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The original Weyl-Titchmarsh functions and sectorial Schrödinger L-systems

S. Belyi Department of Mathematics
Troy University
Troy, AL 36082, USA
[email protected]
 and  E. Tsekanovskiĭ Department of Mathematics
Niagara University
Lewiston, NY 14109
USA
[email protected] Dedicated with great pleasure to Seppo Hassi on the occasion of his 60-th birthday
(Date: DD/MM/2004)
Abstract.

In this paper we study the L-system realizations generated by the original Weyl-Titchmarsh functions mα(z)m_{\alpha}(z) in the case when the minimal symmetric Schrödinger operator in L2[,+)L_{2}[\ell,+\infty) is non-negative. We realize functions (mα(z))(-m_{\alpha}(z)) as impedance functions of Schrödinger L-systems and derive necessary and sufficient conditions for (mα(z))(-m_{\alpha}(z)) to fall into sectorial classes Sβ1,β2S^{\beta_{1},\beta_{2}} of Stieltjes functions. Moreover, it is shown that the knowledge of the value m(0)m_{\infty}(-0) and parameter α\alpha allows us to describe the geometric structure of the L-system that realizes (mα(z))(-m_{\alpha}(z)). Conditions when the main and state space operators of the L-system realizing (mα(z))(-m_{\alpha}(z)) have the same or not angle of sectoriality are presented in terms of the parameter α\alpha. Example that illustrates the obtained results is presented in the end of the paper.

Key words and phrases:
L-system, Schrödinger operator, transfer function, impedance function, Herglotz-Nevanlinna function, Stieltjes function, Weyl-Titchmarsh function
1991 Mathematics Subject Classification:
Primary 47A10; Secondary 47N50, 81Q10

1. Introduction

This paper is a part of an ongoing project studying the realizations of the original Weyl-Titchmarsh function m(z)m_{\infty}(z) and its linear-fractional transformation mα(z)m_{\alpha}(z) associated with a Schrödinger operator in L2[,+)L_{2}[\ell,+\infty). In this project the Herglotz-Nevanlinna functions (m(z))(-m_{\infty}(z)) and (1/m(z))(1/m_{\infty}(z)) as well as (mα(z))(-m_{\alpha}(z)) and (1/mα(z))(1/m_{\alpha}(z)) are being realized as impedance functions of L-systems with a dissipative Schrödinger main operator ThT_{h}, (Imh>0\operatorname{Im}h>0). For the sake of brevity we will refer to these L-systems as Schrödinger L-systems for the rest of the manuscript. The formal definition, exposition and discussions of general and Schrödinger L-systems are presented in Sections 2 and 4. We capitalize on the fact that all Schrödinger L-systems Θμ,h\Theta_{\mu,h} form a two-parametric family whose members are uniquely defined by a real-valued parameter μ\mu and a complex boundary value hh of the main dissipative operator.

The focus of this paper is set on the case when the realizing Schrödinger L-systems are based on non-negative symmetric Schrödinger operator with (1,1)(1,1) deficiency indices and have accretive state-space operator. It is known (see [2]) that in this case the impedance functions of such L-systems are Stieltjes. Here we study the situation when the realizing Schrödinger L-systems are also sectorial and the Weyl-Titchmarsh functions (mα(z))(-m_{\alpha}(z)) fall into sectorial classes SβS^{\beta} and Sβ1,β2S^{\beta_{1},\beta_{2}} of Stieltjes functions that are discussed in details in Section 3. Section 5 provides us with the general realization results (obtained in [7]) for the functions (m(z))(-m_{\infty}(z)), (1/m(z))(1/m_{\infty}(z)), and (mα(z))(-m_{\alpha}(z)). It is shown that (m(z))(-m_{\infty}(z)), (1/m(z))(1/m_{\infty}(z)), and (mα(z))(-m_{\alpha}(z)) can be realized as the impedance function of Schrödinger L-systems Θ0,i\Theta_{0,i}, Θ,i\Theta_{\infty,i}, and Θtanα,i\Theta_{\tan\alpha,i}, respectively.

The main results of the paper are contained in Section 6. Here we apply the realization theorems from Section 5 to Schrödinger L-systems that are based on non-negative symmetric Schrödinger operator to obtain additional properties. Utilizing the results presented in Section 4, we derive some new features of Schrödinger L-systems Θtanα,i\Theta_{\tan\alpha,i} whose impedance functions fall into particular sectorial classes Sβ1,β2S^{\beta_{1},\beta_{2}} with β1\beta_{1} and β2\beta_{2} explicitly described. The results are given in terms of the parameter α\alpha that appears in the definition of the function mα(z)m_{\alpha}(z). Moreover, the knowledge of the limit value m(0)m_{\infty}(-0) and the value of α\alpha allows us to find the angle of sectoriality of the main and state-space operators of the realizing L-system. This, in turn, leads to connections to Kato’s problem about sectorial extension of sectorial forms.

The paper is concluded with an example that illustrates main results and concepts. The present work is a further development of the theory of open physical systems conceived by M. Livs̆ic in [19].

2. Preliminaries

For a pair of Hilbert spaces 1{\mathcal{H}}_{1}, 2{\mathcal{H}}_{2} we denote by [1,2][{\mathcal{H}}_{1},{\mathcal{H}}_{2}] the set of all bounded linear operators from 1{\mathcal{H}}_{1} to 2{\mathcal{H}}_{2}. Let A˙{\dot{A}} be a closed, densely defined, symmetric operator in a Hilbert space {\mathcal{H}} with inner product (f,g),f,g(f,g),f,g\in{\mathcal{H}}. Any non-symmetric operator TT in {\mathcal{H}} such that A˙TA˙{\dot{A}}\subset T\subset{\dot{A}}^{*} is called a quasi-self-adjoint extension of A˙{\dot{A}}.

Consider the rigged Hilbert space (see [11], [2]) +,{\mathcal{H}}_{+}\subset{\mathcal{H}}\subset{\mathcal{H}}_{-}, where +=Dom(A˙){\mathcal{H}}_{+}=\text{\rm{Dom}}({\dot{A}}^{*}) and

(1) (f,g)+=(f,g)+(A˙f,A˙g),f,gDom(A).(f,g)_{+}=(f,g)+({\dot{A}}^{*}f,{\dot{A}}^{*}g),\;\;f,g\in\text{\rm{Dom}}(A^{*}).

Let {\mathcal{R}} be the Riesz-Berezansky operator {\mathcal{R}} (see [11], [2]) which maps \mathcal{H}_{-} onto +\mathcal{H}_{+} such that (f,g)=(f,g)+(f,g)=(f,{\mathcal{R}}g)_{+} (f+\forall f\in{\mathcal{H}}_{+}, gg\in{\mathcal{H}}_{-}) and g+=g\|{\mathcal{R}}g\|_{+}=\|g\|_{-}. Note that identifying the space conjugate to ±{\mathcal{H}}_{\pm} with {\mathcal{H}}_{\mp}, we get that if 𝔸[+,]{\mathbb{A}}\in[{\mathcal{H}}_{+},{\mathcal{H}}_{-}], then 𝔸[+,].{\mathbb{A}}^{*}\in[{\mathcal{H}}_{+},{\mathcal{H}}_{-}]. An operator 𝔸[+,]{\mathbb{A}}\in[{\mathcal{H}}_{+},{\mathcal{H}}_{-}] is called a self-adjoint bi-extension of a symmetric operator A˙{\dot{A}} if 𝔸=𝔸{\mathbb{A}}={\mathbb{A}}^{*} and 𝔸A˙{\mathbb{A}}\supset{\dot{A}}. Let 𝔸{\mathbb{A}} be a self-adjoint bi-extension of A˙{\dot{A}} and let the operator A^\hat{A} in {\mathcal{H}} be defined as follows:

Dom(A^)={f+:𝔸f},A^=𝔸Dom(A^).\text{\rm{Dom}}(\hat{A})=\{f\in{\mathcal{H}}_{+}:{\mathbb{A}}f\in{\mathcal{H}}\},\quad\hat{A}={\mathbb{A}}{\upharpoonright\,}\text{\rm{Dom}}(\hat{A}).

The operator A^\hat{A} is called a quasi-kernel of a self-adjoint bi-extension 𝔸{\mathbb{A}} (see [26], [2, Section 2.1]). A self-adjoint bi-extension 𝔸{\mathbb{A}} of a symmetric operator A˙{\dot{A}} is called t-self-adjoint (see [2, Definition 4.3.1]) if its quasi-kernel A^\hat{A} is self-adjoint operator in {\mathcal{H}}. An operator 𝔸[+,]{\mathbb{A}}\in[{\mathcal{H}}_{+},{\mathcal{H}}_{-}] is called a quasi-self-adjoint bi-extension of an operator TT if 𝔸TA˙{\mathbb{A}}\supset T\supset{\dot{A}} and 𝔸TA˙.{\mathbb{A}}^{*}\supset T^{*}\supset{\dot{A}}. We will be mostly interested in the following type of quasi-self-adjoint bi-extensions. Let TT be a quasi-self-adjoint extension of A˙{\dot{A}} with nonempty resolvent set ρ(T)\rho(T). A quasi-self-adjoint bi-extension 𝔸{\mathbb{A}} of an operator TT is called (see [2, Definition 3.3.5]) a (*)-extension of TT if Re𝔸{\rm Re\,}{\mathbb{A}} is a t-self-adjoint bi-extension of A˙{\dot{A}}. In what follows we assume that A˙{\dot{A}} has deficiency indices (1,1)(1,1). In this case it is known [2] that every quasi-self-adjoint extension TT of A˙{\dot{A}} admits ()(*)-extensions. The description of all ()(*)-extensions via Riesz-Berezansky operator {\mathcal{R}} can be found in [2, Section 4.3].

