Quasi-Fredholm spectrum and compact perturbations
Anuradha Gupta and Ankit Kumar∗
Abstract
In this paper we explore some characteristics of the quasi-Fredholm resolvent set ρqf(T) of an operator T defined on an infinite dimensional Banach space X. Moreover, in the case of Hilbert space H, we study the stability of the SVEP and describe the operators for which the SVEP is preserved under compact perturbations using quasi-Fredholm spectrum and ρqf(T).
Mathematics Subject Classification: 47A10, 47A55, 47B15.
Keywords: Quasi-Fredholm spectrum, topological uniform descent, SVEP, compact perturbation.
Introduction and Preliminaries
Throughout this paper, denote by B(X) the Banach algebra of all bounded linear operators defined on an infinite dimensional complex Banach space X. For A⊂C, \mboxisoA, \mboxintA, A and \mboxaccA denote the set of isolated points of A, interior points of A, closure of A and accumulation points of A, respectively. For λ∈C and r>0, B(λ,r) denotes the open disc of radius r centred at λ. For T∈B(X), the null space of T, range of T, spectrum of T and adjoint of T are denoted by N(T), T(X), σ(T) and T∗, respectively.
Let α(T)= dim N(T) and β(T)= codim T(X) be the nullity of T and deficiency of T, respectively. An operator T∈B(X) is called bounded below if T is injective and T(X) is closed. A bounded linear operator T is said to be an upper semi-Fredholm operator if α(T)<∞ and T(X) is closed. An operator T∈B(X) is said to be a lower semi-Fredholm operator if β(T)<∞. An operator T∈B(X) is called a semi-Fredholm operator if it is either upper semi-Fredholm or lower semi-Fredholm. For a semi-Fredholm operator T, the index of T is defined by \mboxind(T):=α(T)−β(T).
The point spectrum, approximate point spectrum and semi-Fredholm spectrum are defined by
[TABLE]
Clearly, σsf(T)⊂σa(T). Let ρa(T)=C∖σa(T) and ρsf(T)=C∖σsf(T). An operator T∈B(X) is called said to be an upper semi-Weyl (lower semi-Weyl, respectively) operator if it is upper semi-Fredholm (lower semi-Fredholm, respectively) and
\mboxind(T)≤0 (\mboxind(T)≥0, respectively). A bounded linear operator T is called Weyl if it is semi-Fredholm and \mboxind(T)=0. The Weyl essential approximate point spectrum and Weyl spectrum are defined by
[TABLE]
Let ρuw(T)=C∖σuw(T) and ρw(T)=C∖σbw(T).
Let T∈B(X), then for each non negative integer n, T induces a linear transformation
[TABLE]
defined by
[TABLE]
Clearly, Ψn is surjective for each n. For each n, let kn(T)=α(Ψn). Define a norm ∥.∥n on Tn(X) by
[TABLE]
The topology induced by this norm is called operator range topology on Tn(X).
An operator T∈B(X) is said to have uniform descent for n≥d if there exists a non negative integer d such that kn(T)=0 for n≥d. In addition, if Tn(X) is closed in the operator range topology of Td(X) for n≥d, then T is said to have topological uniform descent for n≥d. The topological uniform descent spectrum is defined by
[TABLE]
Let ρΓ(T)=C∖σΓ(T) be the topological uniform descent resolvent of T.
For T∈B(X) consider the set
[TABLE]
The degree of stable iteration is defined by \mboxdis(T):=infΔ(T) whenever Δ(T)=∅. If Δ(T)=∅, set \mboxdis(T)=∞.
Let T∈B(X). An operator T∈B(X) is said to be quasi-Fredholm of degree d if there exists a d∈N such that
(i) \mboxdis(T)=d,
(ii) Tn(X) is a closed subspace of X for each n≥d,
(iii) T(X)+N(Td) is a closed subspace of X.
For T∈B(X), the quasi-Fredholm spectrum is defined by
[TABLE]
Let ρqf(T)=C∖σqf(T) be the quasi-Fredholm resolvent of T. By [2, Theorem 1.96] we know that σΓ(T)⊂σqf(T)⊂σsf(T).
