1 Introduction

Let T be a bounded linear operator on a complex Hilbert space H,write it for TB(H), take a complex number λ in ℂ, and,henceforth, shorten TλI to Tλ. One of recent trends in operator theory is studying naturalextensions of normal operators. We introduce some of these operators as follows.

T is said to be a hyponormal operator if T TT T ;

T is M-hyponormal [1] if there exists a real positive number M such that

M 2 ( T λ ) (Tλ)(Tλ) ( T λ ) for all λC;

T is quasi-M-hyponormal [2] if there exits a real positive number M such that

T ( M 2 ( T λ ) ( T λ ) ) T T (Tλ) ( T λ ) Tfor all λC;

T is k-quasi-M-hyponormal [3] if there exists a real positive number M such that

T k ( M 2 ( T λ ) ( T λ ) ) T k T k (Tλ) ( T λ ) T k for all λC,

where k is a natural number.

It is clear that hyponormalM-hyponormalk-quasi-M-hyponormal.

We give the following example to indicate that there exists an M-hyponormaloperator, which is not hyponormal.

Example 1.1 Consider the unilateral weighted shift operator as aninfinite-dimensional Hilbert space operator. Recall that given a bounded sequence ofpositive numbers α: α 1 , α 2 , α 3 , (called weights), the unilateral weighted shift W α associated with α is the operator on H= l 2 defined by W α e n := α n e n + 1 for all n1, where { e n } n = 1 is the canonical orthogonal basis for l 2 . It is well known that W α is hyponormal if and only if α is monotonicallyincreasing. Also, W α is M-hyponormal if and only if α iseventually increasing. Hence, if we take the weights α such that α 1 =2, α 2 =1, α 3 =2, α 3 = α 4 = , then W α is an M-hyponormal operator, but it is nothyponormal.

Next, we give a 2-quasi-M-hyponormal operator, which is notM-hyponormal.

Example 1.2 Let T= ( 0 1 0 0 ) defined on C 2 . Then by simple calculations, we see that T is a2-quasi-M-hyponormal operator, but is not M-hyponormal.

If TB(H), we shall write N(T) and R(T) for the null space and the range space of T. Also, let α(T):=dimN(T), β(T):=dimN( T ), σ(T) and isoσ(T) for the spectrum and the isolated points of the spectrum ofT, respectively.

Let λisoσ(T). The Riesz idempotent E of T with respect toλ is defined by E= 1 2 π i D ( μ T ) 1 dμ, where D is a closed disk, centered at λ,which contains no other points of σ(T). It is well known that the Riesz idempotent satisfies E 2 =E, ET=TE, σ(T | R ( E ) )={λ}, and N(Tλ)R(E). Stampfli [4] showed that if T satisfies the growth condition G 1 , then E is self-adjoint and R(E)=N(Tλ). Recently, Chō and Tanahashi [5] obtained an improvement of Stampfli’s result top-hyponormal operators or log-hyponormal operators. Furthermore, Chōand Han extended it to M-hyponormal operators as follows.

Proposition 1.3 [[6], Theorem 4]

Let T be an M-hyponormal operator, and let λ be an isolated point ofσ(T). If E is the Riesz idempotent for λ, then E is self-adjoint, andR(E)=N(Tλ)=N ( T λ ) .

2 Isolated point of spectrum of k-quasi-M-hyponormaloperators

Lemma 2.1 Let T be a k-quasi-M-hyponormal operator. If0λC, and assume thatσ(T)={λ}, thenT=λI.

Proof If λ0 and σ(T)={λ}, then T is invertible, so T is anM-hyponormal operator, and hence, T=λI by [6]. □

Lemma 2.2 Let T be a k-quasi-M-hyponormal operator and0λC. ThenTx=λximplies that T x= λ ¯ x.

Proof Suppose that Tx=λx. Since T is a k-quasi-M-hyponormaloperator, M(Tα) T k y ( T α ) T k y for all vectors yH and αC. In particular, M(Tλ) T k x ( T λ ) T k x. Since Tx=λx, 0=M | λ | k (Tλ)x=M(Tλ) T k x ( T λ ) T k x= | λ | k ( T λ ) x. |λ|0, therefore ( T λ ) x=0. □

Theorem 2.3 Let T be a k-quasi-M-hyponormal operator, and let λ be a non-zero isolated point ofσ(T). Then the Riesz idempotent E for λ is self-adjoint, and

R(E)=N(Tλ)=N ( T λ ) .