Recall that a linear operator TT in a Hilbert space {\mathcal{H}} is called accretive [17] if Re(Tf,f)0{\rm Re\,}(Tf,f)\geq 0 for all fDom(T)f\in\text{\rm{Dom}}(T). We call an accretive operator TT β\beta-sectorial [17] if there exists a value of β(0,π/2)\beta\in(0,\pi/2) such that

(2) (cotβ)|Im(Tf,f)|Re(Tf,f),fDom(T).(\cot\beta)|\operatorname{Im}(Tf,f)|\leq\,{\rm Re\,}(Tf,f),\qquad f\in\text{\rm{Dom}}(T).

We say that the angle of sectoriality β\beta is exact for a β\beta-sectorial operator TT if

tanβ=supfDom(T)|Im(Tf,f)|Re(Tf,f).\tan\beta=\sup_{f\in\text{\rm{Dom}}(T)}\frac{|\operatorname{Im}(Tf,f)|}{{\rm Re\,}(Tf,f)}.

An accretive operator is called extremal accretive if it is not β\beta-sectorial for any β(0,π/2)\beta\in(0,\pi/2). A ()(*)-extension 𝔸{\mathbb{A}} of TT is called accretive if Re(𝔸f,f)0{\rm Re\,}({\mathbb{A}}f,f)\geq 0 for all f+f\in{\mathcal{H}}_{+}. This is equivalent to that the real part Re𝔸=(𝔸+𝔸)/2{\rm Re\,}{\mathbb{A}}=({\mathbb{A}}+{\mathbb{A}}^{*})/2 is a nonnegative t-self-adjoint bi-extension of A˙{\dot{A}}.

The following definition is a “lite” version of the definition of L-system given for a scattering L-system with one-dimensional input-output space. It is tailored for the case when the symmetric operator of an L-system has deficiency indices (1,1)(1,1). The general definition of an L-system can be found in [2, Definition 6.3.4] (see also [10] for a non-canonical version).

Definition 1.

An array

(3) Θ=(𝔸K 1+)\Theta=\begin{pmatrix}{\mathbb{A}}&K&\ 1\cr{\mathcal{H}}_{+}\subset{\mathcal{H}}\subset{\mathcal{H}}_{-}&&{\mathbb{C}}\cr\end{pmatrix}

is called an L-system if:

  1. (1)

    TT is a dissipative (Im(Tf,f)0\operatorname{Im}(Tf,f)\geq 0, fDom(T)f\in\text{\rm{Dom}}(T)) quasi-self-adjoint extension of a symmetric operator A˙{\dot{A}} with deficiency indices (1,1)(1,1);

  2. (2)

    𝔸\mathbb{A} is a (\ast)-extension of TT;

  3. (3)

    Im𝔸=KK\operatorname{Im}{\mathbb{A}}=KK^{*}, where K[,]K\in[{\mathbb{C}},{\mathcal{H}}_{-}] and K[+,]K^{*}\in[{\mathcal{H}}_{+},{\mathbb{C}}].

Operators TT and 𝔸{\mathbb{A}} are called a main and state-space operators respectively of the system Θ\Theta, and KK is a channel operator. It is easy to see that the operator 𝔸{\mathbb{A}} of the system (3) is such that Im𝔸=(,χ)χ\operatorname{Im}{\mathbb{A}}=(\cdot,\chi)\chi, χ\chi\in{\mathcal{H}}_{-} and pick Kc=cχKc=c\cdot\chi, cc\in{\mathbb{C}} (see [2]). A system Θ\Theta in (3) is called minimal if the operator A˙{\dot{A}} is a prime operator in {\mathcal{H}}, i.e., there exists no non-trivial reducing invariant subspace of {\mathcal{H}} on which it induces a self-adjoint operator. Minimal L-systems of the form (3) with one-dimensional input-output space were also considered in [6].

We associate with an L-system Θ\Theta the function

(4) WΘ(z)=I2iK(𝔸zI)1K,zρ(T),W_{\Theta}(z)=I-2iK^{\ast}(\mathbb{A}-zI)^{-1}K,\quad z\in\rho(T),

which is called the transfer function of the L-system Θ\Theta. We also consider the function

(5) VΘ(z)=K(Re𝔸zI)1K,V_{\Theta}(z)=K^{\ast}({\rm Re\,}{\mathbb{A}}-zI)^{-1}K,

that is called the impedance function of an L-system Θ\Theta of the form (3). The transfer function WΘ(z)W_{\Theta}(z) of the L-system Θ\Theta and function VΘ(z)V_{\Theta}(z) of the form (5) are connected by the following relations valid for Imz0\operatorname{Im}z\neq 0, zρ(T)z\in\rho(T),

VΘ(z)\displaystyle V_{\Theta}(z) =i[WΘ(z)+I]1[WΘ(z)I],\displaystyle=i[W_{\Theta}(z)+I]^{-1}[W_{\Theta}(z)-I],
WΘ(z)\displaystyle W_{\Theta}(z) =(I+iVΘ(z))1(IiVΘ(z)).\displaystyle=(I+iV_{\Theta}(z))^{-1}(I-iV_{\Theta}(z)).

An L-system Θ\Theta of the form (3) is called an accretive L-system ([9], [14]) if its state-space operator operator 𝔸{\mathbb{A}} is accretive, that is Re(𝔸f,f)0{\rm Re\,}({\mathbb{A}}f,f)\geq 0 for all f+f\in{\mathcal{H}}_{+}. An accretive L-system is called sectorial if the operator 𝔸{\mathbb{A}} is sectorial, i.e., satisfies (2) for some β(0,π/2)\beta\in(0,\pi/2) and all f+f\in{\mathcal{H}}_{+}.

3. Sectorial classes and and their realizations

A scalar function V(z)V(z) is called the Herglotz-Nevanlinna function if it is holomorphic on {{\mathbb{C}}\setminus{\mathbb{R}}}, symmetric with respect to the real axis, i.e., V(z)=V(z¯)V(z)^{*}=V(\bar{z}), zz\in{{\mathbb{C}}\setminus{\mathbb{R}}}, and if it satisfies the positivity condition ImV(z)0\operatorname{Im}V(z)\geq 0, z+z\in{\mathbb{C}}_{+}. The class of all Herglotz-Nevanlinna functions, that can be realized as impedance functions of L-systems, and connections with Weyl-Titchmarsh functions can be found in [2], [6], [13], [15] and references therein. The following definition can be found in [16]. A scalar Herglotz-Nevanlinna function V(z)V(z) is a Stieltjes function if it is holomorphic in Ext[0,+)\operatorname{Ext}[0,+\infty) and

(6) Im[zV(z)]Imz0.\frac{\operatorname{Im}[zV(z)]}{\operatorname{Im}z}\geq 0.

It is known [16] that a Stieltjes function V(z)V(z) admits the following integral representation

(7) V(z)=γ+0dG(t)tz,V(z)=\gamma+\int\limits_{0}^{\infty}\frac{dG(t)}{t-z},

where γ0\gamma\geq 0 and G(t)G(t) is a non-decreasing on [0,+)[0,+\infty) function such that 0dG(t)1+t<.\int^{\infty}_{0}\frac{dG(t)}{1+t}<\infty. We are going to focus on the class S0(R)S_{0}(R) (see [9], [14], [2]) of scalar Stieltjes functions such that the measure G(t)G(t) in representation (7) is of unbounded variation. It was shown in [2] (see also [9]) that such a function V(z)V(z) can be realized as the impedance function of an accretive L-system Θ\Theta of the form (3) with a densely defined symmetric operator if and only if it belongs to the class S0(R)S_{0}(R).

Now we are going to consider sectorial subclasses of scalar Stieltjes functions introduced in [1]. Let β(0,π2)\beta\in(0,\frac{\pi}{2}). Sectorial subclasses SβS^{\beta} of Stieltjes functions are defined as follows: a scalar Stieltjes function V(z)V(z) belongs to SβS^{\beta} if

(8) Kβ=k,l=1n[zkV(zk)z¯lV(z¯l)zkz¯l(cotβ)V(z¯l)V(zk)]hkh¯l0,K_{\beta}=\sum_{k,l=1}^{n}\left[\frac{z_{k}V(z_{k})-\bar{z}_{l}V(\bar{z}_{l})}{z_{k}-\bar{z}_{l}}-{{(\cot\beta)}~{}}V(\bar{z}_{l})V(z_{k})\right]h_{k}\bar{h}_{l}\geq 0,

for an arbitrary sequences of complex numbers {zk}\{z_{k}\}, (Imzk>0\operatorname{Im}z_{k}>0) and {hk}\{h_{k}\}, (k=1,,nk=1,...,n). For 0<β1<β2<π20<\beta_{1}<\beta_{2}<\frac{\pi}{2}, we have

Sβ1Sβ2S,S^{\beta_{1}}\subset S^{\beta_{2}}\subset{S},

where SS denotes the class of all Stieltjes functions (which corresponds to the case β=π2\beta=\frac{\pi}{2}). Let Θ\Theta be a minimal L-system of the form (3) with a densely defined non-negative symmetric operator A˙{\dot{A}}. Then (see [2]) the impedance function VΘ(z)V_{\Theta}(z) defined by (5) belongs to the class SβS^{\beta} if and only if the operator 𝔸{\mathbb{A}} of the L-system Θ\Theta is β\beta-sectorial.