For a bounded linear operator T and a non negative integer n, denote by T[n] the restriction of T to Tn(X). An opeartor T∈B(X) is said to be B-Fredholm (an upper semi B-Fredholm, a lower semi B-Fredholm, respectively) if for some non negative integer n, Tn(X) is closed and T[n] is Fredholm (an upper semi B-Fredholm, a lower semi B-Fredholm, respectively). In this case, the \mboxind(T) is defined to be the \mboxindT[n] (see [4]). An operator is said to be a semi B-Fredholm operator if is a lower semi B-Fredholm or an upper semi B-Fredholm operator. The * semi B-Fredholm spectrum* is defined by
[TABLE]
Clearly, σsbf(T)⊂σsf(T). Let ρsbf(T)=C∖σsbf(T). By [2, Theorem 1.116] we know that every semi B-Fredholm operator is quasi-Fredholm. Therefore, σΓ(T)⊂σqf(T)⊂σsbf(T)⊂σsf(T).
An operator T∈B(X) is called an upper semi B-Weyl (B-Weyl, respectively) operator if T is an upper semi B-Fredholm (B-Fredholm, respectively) having \mboxind(T)≤0 (\mboxind(T)=0, respectively). The upper semi B-Weyl spectrum and B-Weyl spectrum are defined by
[TABLE]
Let ρbw(T)=C∖σbw(T) and ρw(T)=C∖σw(T). For an operator T∈B(X), the ascent of T denoted by p(T) is the smallest non negative integer p such that N(Tp)=N(Tp+1). If no such integer exists, set p(T)=∞. For an operator T∈B(X), the descent of T denoted by q(T) is the smallest non negative integer q such that Tq(X)=Tq+1(X). If no such integer exists, set q(T)=∞. Evidently, p(T)=0 if and only if T is injective and q(T)=0 if and only if T is surjective. By [2, Theorem 1.20] we know that if both p(T) and q(T) are finite, then p(T)= q(T). An operator T∈B(X) is called left Drazin invertible if p(T)<∞ and Tp+1(X) is closed. We say that λ∈\mboxisoσa(T) is a left pole of the resolvent of T if λI−T is left Drazin invertible. An operator T∈B(X) is called right Drazin invertible if q(T)<∞ and Tq(X) is closed. An operator T∈B(X) is called Drazin invertible if p(T)=q(T)<∞. We say that λ∈\mboxisoσ(T) is a pole of the resolvent of T if λI−T is Drazin invertible. The left Drazin spectrum and Drazin spectrum are defined by
[TABLE]
By [2, Theorem 1.142] we know that σqf(T)⊂σld(T)⊂σd(T). The set of all the poles of the resolvent of T and all left poles of the resolvent of T are denoted by Π(T)=σ(T)∖σd(T) and Πa(T)=σa(T)∖σld(T), respectively.
An operator T∈B(X) is said to have the single-valued extension property (SVEP) at λ0∈C, if for every neighborhood V of λ0 the only analytic function f:V→X which satisfies the equation (λI−T)f(λ)=0 is the function f=0. An operator T∈B(X) is said to have SVEP if T has SVEP at every λ∈C. It is known that if \mboxintσp(T)=∅, then T has SVEP. Recall that
[TABLE]
and
[TABLE]
Zeng et al. [9] studied the components of quasi-Fredholm resolvent and characterized them by means of localized SVEP. Shi [8] considered the topological uniform descent and studied how topological uniform descent resolvent is distributed in ρsf(T). As we know that for an operator T∈B(X), topological uniform descent, quasi-Fredholmness, semi-Fredholmness and semi B-Fredholness are closely related to each other. Motivated by them we study the distribution of ρqf(T) in ρsbf(T). Zhu and Li [10] obtained results for non commuting compact perturbations of an operator T∈B(X) using semi-Fredholm spectrum. Recently, for T∈B(X) various authors (see [3, 6, 7]) discussed various spectral properties under compact (not necessarily commuting) perturbations. Motivated by them we obtain results for compact perturbations of an operator T∈B(X) using quasi-Fredholm spectrum.
In this paper we discuss some characteristics of quasi-Fredholm resolvent set ρqf(T) for T∈B(X). We give results regarding the distribution of semi B-Fredholm domain ρsbf(T) in ρqf(T). We prove that if \mboxintσsbf(T)=∅, then there is one-to-one correspondence between the bounded components of ρsbf(T) and the bounded components of ρqf(T). In the last section we discuss the permanence of SVEP under(small) compact perturbations using quasi-Fredholm resolvent set and quasi-Fredholm spectrum. Also, we describe those operators for which SVEP is stable under compact perturbations by means of quasi-Fredholm resolvent.
