In this paper, we conducted a study of H-Toeplitz operators on the Dirichlet type space Dt, which included several aspects. To begin, we established the matrix representation of the H-Toeplitz operator Sφ with respect to the orthonormal basis of Dt. Subsequently, we characterized the compactness of Sφ in terms of the symbol φ. Furthermore, we developed a new method to investigate the algebraic properties of H-Toeplitz operators, including self-adjointness, diagonality, co-isometry, partial isometry as well as commutativity.
Citation: Peiying Huang, Yiyuan Zhang. H-Toeplitz operators on the Dirichlet type space[J]. AIMS Mathematics, 2024, 9(7): 17847-17870. doi: 10.3934/math.2024868
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In this paper, we conducted a study of H-Toeplitz operators on the Dirichlet type space Dt, which included several aspects. To begin, we established the matrix representation of the H-Toeplitz operator Sφ with respect to the orthonormal basis of Dt. Subsequently, we characterized the compactness of Sφ in terms of the symbol φ. Furthermore, we developed a new method to investigate the algebraic properties of H-Toeplitz operators, including self-adjointness, diagonality, co-isometry, partial isometry as well as commutativity.
Let D be the unit disk in the complex plane C and dA=1πdxdy be the normalized Lebesgue measure on D. Set
dAt(z)=(t+1)(1−|z|2)tdA(z),t>−1. |
The Sobolev space L2,1t is the completion of the space of smooth functions f on D such that
‖f‖t={|∫DfdAt|2+∫D(|∂f∂z|2+|∂f∂¯z|2)dAt}1/2<∞. |
Clearly, L2,1t is a Hilbert space with the inner product
⟨f,g⟩t=∫DfdAt∫D¯gdAt+∫D(∂f∂z¯∂g∂z+∂f∂¯z¯∂g∂¯z)dAt. |
The Dirichlet type space Dt consists of all analytic functions f∈L2,1t with f(0)=0. The space Dt has been widely investigated; see [1,2,3,4], for example. Note that Dt is a closed subspace of L2,1t and hence, Dt is a Hilbert space. It is well-known that the Dirichlet type space Dt corresponds to several important spaces at specific values of t: the Hardy space (t=1), the Dirichlet space (t=0), and the weighted Bergman space (t>1).
Let N be the set of all positive integers. For z∈D and k∈N, let
ek(z)=√Γ(k+t+1)√kk!Γ(t+2)zk, |
then {ek}∞k=1 forms an orthonormal basis of Dt. Dt is a reproducing kernel space with reproducing kernel given by
Ktz(w)=∞∑k=1ek(w)¯ek(z)=∞∑k=1Γ(k+t+1)kk!Γ(t+2)wk¯zk, | (1.1) |
where Γ denotes the gamma function.
Let P be the orthogonal projection from L2,1t onto Dt, which by the property of reproducing kernel Ktw can be expressed as
P(f)(w)=⟨f,Ktw⟩t,w∈D | (1.2) |
for all f∈L2,1t.
Denote
M={φ |φ,∂φ∂z,∂φ∂¯z∈L∞(D)}, |
where the derivatives are taken in the sense of distribution.
For any φ∈M, the multiplication operator Mφ:L2,1t→L2,1t is defined as Mφ(f)=φf for f∈L2,1t. Given φ∈M, the Toeplitz operator Tφ:Dt→Dt and the Hankel operator Hφ:Dt→Dt with symbol φ are defined by
Tφ=PMφandHφ=PMφJ, |
respectively. Here, J:Dt→¯Dt denotes the flip operator given by J(ek)=¯ek for all k∈N, where ¯Dt:={¯f:f∈Dt}. It can be checked that Tφ and Hφ induced by φ∈M are bounded operators on Dt.
The harmonic Dirichlet space Dh is the closed subspace of L2,1t consisting of all harmonic functions f with f(0)=0. It is well-known that Dh=Dt⊕¯Dt. Consider the dilation operator K:Dt→Dh defined by
K(e2k)=ekandK(e2k−1)=¯ek |
for all k∈N. It can be observed that K is bounded on Dt with ‖K‖=1. Moreover, the adjoint K∗ of the operator K is given by
K∗(ek)=e2kandK∗(¯ek)=e2k−1 |
for all k∈N. Hence, K∗K=I on Dt and KK∗=I on Dh.
With these notations, we introduce the H-Toeplitz operator on the Dirichlet type space Dt, which is defined as follows.
Definition 1.1. For φ∈M, the H-Toeplitz operator Sφ:Dt→Dt with symbol φ is defined by
Sφ(f)=PMφK(f) |
for all f∈Dt.
The H-Toeplitz operator is closely related to both the Toeplitz and Hankel operators. In fact, for any φ∈M and k∈N, we have
Sφ(e2k)=PMφK(e2k)=PMφ(ek)=Tφ(ek) | (1.3) |
and
Sφ(e2k−1)=PMφK(e2k−1)=PMφ(¯ek)=PMφJ(ek)=Hφ(ek). | (1.4) |
Motivated by the notions of Toeplitz, Hankel and Slant Toeplitz operators, Arora and Paliwal [5] introduced the H-Toeplitz operators on the Hardy space, where they established the necessary and sufficient conditions under which H-Toeplitz operators become partial isometric, co-isometric, Hilbert-Schmidt and hyponormal. Moreover, they demonstrated that any H-Toeplitz operator is unitarily equivalent to a direct sum of a Toeplitz operator and a Hankel operator. The concept of H-Toeplitz operators is significant because it connects closely with a class of Hankel operators and a class of Toeplitz operators where the original operators are neither Hankel nor Toeplitz.
In recent years, H-Toeplitz operators on the Bergman space have been investigated by some specialists. Gupta and Singh [6] initiated the study of H-Toeplitz operators on the Bergman space, where the fundamental properties of the H-Toeplitz operators have been systematically studied, such as compactness, Fredholmness, co-isometry, partial isometry and commutativity. Later, Kim and Lee [7] established the contractivity and expansivity criteria for H-Toeplitz operators. Moreover, Liang et al. [8] studied the commutativity of H-Toeplitz operators with quasi-homogeneous symbols. In the recent paper [9], Ding and Chen characterized when the product of two H-Toeplitz operators with a bounded and a quasi-homogeneous symbol, respectively, becomes an H-Toeplitz operator. They also characterized when the product of an H-Toeplitz operator and a Toeplitz operator equals to another H-Toeplitz operator with bounded harmonic symbols.
It is well-known that Hardy, Bergman and Dirichlet spaces are the three most important classical Hilbert spaces of analytic functions in the unit disk. Despite the fruitful results achieved in the realm of H-Toeplitz operators on Hardy spaces and Bergman spaces, the theory of H-Toeplitz operators on Dirichlet spaces is largely unexplored. On the other hand, there is no any result in the literatures about H-Toeplitz operators on the weighted versions of these classical spaces. For the full generality and potential applicability, the main purpose of this article is to fill in these blanks by studying several fundamental properties of H-Toeplitz operators on the Dirichlet type space.
Before we mention the novelties of our work, it is worthwhile to recall from [10,11] that the study of Toeplitz operators and Hankel operators on the Dirichlet space are essentially different from that on the Hardy space and the Bergman space. Moreover, nontrivial self-adjoint Toeplitz operator with C1-symbol and non-scalar Toeplitz operator satisfying T∗φ=T¯φ do not exist on the Dirichlet space [12,13,14]. Since H-Toeplitz operators connect closely with Hankel operators and Toeplitz operators, it is natural to predict from the results mentioned in the literatures above that many techniques in the study of H-Toeplitz operators on the Hardy space and the Bergman space are not available on the Dirichlet space. For instance, one of the important steps to establish many properties (e.g., co-isometry and partial isometry) of an H-Toeplitz operator on the Hardy space and the Bergman space is using the adjoint of the H-Toeplitz operator, where the adjoint can be expressed as a composition of several specific operators. However, this cannot be done on the Dirichlet type space. To overcome this difficulty, our strategy is to establish an equivalent form of the Dirichlet Toeplitz operators under unitary conditions. This new form behaves much better than the original and avoids the need to compute the adjoint of the H-Toeplitz operator.
This paper is organized as follows. In Section 2, we obtain the matrix representation of the H-Toeplitz operator with the polynomial harmonic symbol under the orthonormal basis of the Dirichlet type space Dt. In Section 3, we mainly characterize the compactness of H-Toeplitz operators. In Section 4, several algebraic properties of H-Toeplitz operators are investigated, including self-adjointness, diagonality, co-isometry, partial isometry as well as commutativity.