Let 0β1<π20\leq\beta_{1}<\frac{\pi}{2}, 0<β2π20<\beta_{2}\leq\frac{\pi}{2}, and β1β2\beta_{1}\leq\beta_{2}. We say that a scalar Stieltjes function V(z)V(z) belongs to the class Sβ1,β2S^{\,\beta_{1},\beta_{2}} if

(9) tanβ1=limxV(x),tanβ2=limx0V(x).\tan\beta_{1}=\lim_{x\to-\infty}V(x),\qquad\tan\beta_{2}=\lim_{x\to-0}V(x).

The following connection between the classes SβS^{\,\beta} and Sβ1,β2S^{\,\beta_{1},\beta_{2}} can be found in [2]. Let Θ\Theta be an L-system of the form (3) with a densely defined non-negative symmetric operator A˙{\dot{A}} with deficiency numbers (1,1).(1,1). Let also 𝔸{\mathbb{A}} be an β\beta-sectorial ()(*)-extension of TT. Then the impedance function VΘ(z)V_{\Theta}(z) defined by (5) belongs to the class Sβ1,β2S^{\beta_{1},\beta_{2}}, tanβ2tanβ\tan\beta_{2}\leq\tan\beta. Moreover, the main operator TT is (β2β1)(\beta_{2}-\beta_{1})-sectorial with the exact angle of sectoriality (β2β1)(\beta_{2}-\beta_{1}). In the case when β\beta is the exact angle of sectoriality of the operator TT we have that VΘ(z)S0,βV_{\Theta}(z)\in S^{0,\beta} (see [2]). It also follows that under this set of assumptions, the impedance function VΘ(z)V_{\Theta}(z) is such that γ=0\gamma=0 in representation (7).

Now let Θ\Theta be an L-system of the form (3), where 𝔸{\mathbb{A}} is a ()(*)-extension of TT and A˙{\dot{A}} is a closed densely defined non-negative symmetric operator with deficiency numbers (1,1).(1,1). It was proved in [2] that if the impedance function VΘ(z)V_{\Theta}(z) belongs to the class Sβ1,β2S^{\beta_{1},\beta_{2}} and β2π/2\beta_{2}\neq\pi/2, then 𝔸{\mathbb{A}} is β\beta-sectorial, where

(10) tanβ=tanβ2+2tanβ1(tanβ2tanβ1).\tan\beta=\tan\beta_{2}+2\sqrt{\tan\beta_{1}(\tan\beta_{2}-\tan\beta_{1})}.

Under the above set of conditions on L-system Θ\Theta, it is shown in [2] that 𝔸{\mathbb{A}} is β\beta-sectorial ()(*)-extension of an β\beta-sectorial operator TT with the exact angle β(0,π/2)\beta\in(0,\pi/2) if and only if VΘ(z)S0,βV_{\Theta}(z)\in S^{0,\beta}. Moreover, the angle β\beta can be found via the formula

(11) tanβ=0dG(t)t,\tan\beta=\int_{0}^{\infty}\frac{dG(t)}{t},

where G(t)G(t) is the measure from integral representation (7) of VΘ(z)V_{\Theta}(z).

4. L-systems with Schrödinger operator and their impedance functions

Let =L2[,+){\mathcal{H}}=L_{2}[\ell,+\infty), 0\ell\geq 0, and l(y)=y′′+q(x)yl(y)=-y^{\prime\prime}+q(x)y, where qq is a real locally summable on [,+)[\ell,+\infty) function. Suppose that the symmetric operator

(12) {A˙y=y′′+q(x)yy()=y()=0\left\{\begin{array}[]{l}{\dot{A}}y=-y^{\prime\prime}+q(x)y\\ y(\ell)=y^{\prime}(\ell)=0\\ \end{array}\right.

has deficiency indices (1,1). Let DD^{*} be the set of functions locally absolutely continuous together with their first derivatives such that l(y)L2[,+)l(y)\in L_{2}[\ell,+\infty). Consider +=Dom(A˙)=D{\mathcal{H}}_{+}=\text{\rm{Dom}}({\dot{A}}^{*})=D^{*} with the scalar product

(y,z)+=(y(x)z(x)¯+l(y)l(z)¯)𝑑x,y,zD.(y,z)_{+}=\int_{\ell}^{\infty}\left(y(x)\overline{z(x)}+l(y)\overline{l(z)}\right)dx,\;\;y,\;z\in D^{*}.

Let +L2[,+){\mathcal{H}}_{+}\subset L_{2}[\ell,+\infty)\subset{\mathcal{H}}_{-} be the corresponding triplet of Hilbert spaces. Consider the operators

(13) {Thy=l(y)=y′′+q(x)yhy()y()=0,{Thy=l(y)=y′′+q(x)yh¯y()y()=0,\left\{\begin{array}[]{l}T_{h}y=l(y)=-y^{\prime\prime}+q(x)y\\ hy(\ell)-y^{\prime}(\ell)=0\\ \end{array}\right.,\quad\left\{\begin{array}[]{l}T^{*}_{h}y=l(y)=-y^{\prime\prime}+q(x)y\\ \overline{h}y(\ell)-y^{\prime}(\ell)=0\\ \end{array}\right.,

where Imh>0\operatorname{Im}h>0. Let A˙{\dot{A}} be a symmetric operator of the form (12) with deficiency indices (1,1), generated by the differential operation l(y)=y′′+q(x)yl(y)=-y^{\prime\prime}+q(x)y. Let also φk(x,λ)(k=1,2)\varphi_{k}(x,\lambda)(k=1,2) be the solutions of the following Cauchy problems:

{l(φ1)=λφ1φ1(,λ)=0φ1(,λ)=1,{l(φ2)=λφ2φ2(,λ)=1φ2(,λ)=0.\left\{\begin{array}[]{l}l(\varphi_{1})=\lambda\varphi_{1}\\ \varphi_{1}(\ell,\lambda)=0\\ \varphi^{\prime}_{1}(\ell,\lambda)=1\\ \end{array}\right.,\qquad\left\{\begin{array}[]{l}l(\varphi_{2})=\lambda\varphi_{2}\\ \varphi_{2}(\ell,\lambda)=-1\\ \varphi^{\prime}_{2}(\ell,\lambda)=0\\ \end{array}\right..

It is well known [20], [18] that there exists a function m(λ)m_{\infty}(\lambda) introduced by H. Weyl [27], [28] for which

φ(x,λ)=φ2(x,λ)+m(λ)φ1(x,λ)\varphi(x,\lambda)=\varphi_{2}(x,\lambda)+m_{\infty}(\lambda)\varphi_{1}(x,\lambda)

belongs to L2[,+)L_{2}[\ell,+\infty). The function m(λ)m_{\infty}(\lambda) is not a Herglotz-Nevanlinna function but (m(λ))(-m_{\infty}(\lambda)) and (1/m(λ))(1/m_{\infty}(\lambda)) are.

Now we shall construct an L-system based on a non-self-adjoint Schrödinger operator ThT_{h} with Imh>0\operatorname{Im}h>0. It was shown in [4], [2] that the set of all (*)-extensions of a non-self-adjoint Schrödinger operator ThT_{h} of the form (13) in L2[,+)L_{2}[\ell,+\infty) can be represented in the form

(14) 𝔸μ,hy=y′′+q(x)y1μh[y()hy()][μδ(x)+δ(x)],𝔸μ,hy=y′′+q(x)y1μh¯[y()h¯y()][μδ(x)+δ(x)].\begin{split}&{\mathbb{A}}_{\mu,h}\,y=-y^{\prime\prime}+q(x)y-\frac{1}{\mu-h}\,[y^{\prime}(\ell)-hy(\ell)]\,[\mu\delta(x-\ell)+\delta^{\prime}(x-\ell)],\\ &{\mathbb{A}}^{*}_{\mu,h}\,y=-y^{\prime\prime}+q(x)y-\frac{1}{\mu-\overline{h}}\,[y^{\prime}(\ell)-\overline{h}y(\ell)]\,[\mu\delta(x-\ell)+\delta^{\prime}(x-\ell)].\end{split}

Moreover, the formulas (14) establish a one-to-one correspondence between the set of all (*)-extensions of a Schrödinger operator ThT_{h} of the form (13) and all real numbers μ[,+]\mu\in[-\infty,+\infty]. One can easily check that the (*)-extension 𝔸{\mathbb{A}} in (14) of the non-self-adjoint dissipative Schrödinger operator ThT_{h}, (Imh>0\operatorname{Im}h>0) of the form (13) satisfies the condition