Main Results
It is known that the sets ρsf(T),ρsbf(T),ρqf(T) and ρsf(T) are nonempty open sets of C, they can be decomposed into (pairwise disjoint, maximal, open, connected) non-empty components.
Lemma 2.1**.**
Let T∈B(X). Then σsf(T)=σsbf(T)∪\mboxisoσsf(T).
Proof.
Let λ0∈σsf(T)∖σsbf(T). Then λ0I−T is semi B-Fredholm. By [2, Theorem 1.117] there exists an ϵ>0 such that λI−T is semi-Fredholm for all λ∈B(λ0,ϵ)∖{λ0}. Therefore, λ0∈\mboxisoσsf(T). Thus, σsf(T)⊂σsbf(T)∪\mboxisoσsf(T). The reverse inclusion always holds.
∎
Recall that a hole of a compact set σ⊂C is a bounded component of C∖σ. It is known that C∖σ has always an unbounded component. Therefore, C∖σ is connected if and only if σ has no holes.
Theorem 2.2**.**
Let T∈B(X), then ρsbf(T) is connected if and only if ρsf(T) is connected.
Proof.
Suppose that ρsbf(T) is connected. Since σsf(T)=σsbf(T)∪\mboxisoσsf(T), ρsf(T)=ρsbf(T)∖\mboxisoσsf(T). As ρsbf(T) is connected and \mboxisoσsf(T) is at most countable we deduce that ρsf(T) is connected.
Conversely, suppose that ρsf(T) is connected. Assume that ρsbf(T) is not connected then there exists a bounded component Ω of ρsbf(T). Then either Ω∩ρsf(T)=∅ or Ω∩ρsf(T)=∅. If Ω ∩ ρsf(T)=∅, then Ω⊂σsf(T) which implies that Ω⊂\mboxisoσsf(T) which is not possible. Therefore, Ω∩ρsf(T)=∅. Then there exists λ0 such that λ0∈Ω∩ρsf(T). Let Ω′ be the component of ρsf(T) containing λ0. Therefore, Ω′ is an open connected subset of ρsbf(T) such that Ω∩Ω′=∅. This implies that Ω′⊂Ω. Thus, Ω′ is a bounded component of ρsf(T), a contradiction. Hence, ρsbf(T) is connected.
∎
By [5, Lemma 2.2] we have σuw(T)=σusbw(T)∪\mboxisoσuw(T) and σw(T)=σbw(T)∪\mboxisoσw(T). Following the lines of the proof of Theorem 2.2 we have the following result:
Theorem 2.3**.**
Let T∈B(X), then
(i) ρbw(T) is connected if and only if ρw(T) is connected.
(ii) ρusbw(T) is connected if and only if ρuw(T) is connected.
Theorem 2.4**.**
Let T∈B(X) and Ωqf be a connected component of ρqf(T). If Ωqf∩ρsbf(T)=∅, then there exists a unique connected component Ωsbf of ρsbf(T) such that Ωqf=Ωsbf∪E, where E0⊂\mboxisoσsf(T).
Proof.
As Ωqf is a connected component of ρqf(T) and ρqf(T)⊂ρΓ(T), there exists a component ΩΓ of ρΓ(T) such that Ωqf⊂ΩΓ. Since Ωqf∩ρsbf(T)=∅ and ρsbf(T)⊂ρqf(T), proceeding as in the proof of Theorem 2.2 there exists a component Ωsbf of ρsbf(T) such that Ωsbf⊂Ωqf. By the proof of Theorem 2.2 we get a component Ωsf of ρsf such that Ωsf⊂Ωsbf⊂Ωqf⊂ΩΓ. Using [8, Theorem 1] we have ΩΓ=Ωsf∪E, where E⊂\mboxisoσsf(T). This gives Ωsbf⊂Ωqf⊂Ωsf∪E⊂Ωsbf∪E. Therefore, there exists E0⊂E⊂\mboxisoσsf(T) such that Ωqf=Ωsbf∪E0.
Assume that there exist connected components Ωsbf and Ωsbf′ of ρsbf(T) such that Ωqf=Ωsbf∪E and Ωqf=Ωsbf′∪F, where E,F⊂\mboxisoσsf(T). Then Ωsbf∪E=Ωsbf′∪F which implies that Ωsbf⊂F, a contradiction.
