozye˘ gin University, Istanbul deha.kariksiz@ozyegin.edu.tr

03.07.2018

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Outline

1 Introduction 2 Conditions on linear dynamical properties using dynamical

transference principles

3 Conditions on linear dynamical properties via eigenvalues

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Introduction

Linear Dynamical Properties

An operator T on a topological vector space X is called hypercyclic if there is some x ∈ X such that the set {x, Tx, T 2x, · · · , T nx, · · · }, called the orbit of x under T, is dense in X.

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Introduction

Linear Dynamical Properties

An operator T on a topological vector space X is called hypercyclic if there is some x ∈ X such that the set {x, Tx, T 2x, · · · , T nx, · · · }, called the orbit of x under T, is dense in X. topologically transitive if for any pair of nonempty open subsets U, V of X, there exists some n ∈ N such that T n(U) ∩ V = ∅.

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Introduction

Linear Dynamical Properties

An operator T on a topological vector space X is called mixing if for any pair of nonempty open subsets U, V of X, there exists some N ∈ N such that for every n ≥ N we have T n(U) ∩ V = ∅.

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Introduction

Linear Dynamical Properties

An operator T on a topological vector space X is called mixing if for any pair of nonempty open subsets U, V of X, there exists some N ∈ N such that for every n ≥ N we have T n(U) ∩ V = ∅. chaotic if T is topologically transitive and has a dense set of periodic points.

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Introduction

Weighted Backward Shifts on Fr´ echet Sequence Spaces

Let X be a Fr´ echet sequence space with canonical unit sequences

  • en. For a sequence of nonzero scalars ω = (ωn)n∈N, the operator

Bω : X → X defined by Bωen = ωnen−1, n ≥ 1, e0 = 0, is called a weighted backward shift on X.

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Introduction

Weighted Backward Shifts on Fr´ echet Sequence Spaces

Let X be a Fr´ echet sequence space with canonical unit sequences

  • en. For a sequence of nonzero scalars ω = (ωn)n∈N, the operator

Bω : X → X defined by Bωen = ωnen−1, n ≥ 1, e0 = 0, is called a weighted backward shift on X. Theorem Let Bω : X → X be a weighted backward shift acting on a Fr´ echet sequence space X in which (en)n∈N is a basis. (i) Bω is hypercyclic ⇔ there is an increasing sequence (nk)k∈N

  • f positive integers such that (nk

ν=1 ων)−1 enk → 0 in X as

k → ∞.

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Introduction

Weighted Backward Shifts on Fr´ echet Sequence Spaces

Let X be a Fr´ echet sequence space with canonical unit sequences

  • en. For a sequence of nonzero scalars ω = (ωn)n∈N, the operator

Bω : X → X defined by Bωen = ωnen−1, n ≥ 1, e0 = 0, is called a weighted backward shift on X. Theorem Let Bω : X → X be a weighted backward shift acting on a Fr´ echet sequence space X in which (en)n∈N is a basis. (i) Bω is hypercyclic ⇔ there is an increasing sequence (nk)k∈N

  • f positive integers such that (nk

ν=1 ων)−1 enk → 0 in X as

k → ∞. (ii) Bω is mixing ⇔ (n

ν=1 ων)−1 en → 0 in X as n → ∞.

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Introduction

Weighted Backward Shifts on Fr´ echet Sequence Spaces

Let X be a Fr´ echet sequence space with canonical unit sequences

  • en. For a sequence of nonzero scalars ω = (ωn)n∈N, the operator

Bω : X → X defined by Bωen = ωnen−1, n ≥ 1, e0 = 0, is called a weighted backward shift on X. Theorem Let Bω : X → X be a weighted backward shift acting on a Fr´ echet sequence space X in which (en)n∈N is an unconditional basis. (i) Bω is hypercyclic ⇔ there is an increasing sequence (nk)k∈N

  • f positive integers such that (nk

ν=1 ων)−1 enk → 0 in X as

k → ∞. (ii) Bω is mixing ⇔ (n

ν=1 ων)−1 en → 0 in X as n → ∞.

(iii) Bω is chaotic ⇔ ∞

n=1 (n ν=1 ων)−1 en converges in X.

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Introduction

Spaces of Real Analytic Functions

Let A(Ω) denote the space of all complex-valued real analytic functions on an open set Ω in R.