Im𝔸μ,h=𝔸μ,h𝔸μ,h2i=(.,gμ,h)gμ,h,\operatorname{Im}{\mathbb{A}}_{\mu,h}=\frac{{\mathbb{A}}_{\mu,h}-{\mathbb{A}}^{*}_{\mu,h}}{2i}=(.,g_{\mu,h})g_{\mu,h},

where

(15) gμ,h=(Imh)12|μh|[μδ(x)+δ(x)]g_{\mu,h}=\frac{(\operatorname{Im}h)^{\frac{1}{2}}}{|\mu-h|}\,[\mu\delta(x-\ell)+\delta^{\prime}(x-\ell)]

and δ(x),δ(x)\delta(x-\ell),\delta^{\prime}(x-\ell) are the delta-function and its derivative at the point \ell, respectively. Furthermore,

(y,gμ,h)=(Imh)12|μh|[μy()y()],(y,g_{\mu,h})=\frac{(\operatorname{Im}h)^{\frac{1}{2}}}{|\mu-h|}\ [\mu y(\ell)-y^{\prime}(\ell)],

where y+y\in{\mathcal{H}}_{+}, gg\in{\mathcal{H}}_{-}, and +L2[,+){\mathcal{H}}_{+}\subset L_{2}[\ell,+\infty)\subset{\mathcal{H}}_{-} is the triplet of Hilbert spaces discussed above.

It was also shown in [2] that the quasi-kernel A^ξ\hat{A}_{\xi} of Re𝔸μ,h{\rm Re\,}{\mathbb{A}}_{\mu,h} is given by

(16) {A^ξy=y′′+q(x)yy()=ξy(),whereξ=μReh|h|2μReh.\left\{\begin{array}[]{l}\hat{A}_{\xi}y=-y^{\prime\prime}+q(x)y\\ y^{\prime}(\ell)=\xi y(\ell)\\ \end{array}\right.,\quad\textrm{where}\quad\xi=\frac{\mu{\rm Re\,}h-|h|^{2}}{\mu-{\rm Re\,}h}.

Let E=E={\mathbb{C}}, Kμ,hc=cgμ,h,(c)K_{\mu,h}{c}=cg_{\mu,h},\;(c\in{\mathbb{C}}). It is clear that

(17) Kμ,hy=(y,gμ,h),y+,K^{*}_{\mu,h}y=(y,g_{\mu,h}),\quad y\in{\mathcal{H}}_{+},

and Im𝔸μ,h=Kμ,hKμ,h.\operatorname{Im}{\mathbb{A}}_{\mu,h}=K_{\mu,h}K^{*}_{\mu,h}. Therefore, the array

(18) Θμ,h=(𝔸μ,hKμ,h1+L2[,+)),\Theta_{\mu,h}=\begin{pmatrix}{\mathbb{A}}_{\mu,h}&K_{\mu,h}&1\cr{\mathcal{H}}_{+}\subset L_{2}[\ell,+\infty)\subset{\mathcal{H}}_{-}&&{\mathbb{C}}\cr\end{pmatrix},

is an L-system with the main operator ThT_{h}, (Imh>0\operatorname{Im}h>0) of the form (13), the state-space operator 𝔸μ,h{\mathbb{A}}_{\mu,h} of the form (14), and with the channel operator Kμ,hK_{\mu,h} of the form (17). It was established in [4], [2] that the transfer and impedance functions of Θμ,h\Theta_{\mu,h} are

(19) WΘμ,h(z)=μhμh¯m(z)+h¯m(z)+h,W_{\Theta_{\mu,h}}(z)=\frac{\mu-h}{\mu-\overline{h}}\,\,\frac{m_{\infty}(z)+\overline{h}}{m_{\infty}(z)+h},

and

(20) VΘμ,h(z)=(m(z)+μ)Imh(μReh)m(z)+μReh|h|2.V_{\Theta_{\mu,h}}(z)=\frac{\left(m_{\infty}(z)+\mu\right)\operatorname{Im}h}{\left(\mu-{\rm Re\,}h\right)m_{\infty}(z)+\mu{\rm Re\,}h-|h|^{2}}.

It was shown in [2, Section 10.2] that if the parameters μ\mu and ξ\xi are related via (16), then the two L-systems Θμ,h\Theta_{\mu,h} and Θξ,h\Theta_{\xi,h} of the form (18) have the following property

(21) WΘμ,h(z)=WΘξ,h(z),VΘμ,h(z)=1VΘξ,h(z),whereξ=μReh|h|2μReh.W_{\Theta_{\mu,h}}(z)=-W_{\Theta_{\xi,h}}(z),\;V_{\Theta_{\mu,h}}(z)=-\frac{1}{V_{\Theta_{\xi,h}}(z)},\;\textrm{where}\quad\xi=\frac{\mu{\rm Re\,}h-|h|^{2}}{\mu-{\rm Re\,}h}.

5. Realizations of m(z)-m_{\infty}(z), 1/m(z)1/m_{\infty}(z) and mα(z)m_{\alpha}(z).

It is known [18], [20] that the original Weyl-Titchmarsh function m(z)m_{\infty}(z) has a property that (m(z))(-m_{\infty}(z)) is a Herglotz-Nevanlinna function. The question whether (m(z))(-m_{\infty}(z)) can be realized as the impedance function of a Schrödinger L-system is answered in the following theorem that was proved in [7].

Theorem 2 ([7]).

Let A˙{\dot{A}} be a symmetric Schrödinger operator of the form (12) with deficiency indices (1,1)(1,1) and locally summable potential in =L2[,).{\mathcal{H}}=L^{2}[\ell,\infty). If m(z)m_{\infty}(z) is the Weyl-Titchmarsh function of A˙{\dot{A}}, then the Herglotz-Nevanlinna function (m(z))(-m_{\infty}(z)) can be realized as the impedance function of a Schrödinger L-system Θμ,h\Theta_{\mu,h} of the form (18) with μ=0\mu=0 and h=ih=i.

Conversely, let Θμ,h\Theta_{\mu,h} be a Schrödinger L-system of the form (18) with the symmetric operator A˙{\dot{A}} such that VΘμ,h(z)=m(z),V_{\Theta_{\mu,h}}(z)=-m_{\infty}(z), for all z±z\in{\mathbb{C}}_{\pm} and μ{}\mu\in\mathbb{R}\cup\{\infty\}. Then the parameters μ\mu and hh defining Θμ,h\Theta_{\mu,h} are such that μ=0\mu=0 and h=ih=i.

A similar result for the function 1/m(z)1/m_{\infty}(z) was also proved in [7].

Theorem 3 ([7]).

Let A˙{\dot{A}} be a symmetric Schrödinger operator of the form (12) with deficiency indices (1,1)(1,1) and locally summable potential in =L2[,).{\mathcal{H}}=L^{2}[\ell,\infty). If m(z)m_{\infty}(z) is the Weyl-Titchmarsh function of A˙{\dot{A}}, then the Herglotz-Nevanlinna function (1/m(z))(1/m_{\infty}(z)) can be realized as the impedance function of a Schrödinger L-system Θμ,h\Theta_{\mu,h} of the form (18) with μ=\mu=\infty and h=ih=i.

Conversely, let Θμ,h\Theta_{\mu,h} be a Schrödinger L-system of the form (18) with the symmetric operator A˙{\dot{A}} such that VΘμ,h(z)=1m(z),V_{\Theta_{\mu,h}}(z)=\frac{1}{m_{\infty}(z)}, for all z±z\in{\mathbb{C}}_{\pm} and μ{}\mu\in\mathbb{R}\cup\{\infty\}. Then the parameters μ\mu and hh defining Θμ,h\Theta_{\mu,h} are such that μ=\mu=\infty and h=ih=i.

We note that both L-systems Θ0,i\Theta_{0,i} and Θ,i\Theta_{\infty,i} obtained in Theorems 2 and 3 share the same main operator

(22) {Tiy=y′′+q(x)yy()=iy().\left\{\begin{array}[]{l}T_{i}\,y=-y^{\prime\prime}+q(x)y\\ y^{\prime}(\ell)=i\,y(\ell)\\ \end{array}\right..

Now we recall the definition of Weyl-Titchmarsh functions mα(z)m_{\alpha}(z). Let A˙{\dot{A}} be a symmetric operator of the form (12) with deficiency indices (1,1), generated by the differential operation l(y)=y′′+q(x)yl(y)=-y^{\prime\prime}+q(x)y. Let also φα(x,z)\varphi_{\alpha}(x,{z}) and θα(x,z)\theta_{\alpha}(x,{z}) be the solutions of the following Cauchy problems:

{l(φα)=zφαφα(,z)=sinαφα(,z)=cosα,{l(θα)=zθαθα(,z)=cosαθα(,z)=sinα.\left\{\begin{array}[]{l}l(\varphi_{\alpha})={z}\varphi_{\alpha}\\ \varphi_{\alpha}(\ell,{z})=\sin\alpha\\ \varphi^{\prime}_{\alpha}(\ell,{z})=-\cos\alpha\\ \end{array}\right.,\qquad\left\{\begin{array}[]{l}l(\theta_{\alpha})={z}\theta_{\alpha}\\ \theta_{\alpha}(\ell,{z})=\cos\alpha\\ \theta^{\prime}_{\alpha}(\ell,{z})=\sin\alpha\\ \end{array}\right..