∎
Corollary 2.5**.**
Let T∈B(X) and Ωsbf be a connected component of ρsbf(T). Then there exists a unique connected component Ωqf of ρqf(T) such that Ωqf=Ωsbf∪E, where E⊂\mboxisoσsf(T).
Proof.
Since Ωsbf⊂ρsbf(T)⊂ρqf(T), there exists a connected component Ωqf of ρqf(T) such that Ωsbf⊂Ωqf. By Theorem 2.4 we get Ωqf=Ωsbf∪E0, where E0⊂\mboxisoσsf(T). Assume that there exists another connected component Ωqf′ of ρqf(T) such that Ωqf′=Ωsbf∪F, where F⊂\mboxisoσsf(T). This gives Ωsbf⊂Ωqf∩Ωqf′, a contradiction.
∎
Corollary 2.6**.**
Let T∈B(X) and \mboxintσsbf(T)=∅. Then ρqf(T)∖ρsbf(T) is at most countable and σsbf(T)=σqf(T)∪\mboxisoσsbf(T).
Proof.
Let {Ωqfn}n=1∞ be an enumeration of connected components of ρqf(T). Since \mboxintσsbf(T)=∅, for every connected component Ωqfn of ρqf(T) we have Ωqfn∩ρsbf(T)=∅. Using Theorem 2.4 for Ωqfn, there exists a unique connected component Ωsbfn of ρsbf(T) such that Ωqfn=Ωsbfn∪En, where En⊂\mboxisoσsf(T). Let E=n=1⋃∞En, then E is at most countable and E⊂\mboxisoσsf(T). Also,
[TABLE]
Since ρsbf(T)⊂ρqf(T), ρqf(T)=ρsbf(T)∪E. Let E′=E∩σsbf(T). Then E′⊂\mboxisoσsbf(T) and ρqf(T)=ρsbf(T)∪E′. This gives σsbf(T)=σqf(T)∪E′ which implies that σsbf(T)=σqf(T)∪\mboxisoσsbf(T).
∎
Let W1, W2, W3 and W4 be the set of all bounded components of ρsbf(T), ρqf(T),ρsf(T) and ρΓ(T), respectively.
Theorem 2.7**.**
Let T∈B(X). Then there exists an injective mapping f:W1→W2. Moreover, if \mboxintσsbf(T)=∅, then f is also surjective.
Proof.
Suppose that Ω∈W1. Using Corollary 2.5 we get a unique connected component Ω′ of ρqf(T) such that Ω′=Ω∪E, where E⊂\mboxisoσsf(T). Since \mboxisoσsf(T)⊂σsf(T), Ω′ is bounded component of ρqf(T) which implies that Ω′∈W2. Define f:W1→W2 by f(Ω)=Ω′. Then f is a well defined mapping. We prove that f is an injective mapping. Let Ω1 and Ω2 be two distinct elements of W1 such that f(Ω1)=f(Ω2). This implies that there exists a component Ω′ of ρqf(T) such that Ω′=Ω1∪E=Ω2∪F, where E,F⊂\mboxisoσsf(T). As Ω1∩Ω2=∅, Ω1⊂F, a contradiction. Therefore, f is an injective mapping.
Suppose that τ∈W2. Since \mboxintσsbf(T)=∅, τ∩ρsbf(T)=∅. Using Theorem 2.4 there exists a unique component τ′ of ρsbf(T) such that τ=τ′∪E, where E⊂\mboxisoσsf(T). Therefore, f(τ′)=τ.
∎
Similarly, using [8, Theorem 1, Corollary 1] we establish the following result:
Theorem 2.8**.**
Let T∈B(X). Then there exists an injective mapping g:W3→W4. Moreover, if \mboxintσsf(T)=∅, then g is also surjective.
Theorem 2.9**.**
Let T∈B(X). Then every non isolated boundary point of σsbf(T) belongs to σqf(T).
Proof.
Let λ be a non isolated boundary point of σsbf(T). Let λ∈ρqf(T) and Ωqf be the component of ρqf(T) containing λ. Then there exists ϵ>0 such that B(λ,ϵ)⊂Ωqf. Since λ is the boundary point of σsbf(T), B(λ,ϵ)∩ρsbf(T)=∅ which implies that Ωqf∩ρsbf(T)=∅. Therefore, by Theorem 2.4 there exists a component Ωsbf of ρsbf(T) such that Ωqf=Ωsbf∪E, where E⊂\mboxisoσsf(T). Since λ∈Ωqf∩\mboxaccσsbf(T)⊂Ωqf∩\mboxaccσsf(T) we deduce that λ∈Ωsbf, a contradiction. Therefore, λ∈σqf(T).