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Introduction

Spaces of Real Analytic Functions

Let A(Ω) denote the space of all complex-valued real analytic functions on an open set Ω in R. Equivalent Topologies on A(Ω) (Martineau 1966) Projective limit topology: A(Ω) = projN∈N H(KN) = projN∈N indn∈N H∞(UN,n), where (KN)N∈N is a compact increasing exhaustion of Ω, and (UN,n)n∈N are fundamental sequences of neighborhoods of KN for each N.

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Introduction

Spaces of Real Analytic Functions

Let A(Ω) denote the space of all complex-valued real analytic functions on an open set Ω in R. Equivalent Topologies on A(Ω) (Martineau 1966) Projective limit topology: A(Ω) = projN∈N H(KN) = projN∈N indn∈N H∞(UN,n), where (KN)N∈N is a compact increasing exhaustion of Ω, and (UN,n)n∈N are fundamental sequences of neighborhoods of KN for each N. Inductive limit topology: A(Ω) = ind H(U) where the inductive limit is taken over all complex neighborhoods of Ω.

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Introduction

Spaces of Real Analytic Functions

Main difficulties These locally convex topologies on A(Ω) are not metrizable, hence A(Ω) is not a Fr´ echet space. (Doma´ nski, Vogt 2000) A(Ω) has no Schauder basis.

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Introduction

Weighted Backward Shifts on A(Ω)

Definition Given a sequence of nonzero scalars ω = (ωn)n∈N, a continuous linear operator Bω : A(Ω) → A(Ω), that sends the monomials xn to ωn−1xn−1 for all n ≥ 1, the unit function to the zero function, is called a weighted backward shift with the weight sequence ω.

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Introduction

Weighted Backward Shifts on A(Ω)

Definition Given a sequence of nonzero scalars ω = (ωn)n∈N, a continuous linear operator Bω : A(Ω) → A(Ω), that sends the monomials xn to ωn−1xn−1 for all n ≥ 1, the unit function to the zero function, is called a weighted backward shift with the weight sequence ω. Problem: How to characterize well-defined weighted backward shifts on A(Ω)?

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Introduction

Hadamard Multipliers on A(Ω)

A linear continuous operator M : A(Ω) → A(Ω) is called a (Hadamard) multiplier whenever every monomial is an eigenvector.

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Introduction

Hadamard Multipliers on A(Ω)

A linear continuous operator M : A(Ω) → A(Ω) is called a (Hadamard) multiplier whenever every monomial is an eigenvector. Observation There is a one-to-one correspondence between the weighted backward shifts and the multipliers on A(Ω) whenever 0 ∈ Ω.

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Introduction

Hadamard Multipliers on A(Ω)

A linear continuous operator M : A(Ω) → A(Ω) is called a (Hadamard) multiplier whenever every monomial is an eigenvector. Observation There is a one-to-one correspondence between the weighted backward shifts and the multipliers on A(Ω) whenever 0 ∈ Ω. In this case, we can use the representation theorems for Hadamard multipliers on A(Ω) (Doma´ nski, Langenbruch 2012). Proposition Let Ω ⊂ R with 0 ∈ Ω be an open set. Then, TFAE: (i) Bω is a w.b.s. with the weight sequence ω = (ωn). (ii) Bω maps a function ∞

n=0 fnzn around zero into a real

analytic function on Ω represented around zero by the series ∞

n=0 fnωn−1zn−1.

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Conditions Using Dynamical Transference Principles

An operator T on X is called quasiconjugate to an operator S on Y via a continuous map φ : Y → X with dense range if T ◦ φ = φ ◦ S. Linear dynamical properties like hypercyclicity, mixing, and chaos are preserved under quasiconjugacy.

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Conditions Using Dynamical Transference Principles

An operator T on X is called quasiconjugate to an operator S on Y via a continuous map φ : Y → X with dense range if T ◦ φ = φ ◦ S. Linear dynamical properties like hypercyclicity, mixing, and chaos are preserved under quasiconjugacy. By considering Bω as an operator acting on the space H(C) of entire functions, and the space H({0}) of germs of holomorphic functions at zero, we obtain the following two quasiconjugacies. H(C)

− − → H(C) ↓ ↓ A(Ω)

− − → A(Ω) A(Ω)

− − → A(Ω) ↓ ↓ H({0})

− − → H({0})

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Conditions Using Dynamical Transference Principles

Using the quasiconjugacy involving H(C), we obtain the following sufficient conditions. Proposition (Doma´ nski, K. 2018) Let Ω ⊂ R be an open set with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms.