It is known [12], [20], [21] that there exists an analytic in ±{\mathbb{C}}_{\pm} function mα(z)m_{\alpha}({z}) for which

(23) ψ(x,z)=θα(x,z)+mα(z)φα(x,z)\psi(x,{z})=\theta_{\alpha}(x,{z})+m_{\alpha}({z})\varphi_{\alpha}(x,{z})

belongs to L2[,+)L_{2}[\ell,+\infty). It is easy to see that if α=π\alpha=\pi, then mπ(z)=m(z)m_{\pi}({z})=m_{\infty}({z}). The functions mα(z)m_{\alpha}({z}) and m(z)m_{\infty}(z) are connected (see [12], [21]) by

(24) mα(z)=sinα+m(z)cosαcosαm(z)sinα.m_{\alpha}({z})=\frac{\sin\alpha+m_{\infty}({z})\cos\alpha}{\cos\alpha-m_{\infty}({z})\sin\alpha}.

We know [20], [21] that for any real α\alpha the function mα(z)-m_{\alpha}({z}) is a Herglotz-Nevanlinna function. Also, modifying (24) slightly we obtain

(25) mα(z)=sinα+m(z)cosαcosα+m(z)sinα=cosα+1m(z)sinαsinα1m(z)cosα.-m_{\alpha}(z)=\frac{\sin\alpha+m_{\infty}(z)\cos\alpha}{-\cos\alpha+m_{\infty}(z)\sin\alpha}=\frac{\cos\alpha+\frac{1}{m_{\infty}(z)}\sin\alpha}{\sin\alpha-\frac{1}{m_{\infty}(z)}\cos\alpha}.

The following realization theorem (see [7]) for Herglotz-Nevanlinna functions mα(z)-m_{\alpha}(z) is similar to Theorem 2.

Theorem 4 ([7]).

Let A˙{\dot{A}} be a symmetric Schrödinger operator of the form (12) with deficiency indices (1,1)(1,1) and locally summable potential in =L2[,).{\mathcal{H}}=L^{2}[\ell,\infty). If mα(z)m_{\alpha}(z) is the function of A˙{\dot{A}} described in (23), then the Herglotz-Nevanlinna function (mα(z))(-m_{\alpha}(z)) can be realized as the impedance function of a Schrödinger L-system Θμ,h\Theta_{\mu,h} of the form (18) with

(26) μ=tanαandh=i.\mu=\tan\alpha\quad\textrm{and}\quad h=i.

Conversely, let Θμ,h\Theta_{\mu,h} be a Schrödinger L-system of the form (18) with the symmetric operator A˙{\dot{A}} such that

VΘμ,h(z)=mα(z),V_{\Theta_{\mu,h}}(z)=-m_{\alpha}(z),

for all z±z\in{\mathbb{C}}_{\pm} and μ{}\mu\in\mathbb{R}\cup\{\infty\}. Then the parameters μ\mu and hh defining Θμ,h\Theta_{\mu,h} are given by (26), i.e., μ=tanα\mu=\tan\alpha and h=ih=i.

We note that when α=π\alpha=\pi we obtain μα=0\mu_{\alpha}=0, mπ(z)=m(z)m_{\pi}(z)=m_{\infty}(z), and the realizing Schrödinger L-system Θ0,i\Theta_{0,i} is thoroughly described in [7, Section 5]. If α=π/2\alpha=\pi/2, then we get μα=\mu_{\alpha}=\infty, mα(z)=1/m(z)-m_{\alpha}(z)=1/m_{\infty}(z), and the realizing Schrödinger L-system is Θ,i\Theta_{\infty,i} (see [7, Section 5]). Assuming that α(0,π]\alpha\in(0,\pi] and neither α=π\alpha=\pi nor α=π/2\alpha=\pi/2 we give the description of a Schrödinger L-system Θμα,i\Theta_{\mu_{\alpha},i} realizing mα(z)-m_{\alpha}(z) as follows.

(27) Θtanα,i=(𝔸tanα,iKtanα,i1+L2[,+)),\Theta_{\tan\alpha,i}=\begin{pmatrix}{\mathbb{A}}_{\tan\alpha,i}&K_{\tan\alpha,i}&1\cr{\mathcal{H}}_{+}\subset L_{2}[\ell,+\infty)\subset{\mathcal{H}}_{-}&&{\mathbb{C}}\cr\end{pmatrix},

where

(28) 𝔸tanα,iy=l(y)1tanαi[y()iy()][(tanα)δ(x)+δ(x)],𝔸tanα,iy=l(y)1tanα+i[y()+iy()][(tanα)δ(x)+δ(x)],\begin{split}&{\mathbb{A}}_{\tan\alpha,i}\,y=l(y)-\frac{1}{\tan\alpha-i}[y^{\prime}(\ell)-iy(\ell)][(\tan\alpha)\delta(x-\ell)+\delta^{\prime}(x-\ell)],\\ &{\mathbb{A}}^{*}_{\tan\alpha,i}\,y=l(y)-\frac{1}{\tan\alpha+i}\,[y^{\prime}(\ell)+iy(\ell)][(\tan\alpha)\delta(x-\ell)+\delta^{\prime}(x-\ell)],\end{split}

Ktanα,ic=cgtanα,iK_{\tan\alpha,i}\,{c}=c\,g_{\tan\alpha,i}, (c)(c\in{\mathbb{C}}) and

(29) gtanα,i=(tanα)δ(x)+δ(x).g_{\tan\alpha,i}=(\tan\alpha)\delta(x-\ell)+\delta^{\prime}(x-\ell).

Also,

(30) VΘtanα,i(z)\displaystyle V_{\Theta_{\tan\alpha,i}}(z) =mα(z)\displaystyle=-m_{\alpha}(z)
WΘtanα,i(z)\displaystyle W_{\Theta_{\tan\alpha,i}}(z) =tanαitanα+im(z)im(z)+i=(e2αi)m(z)im(z)+i.\displaystyle=\frac{\tan\alpha-i}{\tan\alpha+i}\cdot\frac{m_{\infty}(z)-i}{m_{\infty}(z)+i}=(-e^{2\alpha i})\,\frac{m_{\infty}(z)-i}{m_{\infty}(z)+i}.

The realization theorem for Herglotz-Nevanlinna functions 1/mα(z)1/m_{\alpha}(z) is similar to Theorem 3 and can be found in [7].

6. Non-negative Schrödinger operator and sectorial L-systems

Now let us assume that A˙{\dot{A}} is a non-negative (i.e., (A˙f,f)0({\dot{A}}f,f)\geq 0 for all fDom(A˙)f\in\text{\rm{Dom}}({\dot{A}})) symmetric operator of the form (12) with deficiency indices (1,1), generated by the differential operation l(y)=y′′+q(x)yl(y)=-y^{\prime\prime}+q(x)y. The following theorem takes place.

Theorem 5 ([23], [24], [25]).

Let A˙{\dot{A}} be a nonnegative symmetric Schrödinger operator of the form (12) with deficiency indices (1,1)(1,1) and locally summable potential in =L2[,).{\mathcal{H}}=L^{2}[\ell,\infty). Consider operator ThT_{h} of the form (13). Then

  1. (1)

    operator A˙{\dot{A}} has more than one non-negative self-adjoint extension, i.e., the Friedrichs extension AFA_{F} and the Kreĭn-von Neumann extension AKA_{K} do not coincide, if and only if m(0)<m_{\infty}(-0)<\infty;

  2. (2)

    operator ThT_{h}, (h=h¯h=\bar{h}) coincides with the Kreĭn-von Neumann extension AKA_{K} if and only if h=m(0)h=-m_{\infty}(-0);

  3. (3)

    operator ThT_{h} is accretive if and only if

    (31) Rehm(0);{\rm Re\,}h\geq-m_{\infty}(-0);
  4. (4)

    operator ThT_{h}, (hh¯h\neq\bar{h}) is β\beta-sectorial if and only if Reh>m(0){\rm Re\,}h>-m_{\infty}(-0) holds;

  5. (5)

    operator ThT_{h}, (hh¯h\neq\bar{h}) is accretive but not β\beta-sectorial for any β(0,π2)\beta\in(0,\frac{\pi}{2}) if and only if Reh=m(0){\rm Re\,}h=-m_{\infty}(-0)

  6. (6)

    If Th,(Imh>0)T_{h},(\operatorname{Im}h>0) is β\beta-sectorial, then the exact angle β\beta can be calculated via

    (32) tanβ=ImhReh+m(0).\tan\beta=\frac{\operatorname{Im}h}{{\rm Re\,}h+m_{\infty}(-0)}.