In this section, we will present the matrix representation of the H-Toeplitz operator induced by the polynomial harmonic symbol under the orthonormal basis {ek}∞k=1 of the Dirichlet type space Dt. Leveraging the established relationships between the H-Toeplitz operator and both the Toeplitz and Hankel operators as outlined in Eqs (1.3) and (1.4), we will initially provide the matrix representations for the Toeplitz and Hankel operators.
We begin with the following lemma which will be needed in subsequent results.
Lemma 2.1. Suppose t>−1 and z∈D. For any n, m and k∈N, the following identities hold in the Dirichlet type space Dt:
(a) ⟨zn,zm⟩t={nn!Γ(t+2)Γ(n+t+1),ifn=m,0,otherwise.
(b) ⟨¯zn,zm⟩t=0 and ⟨zk¯zn,zm⟩t={m(n+m)!Γ(t+2)Γ(n+m+t+1),ifk=n+m,0,otherwise.
(c) P(¯znzm)={m!Γ(m−n+t+1)(m−n)!Γ(m+t+1)zm−n,ifm>n,0,ifm≤n.
Proof. By integration in polar coordinates, we have
⟨zn,zm⟩t=nm(1+t)∫Dzn−1¯zm−1(1−|z|2)tdAt(z)=n2(1+t)∫10rn−1(1−r)tdr={nn!Γ(t+2)Γ(n+t+1),if n=m,0,otherwise. |
This proves (a). Now, we show (b) in a similar fashion. The first equality is obvious. For the second one, we deduce that
⟨zk¯zn,zm⟩t=∫D∂(zk¯zn)∂z¯(∂zm∂z)dAt(z)=km(1+t)∫Dzk−1¯zn+m−1(1−|z|2)tdA(z)=m(1+t)(n+m)∫10rn+m−1(1−r)tdr={m(n+m)!Γ(t+2)Γ(n+m+t+1),if k=n+m,0,otherwise. |
Next, we show equality (c). By (1.2) and integration in polar coordinates, we get
P(¯znzm)=⟨¯znzm,Ktz⟩t=∫D∂(¯wnwm)∂w¯(∂Ktz(w)∂w)dAt(w)=m(1+t)∫D¯wnwm−1(∞∑k=1Γ(k+t+1)Γ(t+2)k!zk¯wk−1)(1−|w|2)tdA(w)=m(1+t)∫Dwm−1(∞∑k=1Γ(k+t+1)Γ(t+2)k!zk¯wn+k−1)(1−|w|2)tdA(w)=m(1+t)Γ(m−n+t+1)Γ(t+2)(m−n)!zm−n∫D|w|2(m−1)(1−|w|2)tdA(w)=m(1+t)Γ(m−n+t+1)Γ(t+2)(m−n)!zm−n∫10rm−1(1−r)tdr={m!Γ(m−n+t+1)(m−n)!Γ(m+t+1)zm−n,if m>n,0,if m≤n. |
This ends the proof of Lemma 2.1.
According to Lemma 2.1, we can find the matrix representations of Toeplitz operator Tφ and of Hankel operator Hφ on Dt with symbol
φ(z)=∞∑i=0aizi+∞∑j=1bj¯zj∈M,z∈D,ai,bj∈C. |
For any m, n∈N, the (m,n)-th entry of the matrix representation of Tφ with respect to the orthonormal basis {ek}∞k=1 of Dt is given by
⟨Tφ(en),em⟩t=⟨PMφ(en),em⟩t=⟨φen,em⟩t=√Γ(n+t+1)Γ(m+t+1)√nmn!m!Γ(t+2)⟨φzn,zm⟩t=√Γ(n+t+1)Γ(m+t+1)√nmn!m!Γ(t+2)(∞∑i=0ai⟨zi+n,zm⟩t+∞∑j=1bj⟨¯zjzn,zm⟩t)={√mm!Γ(n+t+1)√nn!Γ(m+t+1)am−n,if m≥n,√mn!Γ(m+t+1)√nm!Γ(n+t+1)bn−m,if m<n. | (2.1) |
Therefore, the matrix representation of Tφ is explicitly given by
Tφ=[a01√2+tb1√2√(3+t)(2+t)b2√6Γ(2+t)√Γ(5+t)b3⋯2√2+ta1a0√2√3+tb1√6√(4+t)(3+t)b2⋯3√2√(3+t)(2+t)a23√2(3+t)a1a0√3√4+tb1⋯4√6Γ(2+t)√Γ(5+t)a32√6√(4+t)(3+t)a24√3(4+t)a1a0⋯⋮⋮⋮⋮], | (2.2) |
and the matrix representation of its adjoint T∗φ is given by
T∗φ=[¯a02√2+t¯a13√2√(3+t)(2+t)¯a24√6Γ(2+t)√Γ(5+t)¯a3⋯1√2+t¯b1¯a03√2(3+t)¯a12√6√(4+t)(3+t)¯a2⋯√2√(3+t)(2+t)¯b2√2√3+t¯b1¯a04√2(3+t)¯a1⋯√6Γ(2+t)√Γ(5+t)¯b3√6√(4+t)(3+t)¯b2√3√4+t¯b1¯a0⋯⋮⋮⋮⋮]. |
Next, we find the matrix representation of the Hankel operator. The (m,n)-th entry of the matrix representation of Hφ with respect to the orthonormal basis {ek}∞k=1 of Dt is given by
⟨Hφ(en),em⟩t=⟨PMφJ(en),em⟩t=⟨PMφ(¯en),em⟩t=⟨φ¯en,em⟩t=√Γ(n+t+1)Γ(m+t+1)√nmn!m!Γ(t+2)⟨φ¯zn,zm⟩t=√Γ(n+t+1)Γ(m+t+1)√nmn!m!Γ(t+2)(∞∑i=0ai⟨zi¯zn,zm⟩t+∞∑j=1bj⟨¯zj+n,zm⟩t)=(n+m)!√mΓ(n+t+1)Γ(m+t+1)√nn!m!Γ(m+n+t+1)am+n | (2.3) |
for m, n∈N.
Thus, the matrix representation of Hφ in explicit form is given by
Hφ=[22+ta23(3+t)√2+ta34!√Γ(4+t)Γ(2+t)3√2Γ(5+t)a45!√Γ(5+t)Γ(2+t)2√4!Γ(6+t)a5⋯6(3+t)√2+ta312(4+t)(3+t)a45!√Γ(4+t)Γ(3+t)3√2Γ(6+t)a56!√Γ(5+t)Γ(3+t)2√4!Γ(7+t)a6⋯4!√Γ(2+t)(4+t)√2Γ(4+t)a45!√Γ(3+t)Γ(4+t)2√2Γ(6+t)a56!Γ(4+t)3!Γ(7+t)a67!√Γ(5+t)Γ(4+t)8√3Γ(8+t)a7⋯5!√Γ(2+t)(5+t)√6Γ(5+t)a56!√Γ(3+t)Γ(5+t)2√6Γ(7+t)a67!√Γ(4+t)Γ(5+t)6√3Γ(8+t)a78!Γ(5+t)4!Γ(9+t)a8⋯⋮⋮⋮⋮]. | (2.4) |
Note that the matrix of Hankel operator Hφ is independent of co-analytic term ∑∞j=1bj¯zj of the symbol function φ. By a direct calculation, the matrix representation of its adjoint H∗φ is of the following form:
H∗φ=[22+t¯a26(3+t)√2+t¯a34!√Γ(2+t)(4+t)√2Γ(4+t)¯a45!√Γ(2+t)(5+t)√6Γ(5+t)¯a5⋯3(3+t)√2+t¯a312(4+t)(3+t)¯a45!√Γ(3+t)Γ(4+t)3√2Γ(6+t)¯a56!√Γ(3+t)Γ(5+t)2√6Γ(7+t)¯a6⋯4!√Γ(4+t)Γ(2+t)3√2Γ(5+t)¯a45!√Γ(4+t)Γ(3+t)3Γ(6+t)¯a56!Γ(4+t)3!Γ(7+t)¯a67!√Γ(4+t)Γ(5+t)6√3Γ(8+t)¯a7⋯5!√Γ(5+t)Γ(2+t)2√4!Γ(6+t)¯a56!√Γ(5+t)Γ(3+t)2√4!Γ(7+t)¯a67!√Γ(5+t)Γ(4+t)8√3Γ(8+t)¯a78!Γ(5+t)4!Γ(9+t)¯a8⋯⋮⋮⋮⋮]. |
Observe that H∗φ=H⊤ˆφ for ˆφ(z)=∑∞i=1¯aizi+∑∞j=1¯bj¯zj (each bj can be zero), where H⊤ˆφ denotes the transpose of the matrix representation of Hˆφ.