Proof We can derive the result from Lemma 2.2, [[3], Theorem 2.5] and [[7], Lemma 5.2]. □

3 Weyl-type theorems of algebraically k-quasi-M-hyponormaloperators

We say that T is an algebraically k-quasi-M-hyponormaloperator if there exists a nonconstant complex polynomial p such that p(T) is a k-quasi-M-hyponormal operator. From thedefinition above, T is an algebraicallyk-quasi-M-hyponormal operator, then so is Tλ for each λC.

An operator T is called Fredholm if R(T) is closed, and both N(T) and N( T ) are finite-dimensional. The index of a Fredholm operatorT is given by i(T)=α(T)β(T). An operator T is called Weyl if it is Fredholm of indexzero. The Weyl spectrum of T[8] is defined by w(T):={λC:Tλ is not Weyl}. Following [9], we say that Weyl’s theorem holds for T if σ(T)w(T)= π 00 (T), where π 00 (T):={λisoσ(T):0<α(Tλ)<}.

More generally, Berkani investigated the B-Fredholm theory (see [1012]). We define TSB F + (H) if there exists a positive integer n such that R( T n ) is closed, T [ n ] :R( T n )xTxR( T n ) is upper semi-Fredholm (i.e., R( T [ n ] )=R( T n + 1 ) is closed, dimN( T [ n ] )=dimN(T)R( T n )<) and i( T [ n ] )0[12]. We define σ S B F + (T)={λC:TλSB F + (H)}. Let E a (T) denote the set of all isolated points λ of σ a (T) with 0<α(Tλ). We say that generalized a-Weyl’s theorem holds forT if σ a (T) σ S B F + (T)= E a (T).

We know that Weyl’s theorem holds for hermitian operators [13], which have been extended to hyponormal operators [14], algebraically hyponormal operators by [15], algebraically M-hyponormal operators [6] and algebraically quasi-M-hyponormal operators [2], respectively. In this section, we obtain that generalizeda-Weyl’s theorems hold for algebraicallyk-quasi-M-hyponormal operators.

Lemma 3.1[3]

LetTB(H)be a k-quasi-M-hyponormal operator, let the rangeof T k be not dense and

T=( T 1 T 2 0 T 3 )onH= R ( T k ) ¯ N ( T k ) .

Then T 1 is M-hyponormal, T 3 k =0andσ(T)=σ( T 1 ){0}.

Theorem 3.2 Let T be a quasinilpotent algebraically k-quasi-M-hyponormal operator. Then T is nilpotent.

Proof We first assume that T is ak-quasi-M-hyponormal operator. Consider two cases, Case I: If therange of T k has dense range, then it is an M-hyponormal operator.Hence, by [[6], Lemma 8], T is nilpotent. Case II: If T does nothave dense range, then by Lemma 3.1, we can represent T as the uppertriangular matrix

T=( T 1 T 2 0 T 3 )onH= R ( T k ) ¯ N ( T k ) ,

where T 1 :=T| R ( T k ) ¯ is an M-hyponormal operator. Since T isquasinilpotent, σ(T)={0}. But σ(T)=σ( T 1 ){0}, hence, σ( T 1 )={0}. Since T 1 is an M-hyponormal operator, T 1 =0. Since T 3 k =0, simple computation shows that

T k + 1 =( 0 T 2 T 3 k 0 T 3 k + 1 )=0.

Now, suppose that T is an algebraicallyk-quasi-M-hyponormal operator. Then there exists a nonconstantpolynomial p such that p(T) is a k-quasi-M-hyponormal operator. If p(T) has dense range, then p(T) is an M-hyponormal operator. Thus T is analgebraically M-hyponormal operator. It follows from [[6], Lemma 8] that it is nilpotent. If ( p ( T ) ) k does not have a dense range, then by Lemma 3.1, we canrepresent p(T) as the upper triangular matrix

p(T)=( A B 0 C )onH= R ( ( p ( T ) ) k ) ¯ N ( ( p ( T ) ) k ) ,

where A:=p(T)| R ( ( p ( T ) ) k ) ¯ is an M-hyponormal operator. Since σ(T)={0} and σ(p(T))=p(σ(T))={p(0)}, the operator p(T)p(0) is quasinilpotent. But σ(p(T))=σ(A){0}, thus σ(A){0}={p(0)}. So p(0)=0, and hence, p(T) is quasinilpotent. Since p(T) is a k-quasi-M-hyponormal operator, by theprevious argument p(T) is nilpotent. On the other hand, since p(0)=0, p(z)=c z m (z λ 1 )(z λ 2 )(z λ n ) for some natural number m. p(T)=c T m (T λ 1 )(T λ 2 )(T λ n ). p(T) is nilpotent, therefore, T isnilpotent. □

Recall that an operator T is said to be isoloid if every isolated point of σ(T) is an eigenvalue of T and polaroid if every isolatedpoint of σ(T) is a pole of the resolvent of T. In general, ifT is polaroid, then it is isoloid. However, the converse is not true.In [6], it is showed that every algebraically M-hyponormal operator isisoloid, we can prove more.