For the remainder of this paper we assume that m(0)<m_{\infty}(-0)<\infty. Then according to Theorem 5 above (see also [3], [22], [25]) we have the existence of the operator ThT_{h}, (Imh>0\operatorname{Im}h>0) that is accretive and/or sectorial. It was shown in [2] that if Th(Imh>0)T_{h}\;(\operatorname{Im}h>0) is an accretive Schrödinger operator of the form (13), then for all real μ\mu satisfying the following inequality

(33) μ(Imh)2m(0)+Reh+Reh,\mu\geq\frac{(\operatorname{Im}h)^{2}}{m_{\infty}(-0)+{\rm Re\,}h}+{\rm Re\,}h,

formulas (14) define the set of all accretive ()(*)-extensions 𝔸μ,h{\mathbb{A}}_{\mu,h} of the operator ThT_{h}. Moreover, an accretive ()(*)-extensions 𝔸μ,h{\mathbb{A}}_{\mu,h} of a sectorial operator ThT_{h} with exact angle of sectoriality β(0,π/2)\beta\in(0,\pi/2) also preserves the same exact angle of sectoriality if and only if μ=+\mu=+\infty in (14) (see [8, Theorem 3]). Also, 𝔸μ,h{\mathbb{A}}_{\mu,h} is accretive but not β\beta-sectorial for any β(0,π/2)\beta\in(0,\pi/2) (*)-extension of ThT_{h} if and only if in (14)

(34) μ=(Imh)2m(0)+Reh+Reh,\mu=\frac{(\operatorname{Im}h)^{2}}{m_{\infty}(-0)+{\rm Re\,}h}+{\rm Re\,}h,

(see [8, Theorem 4]). An accretive operator ThT_{h} has a unique accretive ()(*)-extension 𝔸,h{\mathbb{A}}_{\infty,h} if and only if Reh=m(0).{\rm Re\,}h=-m_{\infty}(-0). In this case this unique ()(*)-extension has the form

(35) 𝔸,hy=y′′+q(x)y+[hy()y()]δ(x),\displaystyle{\mathbb{A}}_{\infty,h}y=-y^{\prime\prime}+q(x)y+[hy(\ell)-y^{\prime}(\ell)]\,\delta(x-\ell),
𝔸,hy=y′′+q(x)y+[h¯y()y()]δ(x).\displaystyle{\mathbb{A}}^{*}_{\infty,h}y=-y^{\prime\prime}+q(x)y+[\overline{h}y(\ell)-y^{\prime}(\ell)]\,\delta(x-\ell).

Now we are going to turn to functions mα(z)m_{\alpha}(z) described by (23)-(24) and associated with the non-negative operator A˙{\dot{A}} above. We need to see how the parameter α\alpha in the definition of mα(z)m_{\alpha}(z) affects the L-system realizing (mα(z))(-m_{\alpha}(z)). This question was answered in [7, Theorem 6.3]. It tells us that if the non-negative symmetric Schrödinger operator is such that m(0)0m_{\infty}(-0)\geq 0, then the L-system Θtanα,i\Theta_{\tan\alpha,i} of the form (27) realizing the function (mα(z))(-m_{\alpha}(z)) is accretive if and only if

(36) tanα1m(0).\tan\alpha\geq\frac{1}{m_{\infty}(-0)}.

Note that if m(0)=0m_{\infty}(-0)=0 in (36), then α=π/2\alpha=\pi/2 and mπ2(z)=1/m(z)-m_{\frac{\pi}{2}}(z)={1}/{m_{\infty}(z)}. Also, from [7, Theorem 6.2] we know that if m(0)0m_{\infty}(-0)\geq 0, then 1/m(z){1}/{m_{\infty}(z)} is realized by an accretive system Θ,i\Theta_{\infty,i}.

Now once we established a criteria for an L-system realizing (mα(z))(-m_{\alpha}(z)) to be accretive, we can look into more of its properties. There are two choices for an accretive L-system Θtanα,i\Theta_{\tan\alpha,i}: it is either (1) accretive sectorial or (2) accretive extremal. In the case (1) we have that 𝔸tanα,i{\mathbb{A}}_{\tan\alpha,i} of the form (28) is β1\beta_{1}-sectorial with some angle of sectoriality β1\beta_{1} that can only exceed the exact angle of sectoriality β\beta of TiT_{i}. In the case (2) the state-space operator 𝔸tanα,i{\mathbb{A}}_{\tan\alpha,i} is extremal (not sectorial for any β(0,π/2)\beta\in(0,\pi/2)) and is a ()(*)-extension of TiT_{i} that itself can be either β\beta-sectorial or extremal. These possibilities were described in details in [7, Theorem 6.4]. In particular, it was shown that for the accretive L-system Θtanα,i\Theta_{\tan\alpha,i} realizing the function (mα(z))(-m_{\alpha}(z)) the following is true:

  1. (1)

    if m(0)=0m_{\infty}(-0)=0, then there is only one accretive L-system Θ,i\Theta_{\infty,i} realizing (mα(z))(-m_{\alpha}(z)). This L-system is extremal and its main operator TiT_{i} is extremal as well.

  2. (2)

    if m(0)>0m_{\infty}(-0)>0, then TiT_{i} is β\beta-sectorial for β(0,π/2)\beta\in(0,\pi/2) and

    1. (a)

      if tanα=1/m(0)\tan\alpha={1}/{m_{\infty}(-0)}, then Θtanα,i\Theta_{\tan\alpha,i} is extremal;

    2. (b)

      if 1m(0)<tanα<+\frac{1}{m_{\infty}(-0)}<\tan\alpha<+\infty, then Θtanα,i\Theta_{\tan\alpha,i} is β1\beta_{1}-sectorial with β1>β\beta_{1}>\beta;

    3. (c)

      if tanα=+\tan\alpha=+\infty, then Θ,i\Theta_{\infty,i} is β\beta-sectorial.

Refer to caption
Figure 1. Accretive L-systems Θμ,i\Theta_{\mu,i}

Figure 1 above describes the dependence of the properties of realizing (mα(z))(-m_{\alpha}(z)) L-systems on the value of μ\mu and hence α\alpha. The bold part of the real line depicts values of μ=tanα\mu=\tan\alpha that produce accretive L-systems Θμ,i\Theta_{\mu,i}.

Additional analytic properties of the functions (m(z))(-m_{\infty}(z)), 1/m(z)1/m_{\infty}(z), and (mα(z))(-m_{\alpha}(z)) were described in [7, Theorem 6.5]. It was proved there that under the current set of assumptions we have:

  1. (1)

    the function 1/m(z)1/m_{\infty}(z) is Stieltjes if and only if m(0)0m_{\infty}(-0)\geq 0;

  2. (2)

    the function (m(z))(-m_{\infty}(z)) is never Stieltjes;111It will be shown in an upcoming paper that if m(0)0m_{\infty}(-0)\geq 0, then the function (m(z))(-m_{\infty}(z)) is actually inverse Stieltjes.

  3. (3)

    the function (mα(z))(-m_{\alpha}(z)) given by (24) is Stieltjes if and only if

    0<1m(0)tanα.0<\frac{1}{m_{\infty}(-0)}\leq\tan\alpha.

Now we are going to turn to the case when our realizing L-system Θtanα,i\Theta_{\tan\alpha,i} is accretive sectorial. To begin with let Θ\Theta be an L-system of the form (18), where 𝔸{\mathbb{A}} is a (*)-extension (14) of the accretive Schrödinger operator ThT_{h}. Here we summarize and list some known facts about possible accretivity and sectoriality of Θ\Theta.

  • The operator 𝔸μ,h{\mathbb{A}}_{\mu,h} of Θμ,h\Theta_{\mu,h} is accretive if and only if (33) holds (see [2]).

  • According to Theorem 2 if an accretive operator ThT_{h}, (Imh>0\operatorname{Im}h>0) is β\beta-sectorial, then (32) holds. Conversely, if hh, (Imh>0\operatorname{Im}h>0) is such that Reh>m(0),{\rm Re\,}h>-m_{\infty}(-0), then operator ThT_{h} of the form (13) is β\beta-sectorial and β\beta is determined by (32).

  • ThT_{h} is accretive but not β\beta-sectorial for any β(0,π/2)\beta\in(0,\pi/2) if and only if Reh=m(0){\rm Re\,}h=-m_{\infty}(-0).

  • If Θμ,h\Theta_{\mu,h} is such that μ=+\mu=+\infty, then VΘ,h(z)V_{\Theta_{\infty,h}}(z) belongs to the class S0,βS^{0,\beta}. In the case when μ+\mu\neq+\infty we have VΘμ,h(z)Sβ1,β2V_{\Theta_{\mu,h}}(z)\in S^{\beta_{1},\beta_{2}} (see [5]).

  • The operator 𝔸μ,h{\mathbb{A}}_{\mu,h} is a β\beta-sectorial (*)-extension of ThT_{h} (with the same angle of sectoriality) if and only if μ=+\mu=+\infty in (14) (see [2], [8]).

  • If ThT_{h} is β\beta-sectorial with the exact angle of sectoriality β\beta, then it admits only one β\beta-sectorial (*)-extension 𝔸μ,h{\mathbb{A}}_{\mu,h} with the same angle of sectoriality β\beta. Consequently, μ=+\mu=+\infty and 𝔸μ,h=𝔸,h{\mathbb{A}}_{\mu,h}={\mathbb{A}}_{\infty,h} has the form (35).