Next we find the matrix representation of H-Toeplitz operator Sφ. Clearly, it follows from (1.3), (1.4), (2.1) and (2.3) that
⟨Sφ(e2n),em⟩t=⟨Tφ(en),em⟩t={√mm!Γ(n+t+1)√nn!Γ(m+t+1)am−n,if m≥n,√mn!Γ(m+t+1)√nm!Γ(n+t+1)bn−m,if m<n, | (2.5) |
and
⟨Sφ(e2n−1),em⟩t=⟨Hφ(en),em⟩t=(n+m)!√mΓ(n+t+1)Γ(m+t+1)√nn!m!Γ(m+n+t+1)am+n, | (2.6) |
where m, n∈N. Thus, the matrix representation of Sφ with respect to the orthonormal basis {ek}∞k=1 of Dt is given by
Sφ=[22+ta2a03(3+t)√2+ta31√2+tb1⋯6(3+t)√2+ta32√2+ta112(4+t)(3+t)a4a0⋯4!√Γ(2+t)(4+t)√2Γ(4+t)a43√2√(3+t)(2+t)a25!√Γ(3+t)Γ(4+t)2√2Γ(6+t)a53√2(3+t)a1⋯5!√Γ(2+t)(5+t)√6Γ(5+t)a54√6Γ(2+t)√Γ(5+t)a36!√Γ(3+t)Γ(5+t)2√6Γ(7+t)a62√6√(4+t)(3+t)a2⋯⋮⋮⋮⋮], | (2.7) |
and the matrix representation of its adjoint is given by
S∗φ=[22+t¯a26(3+t)√2+t¯a34!√Γ(2+t)(4+t)√2Γ(4+t)¯a45!√Γ(2+t)(5+t)√6Γ(5+t)¯a5⋯¯a02√2+t¯a13√2√(3+t)(2+t)¯a24√6Γ(2+t)√Γ(5+t)¯a3⋯3(3+t)√2+t¯a312(4+t)(3+t)¯a45!√Γ(3+t)Γ(4+t)2√2Γ(6+t)¯a56!√Γ(3+t)Γ(5+t)2√6Γ(7+t)¯a6⋯1√2+t¯b1¯a03√2(3+t)¯a12√6√(4+t)(3+t)¯a2⋯⋮⋮⋮⋮]. |
Remark 2.1. It can be seen from (2.2), (2.4) and (2.7) that the matrix representations of the Toeplitz operator Tφ and the Hankel operator Hφ can be obtained by deleting every odd and even column of the H-Toeplitz operator Sφ, respectively. The matrix of Sφ is an upper triangular matrix if the symbol φ∈M is co-analytic. However, it cannot be lower triangular. Additionally, it is worthwhile to mention that an n×n Dirichlet type H-Toeplitz matrix defined as follows has 2n degree of freedom rather than n2. Consequently, for large n, it is relatively easy to solve the system of linear equations when the coefficient matrix is a Dirichlet type H-Toeplitz matrix.
Definition 2.1. Let φ(z)=∑∞i=0aizi+∑∞j=1bj¯zj∈M with z∈D and ai,bj∈C. We define an infinite matrix (cm,n) as a Dirichlet type H-Toeplitz matrix if its (m,n)-th entry satisfies the following relation:
cm,n={√mm!Γ(l+t+1)√ll!Γ(m+t+1)am−l,ifn=2landm≥l,√ml!Γ(m+t+1)√lm!Γ(l+t+1)bl−m,ifn=2landm<l,(l+m)!√mΓ(l+t+1)Γ(m+t+1)√ll!m!Γ(m+l+t+1)am+l,ifn=2l−1, |
where m, n and l are all in N.
This section is mainly concerned with the compactness of H-Toeplitz operators. It is well-known that compact operators behave like operators on finite-dimensional vector spaces and play a fundamental role in operator theory.
The following proposition follows easily from the definition of the H-Toeplitz operator Sφ.
Proposition 3.1. Suppose that a,b∈C and φ,ψ∈M. Then
(a) Saφ+bψ=aSφ+bSψ;
(b) Sφ is a bounded linear operator on Dt with ‖Sφ‖t≤‖∂φ∂z‖∞+‖φ‖∞.
Let L2a(dAt) be the weighted Bergman space on D, which consists of all analytic functions in L2(D,dAt). We use the notations ‖⋅‖2 and ⟨⋅,⋅⟩2 to represent the norm and inner product in L2a(dAt), respectively.
Similar to the proof of [15, Lemma 12], we have the following result.
Lemma 3.1. The identity operator I from Dt into L2a(dAt) defined by If=f for any f∈Dt is compact.
From Lemma 3.1, we conclude that for any sequence {fk}k converging weakly to 0 in Dt (write fkw→0 for short), the sequence {‖fk‖2}k converges to 0 as k→∞.
The next lemma will be utilized in the compactness of H-Toeplitz operators.
Lemma 3.2. For any φ∈M, S∗φ−K∗PhM¯φ is compact on Dt, where Ph is the orthogonal projection from L2,1t onto Dh.
Proof. For any f,g∈Dt, we have
⟨(S∗φ−K∗PhM¯φ)(f),g⟩t=⟨f,Sφ(g)⟩t−⟨K∗PhM¯φ(f),g⟩t=⟨f,PMφK(g)⟩t−⟨PhM¯φ(f),K(g)⟩t=⟨f,φK(g)⟩t−⟨¯φf,K(g)⟩t=⟨∂f∂z,K(g)∂φ∂z⟩2+⟨∂f∂z,φ∂(K(g))∂z⟩2−⟨f∂¯φ∂z,∂(K(g))∂z⟩2−⟨¯φ∂f∂z,∂(K(g))∂z⟩2=⟨∂f∂z,∂φ∂zK(g)⟩2−⟨f,∂φ∂¯z∂(K(g))∂z⟩2. |
Since Dt is contained in L2a(dAt), it follows that
|⟨(S∗φ−K∗PhM¯φ)(f),g⟩t|≤|⟨∂f∂z,∂φ∂zK(g)⟩2|+|⟨f,∂φ∂¯z∂(K(g))∂z⟩2|≤‖∂f∂z‖2‖∂φ∂zK(g)‖2+‖f‖2‖∂φ∂¯z∂(K(g))∂z‖2≤‖φ‖M(‖f‖t‖K(g)‖2+‖f‖2‖K(g)‖t)≤‖φ‖M(‖f‖t‖g‖2+‖f‖2‖g‖t), |
where
‖φ‖M=esssupz∈Dmax{|φ|,|∂φ∂z|,|∂φ∂¯z|}. |
Let {fk}k be any sequence converging weakly to 0 in Dt. Taking f=fk and g=(S∗φ−K∗PhM¯φ)fk in the above, we obtain
‖(S∗φ−K∗PhM¯φ)fk‖2t≤‖φ‖M[‖fk‖t‖(S∗φ−K∗PhM¯φ)fk‖2+‖fk‖2‖(S∗φ−K∗PhM¯φ)fk‖t]. |
Note that (S∗φ−K∗PhM¯φ)fkw→0 in Dt as k→∞. It follows from Lemma 3.1 that ‖fk‖2 and ‖(S∗φ−K∗PhM¯φ)fk‖2→0 as k→∞. Therefore,
‖(S∗φ−K∗PhM¯φ)fk‖t→0 |
as k→∞, which implies that S∗φ−K∗PhM¯φ is compact on Dt. This completes the proof of the lemma.
Remark 3.1. Let ˇPh denote the orthogonal projection from L2(D,dA) onto the harmonic Bergman space L2h. We have known that the adjoint S∗φ of an H-Toeplitz operator Sφ is equal to K∗M¯φ (resp., K∗ˇPhM¯φ) on the Hardy space [5] (resp., Bergman space [6]). However, there is no analogues identity on the Dirichlet type space. The situation is different from that of Hardy space and Bergman space.
Lemma 3.3. [16, Proposition 7.2] If φ∈L1(D,dAt) is harmonic, then ˇTφ is compact on L2a(dAt) if and only if φ=0.
We apply the above results to show the compactness of the H-Toeplitz operator on Dt.
Theorem 3.1. Suppose t>−1 and φ∈M is co-analytic. Then, Sφ is a compact operator on Dt if and only if φ=0.
Proof. If φ=0, then Sφ is trivially compact on Dt.
