Section IX.3

Star-Cyclic Normal Operators

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Problem IX.3.1

If μ\mu is a compactly supported measure on C\mathbb {C} and f∈L2(μ)f \in L^2(\mu ), ff is a star-cyclic vector for NμN_\mu if and only if μ({x:f(x)=0})=0\mu (\{ x : f(x) = 0\} ) = 0.

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Problem IX.3.2

Prove the following proposition (Proposition 3.2).

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(a)

A vector e0e_0 is a star-cyclic vector for AA if and only if H=cl⁡{Te0:T∈C∗(A)}\mathcal{H} = \operatorname {cl}\{ Te_0 : T \in C^*(A)\}, where C∗(A)=C^*(A) = the C∗C^*-algebra generated by AA.

(b)

A vector e0e_0 is a cyclic vector for AA if and only if H=cl⁡{p(A)e0:p=a polynomial}\mathcal{H} = \operatorname {cl}\{ p(A)e_0 : p = \text{a polynomial}\}.

Problem IX.3.3

If μ1\mu_1 and μ2\mu_2 are compactly supported measures on C\mathbb {C}, show that the following statements are equivalent.

  1. μ1\mu_1 and μ2\mu_2 are boundedly mutually absolutely continuous.

  2. There is an isomorphism V:L2(μ1)→L2(μ2)V: L^2(\mu_1) \to L^2(\mu_2) such that VNμ1V−1=Nμ2VN_{\mu_1}V^{-1} = N_{\mu_2} and VL∞(μ1)=L∞(μ2)VL^\infty (\mu_1) = L^\infty (\mu_2).

  3. There is a bounded bijection R:L2(μ1)→L2(μ2)R: L^2(\mu_1) \to L^2(\mu_2) such that Rp(z,zˉ)=p(z,zˉ)Rp(z, \bar{z}) = p(z, \bar{z}) for every polynomial in zz and zˉ\bar{z}.

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Problem IX.3.4

Show that if NN is a star-cyclic normal operator and λ∈σp(N)\lambda \in \sigma_p(N), then dim⁡ker⁡(N−λ)=1\dim \ker (N - \lambda ) = 1.

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Problem IX.3.5

If NN is diagonalizable and star-cyclic and if σp(N)={λ1,λ2,… }\sigma_p(N) = \{ \lambda_1, \lambda_2, \dots \}, show that NN is unitarily equivalent to NμN_\mu, where μ=∑n=1∞2−nδλn\mu = \sum_{n=1}^\infty 2^{-n} \delta_{\lambda_n} (see Exercise 2.11).

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Problem IX.3.6

Let NN be a diagonalizable normal operator. Show that N≅MN \cong M if and only if MM is a diagonalizable normal operator, σp(N)=σp(M)\sigma_p(N) = \sigma_p(M), and dim⁡ker⁡(N−λ)=dim⁡ker⁡(M−λ)\dim \ker (N - \lambda ) = \dim \ker (M - \lambda ) for all λ\lambda. (Compare this with Theorem II.8.3.)

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Problem IX.3.7

Let UU be the bilateral shift on l2(Z)l^2(\mathbb {Z}). If e0e_0 is the vector in l2(Z)l^2(\mathbb {Z}) that has 11 in the zeroth place and zeros elsewhere, then e0e_0 is a star-cyclic vector for UU. If μ\mu is the compactly supported measure on C\mathbb {C} and V:l2(Z)→L2(μ)V: l^2(\mathbb {Z}) \to L^2(\mu ) is the isomorphism such that Ve0=1Ve_0 = 1 and VUV−1=NμVUV^{-1} = N_\mu, then

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(a)

μ=m=\mu = m = normalized arc length on ∂D\partial \mathbb {D};

(b)

V−1=V^{-1} = the Fourier transform on L2(m)=L2(∂D)L^2(m) = L^2(\partial \mathbb {D}).

Problem IX.3.8

Suppose N1,…,NdN_1, \dots , N_d are normal operators such that NjNk∗=Nk∗NjN_j N_k^* = N_k^* N_j for 1≤j,k≤d1 \leq j, k \leq d and suppose there is a vector e0e_0 in H\mathcal{H} such that H\mathcal{H} is the only subspace of H\mathcal{H} containing e0e_0 that reduces each of the operators N1,…,NdN_1, \dots , N_d. Show that there is a compactly supported measure μ\mu on Cd\mathbb {C}^d and an isomorphism V:H→L2(μ)V: \mathcal{H} \to L^2(\mu ) such that VNkV−1f=zkfVN_k V^{-1} f = z_k f for ff in L2(μ)L^2(\mu ) and 1≤k≤d1 \leq k \leq d (zk=z_k = the kkth coordinate function) (see Exercise 2.17).

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