Theorem 3.3 Let T be an algebraically k-quasi-M-hyponormal operator. Then T is polaroid.

Proof Suppose that T is an algebraicallyk-quasi-M-hyponormal operator. Then p(T) is a k-quasi-M-hyponormal operator for somenonconstant polynomial p. Let λisoσ(T) and E λ be the Riesz idempotent associated to λ defined by E λ := 1 2 π i D ( μ T ) 1 dμ, where D is a closed disk of center λ,which contains no other point of σ(T). We can represent T as the direct sum in the followingform:

T=( T 1 0 0 T 2 ),

where σ( T 1 )={λ} and σ( T 2 )=σ(T){λ}. Since T 1 is an algebraically k-quasi-M-hyponormaloperator, so is T 1 λ. But σ( T 1 λ)={0}, it follows from Theorem 3.2 that T 1 λ is nilpotent, thus T 1 λ has finite ascent and descent. On the other hand, since T 2 λ is invertible, clearly, it has finite ascent and descent. Tλ has finite ascent and descent, and hence, λ is apole of the resolvent of T, therefore, T ispolaroid. □

Corollary 3.4 Let T be an algebraically k-quasi-M-hyponormal operator. Then T is isoloid.

We say that T has the single valued extension property (abbreviated SVEP)if, for every open set U of ℂ, the only analytic solution f: UH of the equation

(Tλ)f(λ)=0for all λU

is a zero function on U.

Theorem 3.5 Let T be an algebraically k-quasi-M-hyponormal operator. Then T has SVEP.

Proof Suppose that T is an algebraicallyk-quasi-M-hyponormal operator. Then p(T) is a k-quasi-M-hyponormal operator for somenonconstant complex polynomial p, and hence, p(T) has SVEP by [[3], Theorem 2.1]. Therefore, T has SVEP by [[16], Theorem 3.3.9]. □

In the following theorem, H(σ(T)) denotes the space of functions analytic in an open neighborhood of σ(T).

Theorem 3.6 Let T or T be an algebraically k-quasi-M-hyponormal operator. ThenWeyl’s theorem holds forf(T)for everyfH(σ(T)).

Proof Firstly, suppose that T is an algebraicallyk-quasi-M-hyponormal operator. We first show that Weyl’stheorem holds for T. Using the fact [[17], Theorem 2.2] that if T is polaroid, then Weyl’stheorem holds for T if and only if T has SVEP at points of λσ(T)w(T). We have that T is polaroid by Theorem 3.3, andT has SVEP by Theorem 3.5. Hence, T satisfiesWeyl’s theorem.

Next, suppose that T is an algebraically k-quasi-M-hyponormaloperator. Now we show that Weyl’s theorem holds for T. We use thefact [[18], Theorem 3.1] that if T or T has SVEP, then Weyl’s theorem holds for T if andonly if π 00 (T)= p 00 (T). Since T has SVEP, it is sufficient to show that π 00 (T)= p 00 (T). p 00 (T) π 00 (T) is clear, so we only need to prove π 00 (T) p 00 (T). Let λ π 00 (T). Then λ is an isolated point of σ(T). Hence, λ is a pole of the resolvent of T,since T is polaroid by Theorem 3.3, that is, p(λT)=q(λT)<. By assumption, we have α(λT)<, so β(λT)<. Hence, we conclude that λ p 00 (T). Therefore, Weyl’s theorem holds for T.

Finally, we can derive the result by Theorem 3.5 and [[17], Theorem 2.4]. □

Following [[19], Theorem 3.12], we obtain the following result.

Theorem 3.7 Let f be an analytic function onσ(T), and f is not constant on each connected component of the open set U containingσ(T).

  1. (i)

    If T is an algebraically k-quasi-M-hyponormal operator, then f(T) satisfies a generalized a-Weyl’s theorem.

  2. (ii)

    If T is an algebraically k-quasi-M-hyponormal operator, then f( T ) satisfies a generalized a-Weyl’s theorem.