Conversely, assume that Sφ is compact on Dt. We are going to show that φ=0. Otherwise, if φ≠0, then ˇTφ is not compact on L2a(dAt) by Lemma 3.3. Hence, there is a sequence {fk}k⊆L2a(dAt), ‖fk‖2=1, fkw→0 such that ‖ˇTφ(fk)‖2↛0 as k→∞. Thus, ‖φfk‖2↛0, that is,
∫D|φ|2|fk|2dAt↛0 |
as k→∞.
Note that Sφ is compact on Dt, so is S∗φ by [16, Theorem 1.16]. We deduce that K∗PhM¯φ is also compact on Dt by Lemma 3.2. This implies that SφK∗PhM¯φ is compact on Dt. Let
Fk:=∫z0fk(w)dw, |
then Fkw→0 in Dt and ‖Fk‖t=1. So, ‖SφK∗PhM¯φ(Fk)‖t→0, that is,
‖|φ|2Fk‖t→0 |
as k→∞. Thus, we have
|⟨|φ|2Fk,Fk⟩t|≤‖|φ|2Fk‖t‖Fk‖t=‖|φ|2Fk‖t→0 |
as k→∞. However,
⟨|φ|2Fk,Fk⟩t=⟨∂(|φ|2Fk)∂z,∂Fk∂z⟩2=⟨Fk∂|φ|2∂z,∂Fk∂z⟩2+⟨|φ|2∂Fk∂z,∂Fk∂z⟩2=⟨φFk∂¯φ∂z,fk⟩2+⟨|φ|2fk,fk⟩2↛0, |
since
|⟨φFk∂¯φ∂z,fk⟩2|≤‖φ‖2M‖Fk‖2‖fk‖t→0 |
and
⟨|φ|2fk,fk⟩2=∫D|φ|2|fk|2dAt↛0 |
as k→∞. This contradiction shows that φ=0. This ends the proof of Theorem 3.1.
Lemma 3.4. Suppose t>−1 and z, w∈D. The dilation operator K:Dt→Dh satisfies
K(Ktz)(w)=∞∑k=1√Γ(2k+t+1)Γ(k+t+1)kΓ(t+2)√2(2k)!k!¯z2kwk+∞∑k=1√Γ(2k+t)Γ(k+t+1)Γ(t+2)√kk!(2k−1)(2k−1)!¯z2k−1¯wk. |
Proof. For z,w∈D, by (1.1) and the definition of K, we obtain
K(Ktz)(w)=∞∑k=1¯e2k(z)K(e2k)(w)+∞∑k=1¯e2k−1(z)K(e2k−1)(w)=∞∑k=1¯e2k(z)ek(w)+∞∑k=1¯e2k−1(z)¯ek(w)=∞∑k=1√Γ(2k+t+1)Γ(k+t+1)kΓ(t+2)√2k!(2k)!¯z2kwk+∞∑k=1√Γ(2k+t)Γ(k+t+1)Γ(t+2)√kk!(2k−1)(2k−1)!¯z2k−1¯wk. |
This finishes the proof of the lemma.
For t>−1 and z, w∈D, denote
htz(w):=K(ktz)(w), |
where
ktz(w)=Ktz(w)‖Ktz‖t |
is the normalized reproducing kernel of Dt. Let ∂D be the boundary of the unit disk D. Next, we will discuss the boundary behavior of htz.
Lemma 3.5. For t≥0 and z∈D, we have htz→0 as z→∂D.
Proof. For t>0, by the Stirling's formula, we have
‖Ktz‖2t=⟨Ktz,Ktz⟩t=Ktz(z)=∞∑k=1Γ(k+t+1)kk!Γ(t+2)|z|2k∼∞∑k=1Γ(k+t)k!Γ(t)|z|2k=1(1−|z|2)t, | (3.1) |
where the notation "∼" is used to denote that the ratio of the two sides tends to 1 as k→∞.
For t=0, we have
‖Ktz‖2t=⟨Ktz,Ktz⟩t=Ktz(z)=∞∑k=1|z|2kk=log11−|z|2. |
We conclude that
htz=K(ktz)=K(Ktz)‖Ktz‖t→0 |
as z→∂D.
Proposition 3.2. Suppose t≥0 and φ∈M. Then, Sφ is not bounded below on Dt.
Proof. Given z∈D, by the dominated convergence theorem, Lemma 3.5, and (3.1), we have
‖Sφ(ktz)‖2t=‖PMφ(htz)‖2t≤‖φhtz‖2t=|∫DφhtzdAt|2+∫D(|∂(φhtz)∂w|2+|∂(φhtz)∂¯w|2)dAt=|∫DφhtzdAt|2+∫D|htz(w)∂φ(w)∂w+φ(w)‖Ktz‖t∞∑k=1√Γ(2k+t+1)Γ(k+t+1)Γ(t+2)√2k!(2k)!¯z2kwk−1|2dAt(w)+∫D|htz(w)∂φ(w)∂¯w+φ(w)‖Ktz‖t∞∑k=1√kΓ(2k+t)Γ(k+t+1)Γ(t+2)√k!(2k−1)(2k−1)!¯z2k−1¯wk−1|2dAt(w)→0 |
as z→∂D, from which we deduce that Sφ is not bounded below on Dt.
Recall that for a bounded linear operator T defined on a Hilbert space, the approximated point spectrum of operator T is defined as the set
σap(T)={λ∈C:T−λIis not bounded below}. |
See [17]. Thus, for the H-Toeplitz operator Sφ defined on Dt, Proposition 2 implies that 0∈σap(Sφ) for t≥0 and φ∈M.
At the end of this section, we explore the question of when an H-Toeplitz operator is Fredholm. For more details concerning Fredholm operators; see [18, CHAPTER XI § 2].
The subsequent proposition illustrates the property of the Fredholm operator on Dt from the perspective of weakly convergent nets.
Proposition 3.3. Suppose t>−1. If T is a Fredholm operator on Dt, then, there is no {hz}z∈D of unit vectors in Dt such that hzw→0 as z→∂D and lim‖Thz‖t=0.
Proof. Suppose there is {hz}z∈D of unit vectors in Dt such that hzw→0 as z→∂D and lim‖Thz‖t=0. We shall provide a proof by contradiction. Since T is Fredholm, there exists a bounded operator B and a compact operator E on Dt such that BT=I+E. Then,
|I−‖BThz‖t|=|‖hz‖t−‖BThz‖t|≤‖Ehz‖t→0 |
as z→∂D by the compactness of E. This implies that ‖BThz‖t→1 as z→∂D, which contradicts to the assumption lim‖Thz‖t=0.
Theorem 3.2. Suppose t≥0 and φ∈M. Then, there is no nonzero H-Toeplitz operator Sφ on Dt which is Fredholm.
Proof. Assume that the H-Toeplitz operator Sφ is Fredholm on Dt for some φ∈M. Take the net {ktz}z∈D of normalized kernels on Dt. Then, ktz→0 weakly and also ‖Sφktz‖t→0 as z→∂D by the proof of Proposition 3.2. This contradicts the fact that Sφ is a Fredholm operator by Proposition 3.3. It follows that Sφ is a Fredholm operator on Dt if and only if φ=0 in M.
Recall that the essential spectrum of a bounded linear operator T is given by
σe(T)={λ∈C:T−λI is not Fredholm}. |
For t≥0 and φ∈M, we derive that the essential spectrum of H-Toeplitz operator Sφ on Dt is nonempty by the above theorem, since 0∈σe(Sφ) in this case.
In this section, we investigate some algebraic properties of H-Toeplitz operators on Dt, which include self-adjointness, diagonality, co-isometry, partial isometry as well as commutativity.
Let
H={φ∈M:φ(z)=∞∑i=0aizi+∞∑j=1bj¯zj, z∈D and ai,bj∈C}. |
In the next theorem, we develop a new method to demonstrate that a nonzero H-Toeplitz operator Sφ induced by φ∈H can never be a self-adjoint operator on Dt.
Theorem 4.1. Let t>−1 and φ∈H. Then the H-Toeplitz operator Sφ is self-adjoint on Dt if and only if φ=0.