∎
Remark 2.10**.**
It is observed that if P is a closed subset of C such that \mboxintP=∅ and \mboxintPc=∅, then (∂P)c is disconnected.**
Lemma 2.11**.**
Let T∈B(X), ρqf(T) be connected and \mboxintσqf(T)=∅. Suppose that P is a closed set contained in σ(T). Then \mboxintP=∅.
Proof.
Suppose that \mboxintP=∅. First we prove that ρqf(T)∩\mboxacc(∂P)=∅. If ρqf(T)∩\mboxacc(∂P)=∅, then
[TABLE]
Since ρqf(T) is connected, \mboxiso(∂P)∪(∂P)c is connected. Let S=\mboxiso(∂P)∪(∂P)c. This implies that (∂P)c=S∖\mboxiso(∂P) which gives (∂P)c is connected. As \mboxintP=∅ then by Remark 2.10 we get a contradiction. Therefore, there exists λ such that λ∈ρqf(T)∩\mboxacc(∂P). As ρqf(T) is connected and ρ(T)⊂ρqf(T), by [9, Theorems 3.6, 3.7] p(λI−T)=q(λI−T)<∞ for all λ∈ρqf(T). Therefore, (λI−T) is drazin invertible for all λ∈ρqf(T). This gives ρqf(T)=ρ(T)∪Π(T), where Π(T) denotes the set of poles of the resolvent of T. Since λ∈\mboxacc(∂P)⊂σ(T) which implies that λ∈Π(T)⊂\mboxisoσ(T). Then there exists an ϵ>0 such that B(λ,ϵ)∖{λ}⊂ρ(T). Since λ∈\mboxacc(∂P), there exists μ∈B(λ,ϵ)∩∂P⊂ρ(T)∩∂P, a contradiction. Hence, \mboxintP=∅.
∎
If ρΓ(T) is connected, then by [8, Proposition 2] we know that ρΓ(T)=ρ(T)∪Π(T). Then proceeding likewise as in Lemma 2.11 we have the following result:
Lemma 2.12**.**
Let T∈B(X), ρΓ(T) be connected and \mboxintσΓ(T)=∅. Suppose that P is closed set contained in σ(T). Then \mboxintP=∅.
Theorem 2.13**.**
Let T∈B(X). Then following statements are equivalent:
(i) ρsf(T) is connected and int σsf(T)=∅,
(ii) ρsbf(T) is connected and int σsbf(T)=∅,
(iii) ρqf(T) is connected and int σqf(T)=∅,
(iv) ρΓ(T) is connected and \mboxintσΓ(T)=∅.
Proof.
Since σΓ(T)⊂σqf(T)⊂σsbf(T)⊂σsf(T), (i)⇒(ii)⇒(iii)⇒(iv) is obvious.
Now suppose that ρΓ(T) is connected and int σΓ(T)=∅. Using Lemma 2.12 we deduce that \mboxintσsf(T)=∅. It remains to prove that ρsf(T) is connected. As ρΓ(T) is connected, by [8, Theorem 1] there exists a unique connected component Ωsf of ρsf(T) such that ρΓ(T)=Ωsf∪E0, where E0⊂\mboxisoσsf(T). This gives ρΓ(T)=ρsf(T)∪E0. This implies that rhosf(T)=ρΓ(T)∖E0. Therefore, ρsf(T) is connected.
∎
Lemma 2.14**.**
Let T∈B(X). Then if ρsf(T) consists of finite bounded components, then ρsbf(T) consists of finite bounded components.
Proof.
Suppose that Ω1 and Ω2 are two distinct bounded components of ρsbf(T). Then by the proof of Theorem 2.2 we get bounded components Ω1′, Ω2′ of ρsf(T) such that Ω1′⊂Ω1 and Ω2′⊂Ω2. This gives Ω1′∩Ω2′=∅ since if Ω1′=Ω2′, then Ω1∩Ω2=∅ which is a contradiction.