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Conditions Using Dynamical Transference Principles

Using the quasiconjugacy involving H(C), we obtain the following sufficient conditions. Proposition (Doma´ nski, K. 2018) Let Ω ⊂ R be an open set with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. (a) if there is a sequence (nk) such that for every R > 0, nk

  • ν=1

ων−1 −1 Rnk → 0 then Bω is hypercyclic.

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Conditions Using Dynamical Transference Principles

Using the quasiconjugacy involving H(C), we obtain the following sufficient conditions. Proposition (Doma´ nski, K. 2018) Let Ω ⊂ R be an open set with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. (a) if there is a sequence (nk) such that for every R > 0, nk

  • ν=1

ων−1 −1 Rnk → 0 then Bω is hypercyclic. (b) if for every R > 0,

  • n
  • ν=1

ων−1 −1 Rn → 0 then Bω is mixing and chaotic.

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Conditions Using Dynamical Transference Principles

Using the quasiconjugacy involving H({0}) and a construction due to Bonet, we obtain the following necessary conditions. Proposition (Doma´ nski, K. 2018) Let Ω ⊂ R be an open set with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms.

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Conditions Using Dynamical Transference Principles

Using the quasiconjugacy involving H({0}) and a construction due to Bonet, we obtain the following necessary conditions. Proposition (Doma´ nski, K. 2018) Let Ω ⊂ R be an open set with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. (a) if Bω is topologically transitive then there is a sequence (nk) and there is R > 0 such that nk

  • ν=1

ων−1 −1 Rnk → 0.

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Conditions Using Dynamical Transference Principles

Using the quasiconjugacy involving H({0}) and a construction due to Bonet, we obtain the following necessary conditions. Proposition (Doma´ nski, K. 2018) Let Ω ⊂ R be an open set with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. (a) if Bω is topologically transitive then there is a sequence (nk) and there is R > 0 such that nk

  • ν=1

ων−1 −1 Rnk → 0. (b) if Bω is mixing then there is R > 0 such that

  • n
  • ν=1

ων−1 −1 Rn → 0.

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Conditions Using Dynamical Transference Principles

Some Problems

Observation There are weight sequences satisfying the conditions nk

  • ν=1

ων−1 −1 Rnk → 0

  • r
  • n
  • ν=1

ων−1 −1 Rn → 0 for some R > 0, but not all R > 0.

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Conditions Using Dynamical Transference Principles

Some Problems

Observation There are weight sequences satisfying the conditions nk

  • ν=1

ων−1 −1 Rnk → 0

  • r
  • n
  • ν=1

ων−1 −1 Rn → 0 for some R > 0, but not all R > 0. Example If we take the unweighted backward shift on A(Ω), that is, ω = (ωn) where ωn = 1 for all n ∈ N, then

  • n
  • ν=1

ων−1 −1 Rn = Rn → 0 only for 0 < R < 1.

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Conditions using Eigenvalues

Godefroy-Shapiro criterion

Godefroy-Shapiro criterion Let T be an operator on a topological vector space X. If the subspaces X0 := span{x ∈ X : Tx = λx for some λ with |λ| < 1}, Y0 := span{x ∈ X : Tx = λx for some λ with |λ| > 1} are dense in X, then T is mixing. If, moreover, X is a complex space and the subspace Z0 := span{x ∈ X : Tx = eαπi for some rational α} is dense in X, then T is chaotic.

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Conditions using Eigenvalues

Description of Eigenvalues of A(Ω)

Definition A set U is called the star of holomorphy of a germ f ∈ H({0}) if it is a maximal star-like set in C around zero such that f extends holomorphically to V . A set U is star-like if for any z ∈ U we have {tz : t ∈ [0, 1]} ⊂ U.

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Conditions using Eigenvalues

Description of Eigenvalues of A(Ω)

Proposition Let Ω ⊆ R be an interval with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. If sup

n

  • n
  • ν=1

ων−1 −1 Rn < ∞ for some R > 0, then (i) zero is an eigenvalue with eigenspace of dimension one,

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Conditions using Eigenvalues

Description of Eigenvalues of A(Ω)

Proposition Let Ω ⊆ R be an interval with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. If sup

n

  • n
  • ν=1

ων−1 −1 Rn < ∞ for some R > 0, then (i) zero is an eigenvalue with eigenspace of dimension one, (ii) λ = 0 is an eigenvalue of Bω if and only if λΩ is contained in the star of holomorphy of the universal eigenfunction Eω(z) := zn+1 +

  • j=n+2
  • j−1
  • k=n+1

ωk −1 zj.