Proof. Let φ∈H defined by φ(z)=∑∞i=0aizi+∑∞j=1bj¯zj, where z∈D and ai,bj∈C. The backward implication is trivial. Now, suppose that Sφ is self-adjoint. Then (S∗φ−Sφ)f=0 for any f∈Dt. Taking f(z)=e1(z)=z, we apply the reproducing property of Ktz, Lemma 3.4, and (1.4) to get
S∗φ(e1)(z)=⟨S∗φ(e1),Ktz⟩t=⟨e1,Sφ(Ktz)⟩t=⟨e1,PMφK(Ktz)⟩t=⟨e1,φ⋅K(Ktz)⟩t=∫D¯∂(φ⋅K(Ktz))∂w(w)dAt(w)=∫D¯K(Ktz)(w)¯∂φ∂w(w)dAt(w)+∫D¯φ(w)¯∂(K(Ktz))∂w(w)dAt(w)=∫D(∞∑i=1i¯ai¯wi−1)(∞∑k=1√Γ(2k+t+1)Γ(k+t+1)kΓ(t+2)√2(2k)!k!z2k¯wk+∞∑k=1√Γ(2k+t)Γ(k+t+1)Γ(t+2)√kk!(2k−1)(2k−1)!z2k−1wk)dAt(w)+∫D(∞∑i=0¯ai¯wi+∞∑j=1¯bjwj)(∞∑k=1√Γ(2k+t+1)Γ(k+t+1)Γ(t+2)√2(2k)!k!z2k¯wk−1)dAt(w)=∞∑k=1(k+1)√(k−1)!Γ(2k+t)Γ(k+t+1)¯ak+1Γ(k+t+2)√(2k−1)(2k−1)!z2k−1+√t+2¯a02z2+∞∑k=1√k!Γ(2k+t+3)¯bk√2(k+1)(2k+2)!Γ(k+t+2)z2k+2, |
and
Sφ(e1)(z)=Hφ(e1)(z)=PMφJ(e1)(z)=P(φ¯e1)(z)=⟨φ¯e1,Ktz⟩t=∫D∂(φ¯e1)∂w(w)¯∂Ktz∂w(w)dAt(w)=∫D(∞∑i=1iaiwi−1¯w)(∞∑k=1Γ(k+t+1)k!Γ(t+2)zk¯wk−1)dAt(w)=∞∑k=1(k+1)ak+1k+t+1zk. |
Therefore,
0= (S∗φ−Sφ)(e1)(z)= (√t+2¯a02−3a3t+3)z2+∞∑k=1((k+1)√(k−1)!Γ(2k+t)Γ(k+t+1)¯ak+1Γ(k+t+2)√(2k−1)(2k−1)!−2ka2k2k+t)z2k−1+∞∑k=1(√k!Γ(2k+t+3)¯bk√2(k+1)(2k+2)!Γ(k+t+2)−(2k+3)a2k+32k+t+3)z2k+2. |
This implies that
¯a0=6a3√t+2(t+3), | (4.1) |
¯ak+1=2kΓ(k+t+2)√(2k−1)(2k−1)!(k+1)(2k+t)√(k−1)!Γ(2k+t)Γ(k+t+1)a2k,k∈N, | (4.2) |
and
¯bk=√2(k+1)(2k+3)!Γ(k+t+2)(2k+t+3)√k!Γ(2k+t+3)a2k+3,k∈N. | (4.3) |
Taking f(z)=e2(z)=√t+22z2 and by the reproducing property of Ktz, Lemma 3.4, and (1.3), we deduce that
S∗φ(e2)(z)=⟨S∗φ(e2),Ktz⟩t=⟨e2,Sφ(Ktz)⟩t=⟨e2,PMφK(Ktz)⟩t=⟨e2,φ⋅K(Ktz)⟩t=∫D∂e2∂w(w)¯∂(φ⋅K(Ktz))∂w(w)dAt(w)=√t+2∫Dw¯∂φ∂w(w)¯K(Ktz)(w)dAt(w)+√t+2∫Dw¯φ(w)¯∂(K(Ktz))∂w(w)dAt(w)=√t+2∫Dw(∞∑i=1i¯ai¯wi−1)(∞∑k=1√Γ(2k+t+1)Γ(k+t+1)kΓ(t+2)√2(2k)!k!z2k¯wk+∞∑k=1√Γ(2k+t)Γ(k+t+1)Γ(t+2)√kk!(2k−1)(2k−1)!z2k−1wk)dAt(w)+√t+2∫Dw(∞∑i=0¯ai¯wi+∞∑j=1¯bjwj)×(∞∑k=1√Γ(2k+t+1)Γ(k+t+1)Γ(t+2)√2(2k)!k!z2k¯wk−1)dAt(w)=¯a1z2+∞∑k=1(k+1)(k+2)√k!Γ(2k+t)Γ(k+t+1)¯ak+2Γ(k+t+3)√k(2k−1)(2k−1)!z2k−1+√Γ(t+5)¯a04√6Γ(t+2)z4+∞∑k=1√(t+2)Γ(2k+t+5)¯bk(k+2)√2(2k+4)!z2(k+2), |
and
Sφ(e2)(z)=Tφ(e1)(z)=PMφ(e1)(z)=⟨φe1,Ktz⟩t=∫D∂(φe1)∂w(w)¯∂Ktz∂w(w)dAt(w)=∫D(∞∑i=1iai−1wi−1+∞∑j=1bj¯wj)(∞∑k=1Γ(k+t+1)k!Γ(t+2)zk¯wk−1)dAt(w)=∞∑k=1ak−1zk. |
Thus, we obtain
0= (S∗φ−Sφ)(e2)(z)= (¯a1−a1)z2+(√Γ(t+5)¯a04√6Γ(t+2)−a3)z4+∞∑k=1((k+1)(k+2)√k!Γ(2k+t)Γ(k+t+1)¯ak+2Γ(k+t+3)√k(2k−1)(2k−1)!−a2k−2)z2k−1+∞∑k=1(√(t+2)Γ(2k+t+5)¯bk(k+2)√2(2k+4)!−a2k+3)z2(k+2). |
This implies that
¯a1=a1, | (4.4) |
¯a0=4√6Γ(t+2)√Γ(t+5)a3, | (4.5) |
¯ak+2=Γ(k+t+3)√k(2k−1)(2k−1)!(k+1)(k+2)√k!Γ(2k+t)Γ(k+t+1)a2k−2,k∈N, | (4.6) |
and
¯bk=(k+2)√2(2k+4)!√(t+2)Γ(2k+t+5)a2k+3,k∈N. | (4.7) |
By (4.1) and (4.5), we get ¯a0=a3=0. This together with (4.2), (4.3), (4.6) and (4.7) further implies that
ai=0,bj=0,for any i∈{0}∪N−{1} and j∈N. | (4.8) |
It remains to show a1=0. Taking
f(z)=e3(z)=√(t+2)(t+3)3√2z3, |
a similar argument shows that
S∗φ(e3)(z)=⟨S∗φ(e3),Ktz⟩t=⟨e3,Sφ(Kz)⟩t=⟨e3,PMφK(Ktz)⟩t=⟨e3,φ⋅K(Ktz)⟩t=∫D∂e3∂w(w)¯∂(φ⋅K(Ktz))∂w(w)dAt(w)=√(t+2)(t+3)√2∫Dw2¯∂φ∂w(w)¯K(Ktz)(w)dAt(w)+√(t+2)(t+3)√2∫Dw2¯φ(w)¯∂(K(Ktz))∂w(w)dA(w)=√(t+2)(t+3)√2∫Dw2(∞∑i=1i¯ai¯wi−1)(∞∑k=1√Γ(2k+t+1)Γ(k+t+1)kΓ(t+2)√2(2k)!k!z2k¯wk+∞∑k=1√Γ(2k+t)Γ(k+t+1)Γ(t+2)√kk!(2k−1)(2k−1)!z2k−1wk)dAt(w)+√(t+2)(t+3)√2∫Dw2(∞∑i=0¯ai¯wi+∞∑j=1¯bjwj)×(∞∑k=1√Γ(2k+t+1)Γ(k+t+1)Γ(t+2)√2(2k)!k!z2k¯wk−1)dAt(w)=√3(t+2)(t+4)¯a18z4+⋯, |
and
Sφ(e3)(z)=Hφ(e2)(z)=PMφJ(e2)(z)=P(φ¯e2)(z)=⟨φ¯e2,Ktz⟩t=∫D∂(φ¯e2)∂w(w)¯∂Ktz∂w(w)dAt(w)=∫D(∞∑i=1√t+2iai2wi−1¯w2)(∞∑k=1Γ(k+t+1)k!Γ(t+2)zk¯wk−1)dAt(w)=∞∑k=1(k+1)(k+2)√t+2ak+22(k+t+2)(k+t+1)zk. |
Hence, we obtain
\begin{align*} 0 = \ (S_{\varphi}^{\ast}-S_{\varphi})(e_{3})(z) = \left( \frac{\sqrt{3 \, (t+2) \, (t+4)}\,\overline{a_{1}}}{8}-\frac{15\sqrt{t+2} \, a_{6}}{(t+6) \, (t+5)} \right) z^{4}+\cdots, \end{align*} |
which implies
a_{1} = \frac{40\sqrt{3}}{(t+6) \, (t+5) \, \sqrt{t+4}}\overline{a_{6}} = 0. |
This together with (4.8) shows that \varphi = 0 , completing the proof of the theorem.
