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Spectrum (functional analysis)

From Wikipedia, the free encyclopedia
Set of eigenvalues of a matrix
For the prime spectrum of a ring, seeSpectrum of a ring.

Inmathematics, particularly infunctional analysis, thespectrum of abounded linear operator (or, more generally, anunbounded linear operator) is a generalisation of the set ofeigenvalues of amatrix. Specifically, acomplex numberλ{\displaystyle \lambda } is said to be in the spectrum of a bounded linear operatorT{\displaystyle T} ifTλI{\displaystyle T-\lambda I}

  • either hasno set-theoreticinverse;
  • or the set-theoretic inverse is either unbounded or defined on a non-dense subset.[1]

Here,I{\displaystyle I} is theidentity operator.

By theclosed graph theorem,λ{\displaystyle \lambda } is in the spectrum if and only if the bounded operatorTλI:VV{\displaystyle T-\lambda I:V\to V} is non-bijective onV{\displaystyle V}.

The study of spectra and related properties is known asspectral theory, which has numerous applications, most notably themathematical formulation of quantum mechanics.

The spectrum of an operator on afinite-dimensionalvector space is precisely the set of eigenvalues. However an operator on an infinite-dimensional space may have additional elements in its spectrum, and may have no eigenvalues. For example, consider theright shift operatorR on theHilbert space2,

(x1,x2,)(0,x1,x2,).{\displaystyle (x_{1},x_{2},\dots )\mapsto (0,x_{1},x_{2},\dots ).}

This has no eigenvalues, since ifRx=λx then by expanding this expression we see thatx1=0,x2=0, etc. On the other hand, 0 is in the spectrum because although the operatorR − 0 (i.e.R itself) is invertible, the inverse is defined on a set which is not dense in2. In factevery bounded linear operator on acomplexBanach space must have a non-empty spectrum.

The notion of spectrum extends tounbounded (i.e. not necessarily bounded) operators. Acomplex numberλ is said to be in the spectrum of an unbounded operatorT:XX{\displaystyle T:\,X\to X} defined on domainD(T)X{\displaystyle D(T)\subseteq X} if there is no bounded inverse(TλI)1:XD(T){\displaystyle (T-\lambda I)^{-1}:\,X\to D(T)} defined on the whole ofX.{\displaystyle X.} IfT isclosed (which includes the case whenT is bounded), boundedness of(TλI)1{\displaystyle (T-\lambda I)^{-1}} follows automatically from its existence.

The space of bounded linear operatorsB(X) on a Banach spaceX is an example of aunitalBanach algebra. Since the definition of the spectrum does not mention any properties ofB(X) except those that any such algebra has, the notion of a spectrum may be generalised to this context by using the same definition verbatim.

Spectrum of a bounded operator

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Definition

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LetT{\displaystyle T} be abounded linear operator acting on a Banach spaceX{\displaystyle X} over the complex scalar fieldC{\displaystyle \mathbb {C} }, andI{\displaystyle I} be theidentity operator onX{\displaystyle X}. Thespectrum ofT{\displaystyle T} is the set of allλC{\displaystyle \lambda \in \mathbb {C} } for which the operatorTλI{\displaystyle T-\lambda I} does not have an inverse that is a bounded linear operator.

SinceTλI{\displaystyle T-\lambda I} is a linear operator, the inverse is linear if it exists; and, by thebounded inverse theorem, it is bounded. Therefore, the spectrum consists precisely of those scalarsλ{\displaystyle \lambda } for whichTλI{\displaystyle T-\lambda I} is notbijective.

The spectrum of a given operatorT{\displaystyle T} is often denotedσ(T){\displaystyle \sigma (T)}, and its complement, theresolvent set, is denotedρ(T)=Cσ(T){\displaystyle \rho (T)=\mathbb {C} \setminus \sigma (T)}. (ρ(T){\displaystyle \rho (T)} is sometimes used to denote the spectral radius ofT{\displaystyle T})

Relation to eigenvalues

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Ifλ{\displaystyle \lambda } is an eigenvalue ofT{\displaystyle T}, then the operatorTλI{\displaystyle T-\lambda I} is not one-to-one, and therefore its inverse(TλI)1{\displaystyle (T-\lambda I)^{-1}} is not defined. However, the converse statement is not true: the operatorTλI{\displaystyle T-\lambda I} may not have an inverse, even ifλ{\displaystyle \lambda } is not an eigenvalue. Thus the spectrum of an operator always contains all its eigenvalues, but is not limited to them.