  • A (*)-extension 𝔸μ,h{\mathbb{A}}_{\mu,h} of ThT_{h} is accretive but not β\beta-sectorial for any β(0,π/2)\beta\in(0,\pi/2) if and only if the value of μ\mu in (14) is given by (34).

Note that it follows from the above that any β\beta-sectorial operator ThT_{h} with the exact angle of sectoriality β(0,π/2)\beta\in(0,\pi/2) admits only one accretive (*)-extension 𝔸μ,h{\mathbb{A}}_{\mu,h} that is not β\beta-sectorial for any β(0,π/2)\beta\in(0,\pi/2). This extension takes form (14) with μ\mu given by (34).

Now let us consider a function (mα(z))(-m_{\alpha}(z)) and Schrödinger L-system Θtanα,i\Theta_{\tan\alpha,i} of the form (27) that realizes it. According to [7, Theorem 6.4-6.5] this L-system Θtanα,i\Theta_{\tan\alpha,i} is sectorial if and only if

(37) tanα>1m(0).\tan\alpha>\frac{1}{m_{\infty}(-0)}.

If we assume that L-system Θtanα,i\Theta_{\tan\alpha,i} is β\beta-sectorial, then its impedance function VΘtanα,i(z)=mα(z)V_{\Theta_{\tan\alpha,i}}(z)=-m_{\alpha}(z) belongs to certain sectorial classes discussed in Section 3. Namely, (mα(z))Sβ(-m_{\alpha}(z))\in S^{\beta}. The following theorem provides more refined properties of (mα(z))(-m_{\alpha}(z)) for this case.

Theorem 6.

Let Θtanα,i\Theta_{\tan\alpha,i} be the accretive L-system of the form (27) realizing the function (mα(z))(-m_{\alpha}(z)) associated with the non-negative operator A˙{\dot{A}}. Let also 𝔸tanα,i{\mathbb{A}}_{\tan\alpha,i} be a β\beta-sectorial ()(*)-extension of TiT_{i} defined by (22). Then the function (mα(z))(-m_{\alpha}(z)) belongs to the class Sβ1,β2S^{\beta_{1},\beta_{2}}, tanβ2tanβ\tan\beta_{2}\leq\tan\beta,

(38) tanβ1=cotα,\tan\beta_{1}=\cot\alpha,

and

(39) tanβ2=tanα+m(0)(tanα)m(0)1.\tan\beta_{2}=\frac{\tan\alpha+m_{\infty}(-0)}{(\tan\alpha)m_{\infty}(-0)-1}.

Moreover, the operator TiT_{i} is (β2β1)(\beta_{2}-\beta_{1})-sectorial with the exact angle of sectoriality (β2β1)(\beta_{2}-\beta_{1}).

Proof.

It is given that Θtanα,i\Theta_{\tan\alpha,i} is β\beta-sectorial and hence (37) holds. For further convenience we re-write (mα(z))(-m_{\alpha}(z)) as

(40) mα(z)=sinα+m(z)cosαcosα+m(z)sinα=tanα+m(z)(tanα)m(z)1.-m_{\alpha}(z)=\frac{\sin\alpha+m_{\infty}(z)\cos\alpha}{-\cos\alpha+m_{\infty}(z)\sin\alpha}=\frac{\tan\alpha+m_{\infty}(z)}{(\tan\alpha)m_{\infty}(z)-1}.

Since under our assumption Θtanα,i\Theta_{\tan\alpha,i} is β\beta-sectorial, then its impedance function VΘtanα,i(z)=mα(z)V_{\Theta_{\tan\alpha,i}}(z)=-m_{\alpha}(z) belongs to certain sectorial classes discussed in Section 3. Namely, mα(z)Sβ-m_{\alpha}(z)\in S^{\beta} and mα(z)Sβ1,β2-m_{\alpha}(z)\in S^{\beta_{1},\beta_{2}}. In order to describe β1\beta_{1} we take into account (see [2, Section 10.3]) that limxm(x)=+\lim_{x\to-\infty}m_{\infty}(x)=+\infty to obtain

tanβ1\displaystyle\tan\beta_{1} =limx(mα(x))=tanα+m()(tanα)m()1=tanαm()+1tanα1m()\displaystyle=\lim_{x\to-\infty}(-m_{\alpha}(x))=\frac{\tan\alpha+m_{\infty}(-\infty)}{(\tan\alpha)m_{\infty}(-\infty)-1}=\frac{\frac{\tan\alpha}{m_{\infty}(-\infty)}+1}{\tan\alpha-\frac{1}{m_{\infty}(-\infty)}}
=1tanα=cotα.\displaystyle=\frac{1}{\tan\alpha}=\cot\alpha.

In order to get β2\beta_{2} we simply pass to the limit in (40)

tanβ2=limx0(mα(x))=tanα+m(0)(tanα)m(0)1.\tan\beta_{2}=\lim_{x\to-0}(-m_{\alpha}(x))=\frac{\tan\alpha+m_{\infty}(-0)}{(\tan\alpha)m_{\infty}(-0)-1}.

The above confirms (38) and (39). In order to show the rest, we apply [2, Theorem 9.8.4]. This theorem states that if 𝔸{\mathbb{A}} is a β\beta-sectorial ()(*)-extension of a main operator TT of an L-system Θ\Theta, then the impedance function VΘ(z)V_{\Theta}(z) belongs to the class Sβ1,β2S^{\beta_{1},\beta_{2}}, tanβ2tanβ\tan\beta_{2}\leq\tan\beta, and TT is (β2β1)(\beta_{2}-\beta_{1})-sectorial with the exact angle of sectoriality (β2β1)(\beta_{2}-\beta_{1}). It can also be checked directly that formulas (38) and (39) (under condition (37)) imply 0<β2β1<π/20<\beta_{2}-\beta_{1}<\pi/2 and hence the definition of (β2β1)(\beta_{2}-\beta_{1})-sectoriality applies correctly. ∎

Refer to caption
Figure 2. Angle of sectoriality β\beta. Here α0=arctan(1m(0))\alpha_{0}=\arctan\big{(}\frac{1}{m_{\infty}(-0)}\big{)}.

Now we state and prove the following.

Theorem 7.

Let Θtanα,i\Theta_{\tan\alpha,i} be an accretive L-system of the form (27) that realizes (mα(z))(-m_{\alpha}(z)), where 𝔸tanα,i{\mathbb{A}}_{\tan\alpha,i} is a (*)-extension of a θ\theta-sectorial operator TiT_{i} with exact angle of sectoriality θ\theta. Let also α(arctan(1m(0)),π2)\alpha_{*}\in\left(\arctan\big{(}\frac{1}{m_{\infty}(-0)}\big{)},\frac{\pi}{2}\right) be a fixed value that defines 𝔸tanα,i{\mathbb{A}}_{\tan\alpha_{*},i} via (14), and (mα(z))Sβ1,β2(-m_{\alpha}(z))\in S^{\beta_{1},\beta_{2}}. Then a (*)-extension 𝔸tanα,i{\mathbb{A}}_{\tan\alpha,i} of TiT_{i} is β\beta-sectorial for any α[α,π/2)\alpha\in[\alpha_{*},\pi/2) with

(41) tanβ=tanβ1+2tanβ1tanβ2,tanβ>tanθ.{\tan\beta=\tan\beta_{1}+2\sqrt{\tan\beta_{1}\,\tan\beta_{2}}},\quad\tan\beta>\tan\theta.

Moreover, if α=π/2\alpha=\pi/2, then

β=β2β1=θ=arctan(1m(0)).\beta=\beta_{2}-\beta_{1}=\theta=\arctan\left(\frac{1}{m_{\infty}(-0)}\right).
Proof.

We note first that the conditions of our theorem imply the following tanα(1m(0),+)\tan\alpha_{*}\in\left(\frac{1}{m_{\infty}(-0)},+\infty\right). Thus, according to [7, Theorem 6.4] part 2(c), a (*)-extension 𝔸tanα,i{\mathbb{A}}_{\tan\alpha,i} is β\beta-sectorial for some β(0,π/2)\beta\in(0,\pi/2). Then we can apply Theorem 6 to confirm that (mα(z))Sβ1,β2(-m_{\alpha}(z))\in S^{\beta_{1},\beta_{2}}, where β1\beta_{1} and β2\beta_{2} are described by (38) and (39). The first part of formula (41) follows from [8, Theorem 8] applied to the L-system Θtanα,i\Theta_{\tan\alpha,i} with μ=tanα\mu=\tan\alpha (see also [2, Theorem 9.8.7]). Note that since 𝔸tanα,i{\mathbb{A}}_{\tan\alpha,i} is a β\beta-sectorial extension of a θ\theta-sectorial operator TiT_{i}, then tanβtanθ\tan\beta\geq\tan\theta with equality possible only when μ=tanα=\mu=\tan\alpha=\infty (see [2], [8]). Since we chose α[α,π/2)\alpha\in[\alpha_{*},\pi/2), then tanα\tan\alpha\neq\infty and hence tanβ>tanθ\tan\beta>\tan\theta that confirms the second part of formula (41).