Recall that an operator T is diagonal on the Dirichlet type space \mathfrak{D}_{t} if and only if \langle Te_{i}, e_{j} \rangle_{t} = 0 for all positive integers i\ne j .
Theorem 4.2. Let t > -1 and \varphi\in \mathfrak{H} . Then, S_\varphi is a diagonal operator on \mathfrak{D}_{t} if and only if \varphi = 0 .
Proof. Let \varphi\in \mathfrak{H} defined by \varphi(z) = \sum_{i = 0}^{\infty}a_{i}z^{i}+\sum_{j = 1}^{\infty}b_{j}\overline{z}^{j} , where z\in\mathbb{D} and a_{i}, b_{j}\in\mathbb{C} . The forward implication is trivial. Suppose conversely that S_\varphi is a diagonal operator on \mathfrak{D}_{t} . Then, for m , n\in\mathbb{N} such that m\ne n , we have \langle S_{\varphi}(e_n), e_m \rangle_{t} = 0 , where \{e_{n}\}_{n = 1}^{\infty} is an orthonormal basis of \mathfrak{D}_{t} . Then, the following two cases arise. If n = 2k for some k\in\mathbb{N} , by (2.5), we get
\begin{align*} \langle S_{\varphi}(e_{2k}),e_{m} \rangle_{t} = \langle T_{\varphi} (e_k),e_m \rangle_{t} = \begin{cases} \dfrac{\sqrt{m\,m!\,\Gamma(k+t+1)}}{\sqrt{k\,k!\,\Gamma(m+t+1)}}a_{m-k}, &\text{if } m\ge k, \\ \dfrac{\sqrt{m\,k!\,\Gamma(m+t+1)}}{\sqrt{k\,m!\,\Gamma(k+t+1)}}b_{k-m}, &\text{if } k > m. \end{cases} \end{align*} |
If n = 2k-1 for some k\in\mathbb{N} , by (2.6), we obtain
\begin{align*} \langle S_{\varphi}(e_{2k-1}),e_{m} \rangle_{t} = \langle H_{\varphi}(e_k),e_m \rangle_{t} = \frac{(k+m)!\sqrt{m\,\Gamma(k+t+1)\,\Gamma(m+t+1)}}{\sqrt{k\,k!\,m!}\,\Gamma(m+k+t+1)} a_{m+k}. \end{align*} |
The above cases indicate that a_i = 0 and b_j = 0 for all i\ge 0 , j\ge 1 . Hence, \varphi = 0 .
Let \check{P} be the Bergman projection from L^{2}(\mathbb{D}, dA_{t}) onto the weighted Bergman space L_{a}^{2}\left(dA_{t} \right) . For any \varphi\in L^{\infty}(\mathbb{D}) , the Toeplitz operator \check{T}_{\varphi} on L_{a}^{2}\left(dA_{t} \right) is defined by
\check{T}_{\varphi} = \check{P}M_\varphi. |
Note that the adjoint of \check{T}_{\varphi} satisfies \check{T}_{\varphi}^{\ast} = \check{T}_{\overline{\varphi}} .
Let
\check{e}_k(z) = \frac{\sqrt{\Gamma(k+t+2)}}{\sqrt{k!\,\Gamma(t+2)}}z^{k},\quad z\in\mathbb{D}. |
Then, \left\{ \check{e}_k \right\} _{k = 0}^{\infty} forms an orthonormal basis of L_{a}^{2}\left(dA_{t} \right) . Define an operator U:\mathfrak{D}_{t}\to L_{a}^{2}\left(dA_{t} \right) by
U(e_k) = \check{e}_{k-1} |
and linearly extending it to \mathfrak{D}_{t} . Then, U is a unitary operator such that
Uf = f^{'} |
for each f\in\mathfrak{D}_{t} .
In the next result, we see that a Toeplitz operator induced by a co-analytic symbol in \mathcal{M} on the Dirichlet type space \mathfrak{D}_{t} is unitarily equivalent to that on the weighted Bergman space L_{a}^{2}\left(dA_{t} \right) .
Lemma 4.1. Let \varphi\in\mathcal{M} be a co-analytic function. Then, T_{\varphi} = U^{\ast}\check{T}_{\varphi}U .
Proof. Recall that \langle \cdot, \cdot \rangle _2 denotes the inner product in L_{a}^{2}\left(dA_{t} \right) . Let \varphi\in\mathcal{M} be a co-analytic function. For any f, g \in \mathfrak{D}_{t} , a direct calculation gives
\begin{align*} \langle T_{\varphi}f, g \rangle _t & = \langle P M_\varphi f, g \rangle _t = \langle \varphi f, g \rangle _t \\ & = \langle \frac{\partial (\varphi f)}{\partial z}, \frac{\partial g}{\partial z} \rangle _2 \\ & = \langle f \frac{\partial \varphi}{\partial z} , \frac{\partial g}{\partial z} \rangle _2 + \langle \varphi \frac{\partial f}{\partial z}, \frac{\partial g}{\partial z} \rangle _2\\ & = \langle \check{T}_{\varphi}Uf, Ug \rangle _2 \\ & = \langle U^* \check{T}_{\varphi}Uf, g \rangle_{t} . \end{align*} |
This gives the desired result.
In the next theorem, we apply Lemma 4.1 to establish a criterion of co-isometry for the H-Toeplitz operator on \mathfrak{D}_{t} .
Theorem 4.3. Suppose t > -1 and \varphi\in \mathcal{M} is a nonzero, co-analytic function on \mathbb{D} . Then, S_{\varphi} is a co-isometry on \mathfrak{D}_{t} if and only if \varphi = 1 on \mathbb{D} .
Proof. Let \varphi\in \mathcal{M} be a nonzero, co-analytic function on \mathbb{D} . Then, by Lemma 4.1,
\begin{aligned} S_\varphi S_\varphi^*\left(z^k\right) & = \left(P M_\varphi K\right)\left(K^* M^*_{\varphi}P\right)\left(z^k\right)\\ & = P M_\varphi T^*_{\varphi}\left(z^k\right) \\ & = P M_\varphi\left(U^{*}\check{T}_{\varphi}U\right)^*\left(z^k\right) \\ & = P M_\varphi U^{*}\check{T}_{\overline{\varphi}}U\left(z^k\right)\\ & = P M_\varphi U^{*}\left(k\overline{\varphi}z^{k-1}\right)\\ & = P M_\varphi \left(\overline{\varphi}z^{k}\right)\\ & = T_{|\varphi|^2}\left(z^k\right) \end{aligned} |
for arbitrary k\in\mathbb{N} . Since the polynomials are dense in \mathfrak{D}_{t} , it follows that
\begin{align} S_\varphi S_\varphi^* = T_{|\varphi|^2}. \end{align} | (4.9) |
Assume that S_\varphi is a co-isometry on \mathfrak{D}_{t} , that is, S_\varphi S_\varphi^* = I . Thus, by (4.9), we have T_{1-|\varphi|^2} = 0 . Since 1-\overline{\varphi} is analytic, it follows that
T_{1-\varphi}T_{1-\overline{\varphi}} = 0. |
Similar to [15, Corollary 10], we conclude that either 1-\varphi = 0 or 1-\overline{\varphi} = 0 , which gives that \varphi = 1 on \mathbb{D} .
Conversely, if \varphi = 1 on \mathbb{D} , then S_\varphi S_\varphi^* = T_{1} = I by (4.9), which means that S_\varphi is a co-isometry on \mathfrak{D}_{t} . This completes the proof of the theorem.
Let \mathcal{B}(\mathfrak{D}_{t}) denote the algebra consisting of all bounded linear operators on the Dirichlet type space \mathfrak{D}_{t} . We are going to show that the map \varphi\mapsto S_{\varphi} is one-to-one if the domain is \mathfrak{H} , which is given in the following.
Lemma 4.2. The map \gamma:\mathfrak{H} \to \mathcal{B}(\mathfrak{D}_{t}) defined by \gamma(\varphi) = S_{\varphi} is one-to-one.