∎
Remark 2.15**.**
If \mboxintσqf(T)=∅ and Ω is bounded component of ρΓ(T), then Ω∩ρqf(T)=∅. Therefore, there exists a component Ω′ of ρqf(T) such that Ω′⊂Ω. From this we can conclude that for any two bounded distinct components of ρΓ(T) we get two distinct component of ρqf(T). Hence, if ρqf(T) consists of finite bounded components, then ρΓ(T) consists of bounded components.**
Theorem 2.16**.**
Let T∈B(H) and intσp(T)=∅. Then following statements are equivalent:
(i) \mboxintσsf(T)=∅ and ρsf(T) consists of finite bounded components,
(ii) \mboxintσsbf(T)=∅ and ρsbf(T) consists of finite bounded components,
(iii) \mboxintσqf(T)=∅ and ρqf(T) consists of finite bounded components,
(iv) \mboxintσΓ(T)=∅ and ρΓ(T) consists of finite bounded components.
Proof.
(i) ⇒(ii) Follows directly from Lemma 2.14.
(ii) ⇒(iii) Follows from Theorem 2.7.
(iii) ⇒(iv) Follows from Remark 2.15.
(iv) ⇒(i) From Theorem 2.8 it follows that ρsf(T) consists of finite bounded components. Also, if \mboxintσp(T)=∅, then T has SVEP. Therefore, by [8, Proposition] we have \mboxintσsf(T)=∅.
∎
Quasi-Fredholm spectrum and compact perturbations
Let K(X) denote the ideal of all compact operators acting on a Banach space X. It is known that for T∈B(X) and K∈K(X),
[TABLE]
where σ∗=σsf or σuw or σw. We start the following section with the following theorem:
Theorem 3.1**.**
Let T∈B(X) and ρqf(T) be connected. Suppose that K∈K(X). Then
[TABLE]
Proof.
Since ρqf(T) is connected, ρqf(T)=ρ(T)∪Π(T) which implies that ρqf(T)=ρsbf(T). Therefore, ρsbf(T) is connected. Using Theorem 2.2 we get ρsf(T) is connected. As ρsf(T)=ρsf(T+K), ρsf(T+K) is connected. Again using Theorem 2.2 ρsbf(T+K) is connected.
By Corollary 2.5 there exists a component Ωqf of ρqf(T+K) such that
[TABLE]
where E⊂\mboxisoσsf(T+K). Let E0=E∩σsbf(T+K). Then Ωqf=ρsbf(T+K)∪E0 and E0⊂\mboxisoσsbf(T+K). As ρ(T+K)⊂ρsbf(T+K)⊂Ω, by [9, Theorems 3.6, 3.7] we get Ω=ρ(T+K)∪Π(T+K). Now
[TABLE]
As ρqf(T+K)∩Ωc=σsbf(T+K)∖σqf(T+K),
[TABLE]
which gives σ(T+K)=σqf(T+K)∪Π(T+K)∪(σsbf(T+K)∖σqf(T+K)).
∎
Denote
[TABLE]
and
[TABLE]
Lemma 3.2**.**
Let T∈B(X). Then ρsbf+(T)=∅ if and only if ρsf+(T)=∅.
Proof.
Evidently, if ρsbf+(T)=∅, then ρsf+(T)=∅. Conversely, suppose that ρsf+(T)=∅. Without loss of generality, we may assume that 0∈ρsbf+(T) then 0∈ρsbf(T) and \mboxind(T)>0. Now by [2, Theorem 1.117] there exists an ϵ>0 such that B(0,ϵ)∖{0}⊂ρsf(T) and \mboxind(λI−T)>0 for all λ∈B(0,ϵ), a contradiction.
∎
The following result is an immediate consequence of Lemma 3.2 and [10, Theorem 1.1]
Theorem 3.3**.**
Let T∈B(H), where H is a Hilbert space. Then the following statements are equivalent:
(i) There exists K∈K(H) such that T+K has SVEP,
(ii) ρsbf+(T)=∅,
(iii) ρsf+(T)=∅.
It is observed that if T has SVEP at every point of ρqf(T) then ρqf(T) need not be connected. The following example illustrates this fact:
Example 3.4**.**
Let R be unilateral shift on l2(N). It is known that σa(T)=S1, where S1 denotes the unit circle. Therefore, ∂σa(T)∩\mboxaccσa(T)=S1. By [11, Corollary 3.6] we have σqf(T)=σusbb(T)=S1. Hence, T has SVEP at every point of ρqf(T) but ρqf(T) is not connected.**
Theorem 3.5**.**
Let T∈B(H), where H is a Hilbert space. Then T+K has SVEP at every point of ρqf(T+K) for any K∈K(H) if and only if ρqf(T+K) is connected for any K∈K(H).