If we assume that α=π/2\alpha=\pi/2, then our function (mα(z))=1/m(z)(-m_{\alpha}(z))=1/m_{\infty}(z) is realized with Θ,i\Theta_{\infty,i} (see Theorem 3) that preserves the angle of sectoriality of its main operator TiT_{i} (see [7, Theorem 6.4] and Figure 1). Therefore, β=θ\beta=\theta. If we combine this fact with (mα(z))Sβ1,β2(-m_{\alpha}(z))\in S^{\beta_{1},\beta_{2}} and apply Theorem 6 we get that β=β2β1\beta=\beta_{2}-\beta_{1}. Finally, since TiT_{i} is θ\theta-sectorial, formula (32) yields tanθ=1m(0)\tan\theta=\frac{1}{m_{\infty}(-0)}. ∎

Note that Theorem 7 provides us with a value β\beta which serves as a universal angle of sectoriality for the entire indexed family of ()(*)-extensions 𝔸tanα,i{\mathbb{A}}_{\tan\alpha,i} of the form (27) as depicted on Figure 2. It is clearly shown on the figure that if α=π/2\alpha=\pi/2, then tanβ=tanθ\tan\beta=\tan\theta.

7. Example

We conclude this paper with a simple illustration. Consider the differential expression with the Bessel potential

lν=d2dx2+ν21/4x2,x[1,)l_{\nu}=-\frac{d^{2}}{dx^{2}}+\frac{\nu^{2}-1/4}{x^{2}},\;\;x\in[1,\infty)

of order ν>0\nu>0 in the Hilbert space =L2[1,){\mathcal{H}}=L^{2}[1,\infty). The minimal symmetric operator

(42) {A˙y=y′′+ν21/4x2yy(1)=y(1)=0\left\{\begin{array}[]{l}{\dot{A}}\,y=-y^{\prime\prime}+\frac{\nu^{2}-1/4}{x^{2}}y\\ y(1)=y^{\prime}(1)=0\\ \end{array}\right.

generated by this expression and boundary conditions has defect numbers (1,1)(1,1). Let ν=3/2\nu=3/2. It is known [2] that in this case

m(z)=iz32z32iz+i12=ziz+iz+i=1izz+im_{\infty}(z)=-\frac{iz-\frac{3}{2}\sqrt{z}-\frac{3}{2}i}{\sqrt{z}+i}-\frac{1}{2}=\frac{\sqrt{z}-iz+i}{\sqrt{z}+i}=1-\frac{iz}{\sqrt{z}+i}

and m(0)=1.m_{\infty}(-0)=1. The minimal symmetric operator then becomes

(43) {A˙y=y′′+2x2yy(1)=y(1)=0.\left\{\begin{array}[]{l}{\dot{A}}\,y=-y^{\prime\prime}+\frac{2}{x^{2}}y\\ y(1)=y^{\prime}(1)=0.\\ \end{array}\right.

The main operator ThT_{h} of the form (13) is written for h=ih=i as

(44) {Tiy=y′′+2x2yy(1)=iy(1)\left\{\begin{array}[]{l}T_{i}\,y=-y^{\prime\prime}+\frac{2}{x^{2}}y\\ y^{\prime}(1)=i\,y(1)\\ \end{array}\right.

will be shared by all the family of L-systems realizing functions (mα(z))(-m_{\alpha}(z)) described by (23)-(24). This operator is accretive and β\beta-sectorial since Reh=0>m(0)=1{\rm Re\,}h=0>-m_{\infty}(-0)=-1 with the exact angle of sectoriality given by (see (32))

(45) tanβ=ImhReh+m(0)=10+1=1 orβ=π4.\tan\beta=\frac{\operatorname{Im}h}{{\rm Re\,}h+m_{\infty}(-0)}=\frac{1}{0+1}=1\quad\textrm{ or}\quad\beta=\frac{\pi}{4}.

A family of L-systems Θtanα,i\Theta_{\tan\alpha,i} of the form (27) that realizes functions (mα(z))(-m_{\alpha}(z)) described by (23)–(25) as

(46) mα(z)=(ziz+i)cosα+(z+i)sinα(ziz+i)sinα(z+i)cosα,-m_{\alpha}(z)=\frac{({\sqrt{z}-iz+i})\cos\alpha+({\sqrt{z}+i})\sin\alpha}{({\sqrt{z}-iz+i})\sin\alpha-({\sqrt{z}+i})\cos\alpha},

was constructed in [7]. According to [7, Theorem 6.3] the L-systems Θtanα,i\Theta_{\tan\alpha,i} in (27) are accretive if

1=1m(0)tanα<+.1=\frac{1}{m_{\infty}(-0)}\leq\tan\alpha<+\infty.

Using part (2c) of [7, Theorem 6.4], we get that the realizing L-system Θtanα,i\Theta_{\tan\alpha,i} in (27) preserves the angle of sectoriality and becomes π4\frac{\pi}{4}-sectorial if μ=tanα=+\mu=\tan\alpha=+\infty or α=π/2\alpha=\pi/2. Therefore the L-system

(47) Θ,i=(𝔸,iK,i1+L2[1,+)),\Theta_{\infty,i}=\begin{pmatrix}{\mathbb{A}}_{\infty,i}&K_{\infty,i}&1\cr{\mathcal{H}}_{+}\subset L_{2}[1,+\infty)\subset{\mathcal{H}}_{-}&&{\mathbb{C}}\cr\end{pmatrix},

where

(48) 𝔸,iy=y′′+2x2y[y(1)iy(1)]δ(x1),𝔸,iy=y′′+2x2y[y(1)+iy(1)]δ(x1),\begin{split}&{\mathbb{A}}_{\infty,i}\,y=-y^{\prime\prime}+\frac{2}{x^{2}}y-\,[y^{\prime}(1)-iy(1)]\,\delta(x-1),\\ &{\mathbb{A}}^{*}_{\infty,i}\,y=-y^{\prime\prime}+\frac{2}{x^{2}}y-\,[y^{\prime}(1)+iy(1)]\,\delta(x-1),\end{split}

K,ic=cg,iK_{\infty,i}{c}=cg_{\infty,i}, (c)(c\in{\mathbb{C}}) and g,i=δ(x1),g_{\infty,i}=\delta(x-1), realizes the function mπ2(z)=1/m(z)-m_{\frac{\pi}{2}}(z)=1/m_{\infty}(z). Also,

(49) VΘ,i(z)\displaystyle V_{\Theta_{\infty,i}}(z) =mπ2(z)=1m(z)=z+iziz+i\displaystyle=-m_{\frac{\pi}{2}}(z)=\frac{1}{m_{\infty}(z)}=\frac{\sqrt{z}+i}{\sqrt{z}-iz+i}
WΘ,i(z)\displaystyle W_{\Theta_{\infty,i}}(z) =(eπi)m(z)im(z)+i=(1i)ziz+1+i(1+i)ziz1+i.\displaystyle=(-e^{{\pi}i})\,\frac{m_{\infty}(z)-i}{m_{\infty}(z)+i}=\frac{(1-i)\sqrt{z}-iz+1+i}{(1+i)\sqrt{z}-iz-1+i}.

This L-system Θ,i\Theta_{\infty,i} is clearly accretive according to [7, Theorem 6.2] which is also independently confirmed by direct evaluation

(Re𝔸,iy,y)=y(x)L22+2y(x)/xL220.({\rm Re\,}{\mathbb{A}}_{\infty,i}\,y,y)=\|y^{\prime}(x)\|^{2}_{L^{2}}+2\|y(x)/x\|^{2}_{L^{2}}\geq 0.

Moreover, according to [7, Theorem 6.4] (see also [2, Theorem 9.8.7]) the L-system Θ,i\Theta_{\infty,i} is π4\frac{\pi}{4}-sectorial. Taking into account that (Im𝔸,iy,y)=|y(1)|2,(\operatorname{Im}{\mathbb{A}}_{\infty,i}\,y,y)=|y(1)|^{2}, (see formula (15)) we obtain inequality (2) with β=π4\beta=\frac{\pi}{4}, that is (Re𝔸,iy,y)|(Im𝔸,iy,y)|,({\rm Re\,}{\mathbb{A}}_{\infty,i}\,y,y)\geq|(\operatorname{Im}{\mathbb{A}}_{\infty,i}\,y,y)|, or

(50) y(x)L22+2y(x)/xL22|y(1)|2.\|y^{\prime}(x)\|^{2}_{L^{2}}+2\|y(x)/x\|^{2}_{L^{2}}\geq|y(1)|^{2}.

In addition, we have shown that the β\beta-sectorial form (Tiy,y)(T_{i}y,y) defined on Dom(Ti)\text{\rm{Dom}}(T_{i}) can be extended to the β\beta-sectorial form (𝔸,iy,y)({\mathbb{A}}_{\infty,i}\,y,y) defined on +=Dom(A˙){\mathcal{H}}_{+}=\text{\rm{Dom}}({\dot{A}}^{*}) (see (43)–(44)) having the exact (for both forms) angle of sectoriality β=π/4\beta=\pi/4. A general problem of extending sectorial sesquilinear forms to sectorial ones was mentioned by T. Kato in [17]. It can be easily seen that function mπ2(z)-m_{\frac{\pi}{2}}(z) in (49) belongs to a sectorial class S0,π4S^{0,\frac{\pi}{4}} of Stieltjes functions.

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