Proof. Let \varphi, \psi\in \mathfrak{H} , which are defined by
\varphi(z) = \sum\limits_{i = 0}^{\infty}a_{i}z^{i}+\sum\limits_{j = 1}^{\infty}b_{j}\overline{z}^{j},\quad z\in\mathbb{D},\ a_{i},b_{j}\in \mathbb{C}, |
and
\psi(z) = \sum\limits_{i = 0}^{\infty}a^{\prime}_{i}z^{i}+\sum\limits_{j = 1}^{\infty}b^{\prime}_{j}\overline{z}^{j},\quad z\in\mathbb{D},\ a^{\prime}_{i},b^{\prime}_{j}\in \mathbb{C}, |
respectively. If S_{\varphi} = S_{\psi} , then S_{\varphi-\psi}(e_{k}) = 0 for all k\in\mathbb{N} . In particular, S_{\varphi-\psi}(e_{2}) = 0 , that is, PM_{\varphi-\psi}K(e_{2}) = 0 . More precisely,
P\left(\sum\limits_{i = 0}^{\infty}(a_{i}-a^{\prime}_{i})z^{i+1}+\sum\limits_{j = 1}^{\infty}(b_{j}-b^{\prime}_{j})\overline{z}^{j}z\right) = 0. |
Applying Lemma 2.1, we derive that
\sum\limits_{i = 0}^{\infty}(a_{i}-a^{\prime}_{i})z^{i+1} = 0. |
Therefore, a_{i} = a^{\prime}_{i} for all i\geq0 . Moreover, S_{\varphi-\psi}(e_{4}) = 0 , thus we obtain
P\left(\sum\limits_{i = 0}^{\infty}(a_{i}-a^{\prime}_{i})z^{i+2}+\sum\limits_{j = 1}^{\infty}(b_{j}-b^{\prime}_{j})\overline{z}^{j}z^{2}\right) = 0. |
Using Lemma 2.1 again, we get
\frac{2}{t+2} (b_{1}-b^{\prime}_{1})z = 0, |
hence b_{1} = b^{\prime}_{1} . Continuing the above process for e_{6} , e_{8} , e_{10} and so on, we obtain b_{j} = b^{\prime}_{j} for all j \geq2 , and then \varphi = \psi . This proves the desired result.
In the next result, we give a necessary and sufficient condition for an H-Toeplitz operator to be a partial isometry on the Dirichlet type space \mathfrak{D}_{t} .
Theorem 4.4. Suppose t > -1 and \varphi\in \mathcal{M} is a nonzero, co-analytic function on \mathbb{D} . Then S_\varphi is a partial isometry on \mathfrak{D}_{t} if and only if \varphi = 1 on \mathbb{D} .
Proof. If \varphi = 1 on \mathbb{D} , then S_\varphi is a co-isometry by Theorem 4.3. Thus, S_\varphi is a partial isometry.
Conversely, suppose S_\varphi is a partial isometry on \mathfrak{D}_{t} . Then, by [17, Theorem 2.3.3], we have S_\varphi S_\varphi^{*}S_\varphi = S_\varphi . In view of (4.9), we get
T_{|\varphi|^{2}}S_\varphi = S_\varphi, |
or equivalently,
T_{1-|\varphi|^{2}}S_\varphi = 0. |
Since \varphi\neq 0 , we have S_\varphi\neq 0 by Lemma 4.2. Thus, T_{1-|\varphi|^{2}} = 0 . The desired result is then obtained by proceeding as in the proof of Lemma 4.3.
As an operator on the Hilbert space, S_\varphi is a partial isometry if and only if S_\varphi^* is a partial isometry for \varphi\in \mathcal{M} ; see [19, Proposition 4.38]. Thus, combining Theorem 4.3 with Theorem 4.4, we get the following corollary.
Corollary 4.1. Suppose t > -1 and \varphi\in \mathcal{M} is a nonzero, co-analytic function on \mathbb{D} . Then, the following statements are equivalent:
(a) S_\varphi^* is a isometry on \mathfrak{D}_{t} .
(b) S_\varphi^* is a partial isometry on \mathfrak{D}_{t} .
(c) \varphi = 1 on \mathbb{D} .
For any fixed positive integer M , define
H_{M} = \text{span}\left\lbrace z^{l},1\leq l\leq2M\right\rbrace. |
Then H_{M} is a closed subspace of the Dirichlet type space \mathfrak{D}_{t} . In fact, the following theorem reveals that it is the kernel of H-Toeplitz operator with some co-analytic symbol.
Theorem 4.5. Suppose t > -1 and M is a fixed positive integer. Let \varphi(z) = \sum_{l = M}^{\infty}a_{l}\overline{z}^l\in \mathcal{M} . Then, the subspace H_{M} of \mathfrak{D}_{t} is the kernel of the H-Toeplitz operator S_{\varphi} .
Proof. Consider positive integers i, j satisfying M \leq i < \infty and 1\leq j\leq2M . If j = 2k for some k\in\mathbb{N} , then by Lemma 2.1
\begin{align*} S_{\overline{z}^i}(z^j) = PM_{\overline{z}^i}K\left(z^{2k}\right) = \begin{cases} \frac{\sqrt{2\, k!\, (2k)!}\,\Gamma(k-i+t+1)}{\sqrt{\Gamma(2k+t+1)\,\Gamma(k+t+1)}\,(k-i)!} z^{k-i}, & \text {if } k > i, \\ 0, & \text {if } k\le i. \end{cases} \end{align*} |
Note that M \leq i < \infty and 1\leq k\leq M , then S_{\overline{z}^i}(z^j) is equal to 0 in the case of j = 2k . If j = 2k-1 for some k\in\mathbb{N} , similarly, we get
\begin{align*} S_{\overline{z}^i}(z^j) = PM_{\overline{z}^i}K\left(z^{2k-1}\right) = \frac{\sqrt{(2k-1)\, (2k-1)!\,\Gamma(k+t+1)}}{\sqrt{k\,k!\,\Gamma(2k+t)}}P(\overline{z}^{i+k}) = 0. \end{align*} |
Hence, S_{\overline{z}^i}(z^j) = 0 for the positive integers i , j satisfying M \leq i < \infty and 1\leq j \leq2M . Now, for \varphi(z) = \sum_{l = M}^{\infty}a_{l}\overline{z}^l\in \mathcal{M} , by Proposition 1(a) and a limiting argument, we see that
S_{\varphi}(z^j) = \sum\limits_{l = M}^{\infty}a_{l}S_{\overline{z}^{l}}(z^j). |
Hence, we have S_{\varphi}(z^j) = 0 for all 1\leq j \leq2M . Therefore, we conclude that H_{M} is the kernel of S_{\varphi} .
Taking the symbol as a polynomial harmonic function for the H-Toeplitz operator, we can prove its kernel is infinite-dimensional.
Theorem 4.6. If \psi \in \mathcal{M} is a polynomial harmonic function, then \dim \ker S_{\psi} = \infty .
Proof. Observe that if \psi is a co-analytic function in \mathcal{M} , then S_{\psi}\left(zf(z^{2}) \right) = 0 for suitable choice of function f\in\mathfrak{D}_{t} . This implies that \ker S_{\psi}\ne \left\{ 0 \right\} . Now, suppose that M , N\in\mathbb{N} are arbitrary given integers, set \psi(z) = \sum_{s = 0}^{N}a_{s}z^{s}+\sum_{m = 1}^{M}b_{m}\overline{z}^{m} . Let \alpha = \max\left\{ M, N \right\} and choose f(z) = \sum_{i = \alpha}^{\infty}c_{i}z^{2i+1}\in\mathfrak{D}_{t} . We can obtain
\begin{align*} \begin{aligned} S_{\psi} f(z) & = P M_{\psi} K \left( \sum\limits_{i = \alpha}^{\infty} c_{i}z^{2i+1} \right) \\ & = PM_{\psi}\left(\sum\limits_{i = \alpha}^{\infty} \frac{\sqrt{(2i+1)(2i+1)!\,\Gamma(i+t+2)}}{\sqrt{(i+1)(i+1)!\,\Gamma(2i+t+2)}}c_{i} \overline{z}^{i+1}\right) \\ & = P \left( \left( \sum\limits_{s = 0}^{N}a_{s}z^{s}+\sum\limits_{m = 1}^{M}b_{m}\overline{z}^{m} \right) \left( \sum\limits_{i = \alpha}^{\infty} \frac{\sqrt{(2i+1)(2i+1)!\,\Gamma(i+t+2)}}{\sqrt{(i+1)(i+1)!\,\Gamma(2i+t+2)}}c_{i} \overline{z}^{i+1} \right) \right) \\ & = P \left( \left( \sum\limits_{s = 0}^{N}a_{s}z^{s} \right) \left( \sum\limits_{i = \alpha}^{\infty} \frac{\sqrt{(2i+1)(2i+1)!\,\Gamma(i+t+2)}}{\sqrt{(i+1)(i+1)!\,\Gamma(2i+t+2)}}c_{i} \overline{z}^{i+1} \right) \right) = 0, \end{aligned} \end{align*} |
where the last equality follows from Lemma 2.1. Similarly, for all n\in\mathbb{N} , S_{\psi}\left(z^{2n} f(z) \right) = 0 . Hence, if a nonzero function g\in\ker S_{\psi} , then \sum_{k = 1}^{n}\lambda_{k}z^{2k}g\in\ker S_{\psi} for n\in\mathbb{N} and \lambda_{k}\in\mathbb{C} . In particular, the set \left\{ z^{2n}g: n\in\mathbb{N} \right\} is a linear independent set. In fact, suppose \sum_{k = 1}^{n}\lambda_{k}z^{2k}g(z) = 0 but g\ne0 , then \sum_{k = 1}^{n}\lambda_{k}z^{2k} vanishes on a positive measure set so that \lambda_{k} = 0 for k = 1, 2, \cdots, n . This shows that \left\{ z^{2}g, z^{4}g, \cdots, z^{2n}g \right\} is linear independent. This is true for all n\in\mathbb{N} and all such functions in \ker S_{\psi} , so \ker S_{\psi} is infinite dimensional.