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Conditions using Eigenvalues

Description of Eigenvalues of A(Ω)

Proposition Let Ω ⊆ R be an interval with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. If sup

n

  • n
  • ν=1

ων−1 −1 Rn < ∞ for some R > 0, then (i) zero is an eigenvalue with eigenspace of dimension one, (ii) λ = 0 is an eigenvalue of Bω if and only if λΩ is contained in the star of holomorphy of the universal eigenfunction Eω(z) := zn+1 +

  • j=n+2
  • j−1
  • k=n+1

ωk −1 zj. If λ = 0 is an eigenvalue of Bω, then its eigenspace is

  • ne-dimensional, spanned by the function fλ(z) := Eω(λz).
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Conditions using Eigenvalues

Application of Godefroy-Shapiro Criterion

Theorem (Doma´ nski, K. 2018) Let Ω ⊆ R be an interval with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. (a) If Bω has a universal eigenfunction such that its star of holomorphy contains at least one interval λΩ for some λ ∈ C with |λ| > 1, then Bω is mixing.

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Conditions using Eigenvalues

Application of Godefroy-Shapiro Criterion

Theorem (Doma´ nski, K. 2018) Let Ω ⊆ R be an interval with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. (a) If Bω has a universal eigenfunction such that its star of holomorphy contains at least one interval λΩ for some λ ∈ C with |λ| > 1, then Bω is mixing. (b) If additionally to (a) the star of holomorphy of the universal eigenfunction contains a strip {z ∈ C : |z − tλ| < ε for some t ∈ R} for some ε > 0, then Bω is also hypercyclic.

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Conditions using Eigenvalues

Application of Godefroy-Shapiro Criterion

Theorem (Doma´ nski, K. 2018) Let Ω ⊆ R be an interval with 0 ∈ Ω, and Bω : A(Ω) → A(Ω) be a weighted backward shift such that ω has no zero terms. (a) If Bω has a universal eigenfunction such that its star of holomorphy contains at least one interval λΩ for some λ ∈ C with |λ| > 1, then Bω is mixing. (b) If additionally to (a) the star of holomorphy of the universal eigenfunction contains a strip {z ∈ C : |z − tλ| < ε for some t ∈ R} for some ε > 0, then Bω is also hypercyclic. (c) If additionally to (a) the star of holomorphy of the universal eigenfunction contains a set of the form {teπai : t ∈ Ω, a ∈ (a1, a2)} for some −∞ < a1 < a2 < ∞ then Bω is also chaotic.

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Conditions using Eigenvalues

Some Examples

Examples Let Ω be an interval containing zero. The following weighted backward shifts are chaotic, mixing, and hypercyclic. (i) the unweighted shift B1,

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Conditions using Eigenvalues

Some Examples

Examples Let Ω be an interval containing zero. The following weighted backward shifts are chaotic, mixing, and hypercyclic. (i) the unweighted shift B1, (ii) the differentiation operator D : A(Ω) → A(Ω) which corresponds to the weighted shift with ωn = n + 1,

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Conditions using Eigenvalues

Some Examples

Examples Let Ω be an interval containing zero. The following weighted backward shifts are chaotic, mixing, and hypercyclic. (i) the unweighted shift B1, (ii) the differentiation operator D : A(Ω) → A(Ω) which corresponds to the weighted shift with ωn = n + 1, (iii) the weighted backward shift Qk : A(Ω) → A(Ω), k > 0, Qk(f )(z) = 1

0 f ′(zt)tk dt which corresponds to the weighted

backward shift with ωn =

n+1 n+1+k .

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References I

  • P. Doma´

nski, C.D. Karıksız, Eigenvalues and dynamical properties of weighted backward shifts on the space of real analytic functions, Studia Math. 242 (2018), 57–78.

  • P. Doma´

nski, M. Langenbruch, Representation of multipliers

  • n spaces of real analytic functions, Analysis 32 (2012),

137–162.

  • P. Doma´

nski, D. Vogt, The space of real-analytic functions has no basis, Studia Math. 142 (2) (2000), 187–200.

  • A. Martineau, Sur la topologie des espaces de fonctions

holomorphes, Math. Ann. 163 (1966), 62–88.

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The End