Proof.
Suppose that T+K has SVEP at every point of ρqf(T+K) for any K∈K(H). Let ρqf(T+K) is not connected for some K∈K(H). Then we can find a bounded connected component Ω of ρqf(T+K). Now ∂Ω⊂σqf(T+K)⊂σsf(T+K). Then the proof of [8, corollary 4] shows that there exist compact operators K1 and K2 such that
[TABLE]
where A is a normal operator and λI−(A+K2) is Weyl but not invertible operator for any λ∈Ω. Since T+K has SVEP at every point of ρqf(T+K), T+K has SVEP at Ω. Then by [9, Theorem 3.6] we have
[TABLE]
Therefore, Ω∩ρa(T+K)=∅ which implies that Ω∩ρsf(T+K)=∅. Let λ∈Ω∩ρsf(T+K) and Ω′ be a connected component of ρsf(T+K) contaning λ. Then Ω′⊂Ω. Since T+K+K1 has SVEP at every point of ρqf(T+K+K1), T+K+K1 has SVEP at every point of ρsf(T+K+K1). Using [1, Theorem 3.36] we have
[TABLE]
This gives Ω′∩ρa(T+K+K1)=∅. Therefore, there exists μ∈Ω′⊂Ω such that μI−(T+K+K1) is bounded below which implies that μI−(A+K2) is bounded below, a contradiction.
Conversely, suppose that ρqf(T+K) is connected for any K∈K(H). Then by [9, Theorem 3.6], we know that T+K has SVEP at every point of ρqf(T+K).
∎
The following result follows from [8, Proposition 6, Corollary 4] and Theorem 2.13.
Theorem 3.6**.**
Let T∈B(H), where H is a Hilbert space. Then following statements are equivalent:
(i) T+K has SVEP for any K∈K(H),
(ii) T∗+K has SVEP for any K∈K(H),
(iii) ρsf(T) is connected and \mboxintσsf(T)=∅,
(iv) ρsbf(T) is connected and \mboxintσsbf(T)=∅,
(v) ρqf(T) is connected and \mboxintσqf(T)=∅,
(vi) ρΓ(T) is connected and \mboxintσΓ(T)=∅,
(vii) ρsf(T+K) is connected and \mboxintσsf(T+K)=∅ for any K∈K(H),
(viii) ρsbf(T+K) is connected and \mboxintσsbf(T+K)=∅ for any K∈K(H),
(ix) ρqf(T+K) is connected and \mboxintσqf(T+K)=∅ for any K∈K(H),
(x) ρΓ(T+K) is connected and \mboxintσΓ(T+K)=∅.
The following result is consequence of [10, Theorem 1.2] and Theorem 2.16.
Theorem 3.7**.**
Let T∈B(H), where H is a Hilbert space. If
(i) \mboxintσp(T)=∅,
(ii) \mboxintσ∗(T)=∅,
*(iii) ρ∗(T) consists of finite bounded components,
where σ∗,ρ∗=σsf, ρsf or σsbf, ρsbf or σqf, ρqf or σΓ, ρΓ. Then there exists δ>0 such that T+K has SVEP for all K∈K(H) with ∥K∥<δ.*
Theorem 3.8**.**
Let T∈B(H), where H is Hilbert space. If σqf(T)=∅, then
[TABLE]
for any compact operator K∈K(X).
Proof.
Since σqf(T)=∅, ρqf(T)=C which implies that σ(T)=Π(T). As \mboxintσqf(T)=∅, by Theorem 2.16 ρqf(T+K) is connected. This gives ρqf(T+K)=ρsbf(T+K). Therefore, by Theorem 3.1 σ(T+K)=σqf(T+K)∪Π(T+K). As σ(T)=Π(T), σ(T) is finite which implies that σsf(T)=σsf(T+K) is finite. This gives
[TABLE]
Therefore, σ(T+K)=\mboxisoσsbf(T+K)∪Π(T+K).
∎
Acknowledgement The corresponding author (Ankit Kumar) is supported by Department of Science and Technology, New Delhi, India (Grant No. DST/INSPIRE Fellowship/[IF170390]).