It is well-known that the C^* -algebra generated by self-adjoint operators is abelian and hence its algebraic structure is primitive. As examples of non-self-adjoint operators, the C^* -algebra generated by H-Toeplitz operators is complicated. Therefore, it is of great importance to study the condition for commutativity of H-Toeplitz operators.
The subsequent theorem characterizes when two H-Toeplitz operators with analytic symbols commute on \mathfrak{D}_{t} under certain conditions.
Theorem 4.7. Suppose t > -1 . Let \varphi = \sum_{i = 1}^{\infty}a_iz^{i} and \psi = \sum_{j = 1}^{\infty}b_jz^{j} in \mathcal{M} , where z\in\mathbb{D} , a_i , b_j\ne 0 for all i , j\in\mathbb{N} and \frac{b_{1}}{a_{1}} = \frac{b_{2i+1}}{a_{2i+1}} for all i\in\mathbb{N} . If \frac{b_{i+k}}{a_{i+k}} \ge \frac{b_{2i}}{a_{2i}} for all i , k\in\mathbb{N} , then S_{\varphi} and S_{\psi} commute on \mathfrak{D}_{t} if and only if \varphi and \psi are linearly dependent.
Proof. We show the forward implication only because the reverse implication is trivial. Suppose S_{\varphi}S_{\psi} = S_{\psi}S_{\varphi} . In particular, S_{\varphi}S_{\psi}(z) = S_{\psi}S_{\varphi}(z) , that is,
\begin{align*} PM_{\varphi}KP\left( \sum\limits_{j = 1}^{\infty}b_jz^{j}\overline{z} \right) = PM_{\psi}KP\left( \sum\limits_{i = 1}^{\infty}a_iz^{i}\overline{z} \right). \end{align*} |
Hence, by Lemma 2.1,
\begin{align*} PM_{\varphi}K\left( \sum\limits_{j = 1}^{\infty}\frac{(j+1)b_{j+1}}{j+1+t} z^{j} \right) = PM_{\psi}K\left( \sum\limits_{i = 1}^{\infty}\frac{(i+1)a_{i+1}}{i+1+t}z^{i} \right). \end{align*} |
Using Lemma 2.1 again,
\begin{align*} &\sum\limits_{k = 1}^{\infty} \sum\limits_{i = 1}^{\infty} \frac{(2k+1)\sqrt{2(2k)!\,\Gamma(k+t+1)}} {(2k+1+t)\sqrt{k!\,\Gamma(2k+t+1)}} b_{2k+1} a_{i} z^{i+k}\\ &+\sum\limits_{k = 1}^{\infty} \sum\limits_{i > k}^{\infty} \frac{2k\sqrt{(2k-1)(2k-1)!\,\Gamma(k+t+1)}} {(2k+t)\sqrt{k\,k!\,\Gamma(2k+t)}} b_{2k} a_{i} z^{i-k} \\ = &\sum\limits_{k = 1}^{\infty} \sum\limits_{j = 1}^{\infty} \frac{(2k+1)\sqrt{2(2k)!\,\Gamma(k+t+1)}} {(2k+1+t)\sqrt{k!\,\Gamma(2k+t+1)}} a_{2k+1} b_{j} z^{j+k}\\ &+\sum\limits_{k = 1}^{\infty} \sum\limits_{j > k}^{\infty} \frac{2k\sqrt{(2k-1)(2k-1)!\,\Gamma(k+t+1)}} {(2k+t)\sqrt{k\,k!\,\Gamma(2k+t)}} a_{2k} b_{j} z^{j-k}. \end{align*} |
Then, comparing the coefficients of z in the above equation, we get
\begin{align*} \sum\limits_{k = 1}^{\infty} \frac{2k\sqrt{(2k-1)(2k-1)!\,\Gamma(k+t+1)}} {(2k+t)\sqrt{k\,k!\,\Gamma(2k+t)}} \left(b_{2k}a_{k+1}-a_{2k}b_{k+1}\right)z = 0, \end{align*} |
which implies that \frac{b_{i+1}}{a_{i+1}} = \frac{b_{2i}}{a_{2i}} for each i\in\mathbb{N} by the hypothesis \frac{b_{i+k}}{a_{i+k}} \ge \frac{b_{2i}}{a_{2i}} . Similarly, comparing the coefficients of z^{2} , we get
\begin{align*} \frac{3\sqrt{4\,\Gamma(t+2)}}{(3+t)\sqrt{\Gamma(t+3)}} \left(b_{3}a_{1}-a_{3}b_{1}\right) z^{2} +\sum\limits_{k = 1}^{\infty} \frac{2k\sqrt{(2k-1)(2k-1)!\,\Gamma(k+t+1)}} {(2k+t)\sqrt{k\,k!\,\Gamma(2k+t)}} (b_{2k}a_{k+2}-a_{2k}b_{k+2}) z^{2} = 0, \end{align*} |
which means that \frac{b_{i+2}}{a_{i+2}} = \frac{b_{2i}}{a_{2i}} for each i\in\mathbb{N} by the hypothesis \frac{b_{i+k}}{a_{i+k}} \ge \frac{b_{2i}}{a_{2i}} again. Continuing in this fashion, we obtain that \frac{b_{i+k}}{a_{i+k}} = \frac{b_{2}}{a_{2}} for each i , k\in\mathbb{N} . Therefore, b_i = \lambda a_i for each integer i\ge 1 , where \lambda = \frac{b_{2}}{a_{2}} is a constant. It follows that \psi = \lambda\varphi .
More generally, we use the same trick in Theorem 4.7 to obtain an equivalent condition for the commutativity of H-Toeplitz operators with polynomial harmonic symbols.
Theorem 4.8. Suppose t > -1 . Let \varphi = \sum_{i = 1}^{\infty}a_iz^{i}+\sum_{j = 1}^{\infty}b_j\overline{z}^{j} and \psi = \sum_{m = 1}^{\infty}c_mz^{m}+\sum_{n = 1}^{\infty}d_n\overline{z}^{n} in \mathcal{M} , where a_i , b_j , c_m , d_n\ne 0 for i , j , m , d\in\mathbb{N} and \frac{c_{1}}{a_{1}} = \frac{c_{2i+1}}{a_{2i+1}} for all i\in\mathbb{N} . If \frac{a_{i+k}}{c_{i+k}} \ge \frac{a_{2i}}{c_{2i} } and \frac{b_{j}}{d_{j}} \ge \frac{a_{2(j+k)+1}}{c_{2(j+k)+1}} for all i , j , k\in\mathbb{N} , then S_{\varphi} and S_{\psi} commute on \mathfrak{D}_{t} if and only if \varphi and \psi are linearly dependent.
In this research, we conduct a study of H-Toeplitz operators on the Dirichlet type space \mathfrak{D}_{t} . Specifically, the compactness, self-adjointness, diagonality, co-isometry, partial isometry and commutativity of H-Toeplitz operators on \mathfrak{D}_{t} are characterized.
Peiying Huang and Yiyuan Zhang: Conceptualization, Formal analysis, Methodology, Writing-original draft, Validation, Writing-review & editing. All authors have read and approved the final version of the manuscript for publication.
The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.
This work was supported by the Guangdong Basic and Applied Basic Research Foundation (No. 2022A1515111187).
The authors declare that they have no competing interests.
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