For example, consider the Hilbert space2(Z){\displaystyle \ell ^{2}(\mathbb {Z} )}, that consists of allbi-infinite sequences of real numbers

v=(,v2,v1,v0,v1,v2,){\displaystyle v=(\ldots ,v_{-2},v_{-1},v_{0},v_{1},v_{2},\ldots )}

that have a finite sum of squaresi=+vi2{\textstyle \sum _{i=-\infty }^{+\infty }v_{i}^{2}}. Thebilateral shift operatorT{\displaystyle T} simply displaces every element of the sequence by one position; namely ifu=T(v){\displaystyle u=T(v)} thenui=vi1{\displaystyle u_{i}=v_{i-1}} for every integeri{\displaystyle i}. The eigenvalue equationT(v)=λv{\displaystyle T(v)=\lambda v} has no nonzero solution in this space, since it implies that all the valuesvi{\displaystyle v_{i}} have the same absolute value (if|λ|=1{\displaystyle \vert \lambda \vert =1}) or are a geometric progression (if|λ|1{\displaystyle \vert \lambda \vert \neq 1}); either way, the sum of their squares would not be finite. However, the operatorTλI{\displaystyle T-\lambda I} is not invertible if|λ|=1{\displaystyle |\lambda |=1}. For example, the sequenceu{\displaystyle u} such thatui=1/(|i|+1){\displaystyle u_{i}=1/(|i|+1)} is in2(Z){\displaystyle \ell ^{2}(\mathbb {Z} )}; but there is no sequencev{\displaystyle v} in2(Z){\displaystyle \ell ^{2}(\mathbb {Z} )} such that(TI)v=u{\displaystyle (T-I)v=u} (that is,vi1=ui+vi{\displaystyle v_{i-1}=u_{i}+v_{i}} for alli{\displaystyle i}).

Basic properties

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The spectrum of a bounded operatorT{\displaystyle T} is always aclosed,bounded subset of thecomplex plane.

If the spectrum were empty, then theresolvent function

R(λ)=(TλI)1,λC,{\displaystyle R(\lambda )=(T-\lambda I)^{-1},\qquad \lambda \in \mathbb {C} ,}

would be defined everywhere on the complex plane and bounded. But it can be shown that the resolvent functionR{\displaystyle R} isholomorphic on its domain. By the vector-valued version ofLiouville's theorem, this function is constant, thus everywhere zero as it is zero at infinity. This would be a contradiction.

The boundedness of the spectrum follows from theNeumann series expansion inλ{\displaystyle \lambda }; the spectrumσ(T){\displaystyle \sigma (T)} is bounded byT{\displaystyle \left\|T\right\|}. A similar result shows the closedness of the spectrum.

The boundT{\displaystyle \left\|T\right\|} on the spectrum can be refined somewhat. Thespectral radius,r(T){\displaystyle r(T)}, ofT{\displaystyle T} is the radius of the smallest circle in the complex plane which is centered at the origin and contains the spectrumσ(T){\displaystyle \sigma (T)} inside of it, i.e.

r(T)=sup{|λ|:λσ(T)}.{\displaystyle r(T)=\sup\{|\lambda |:\lambda \in \sigma (T)\}.}

Thespectral radius formula says[2] that for any elementT{\displaystyle T} of aBanach algebra,

r(T)=limnTn1/n.{\displaystyle r(T)=\lim _{n\to \infty }\left\|T^{n}\right\|^{1/n}.}

Spectrum of an unbounded operator

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One can extend the definition of spectrum tounbounded operators on aBanach spaceX. These operators are no longer elements in the Banach algebraB(X).

Definition

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LetX be a Banach space andT:D(T)X{\displaystyle T:\,D(T)\to X} be alinear operator defined on domainD(T)X{\displaystyle D(T)\subseteq X}.A complex numberλ is said to be in theresolvent set (also calledregular set) ofT{\displaystyle T} if the operator

TλI:D(T)X{\displaystyle T-\lambda I:\,D(T)\to X}

has a bounded everywhere-defined inverse, i.e. if there exists a bounded operator

S:XD(T){\displaystyle S:\,X\rightarrow D(T)}

such that

S(TλI)=ID(T),(TλI)S=IX.{\displaystyle S(T-\lambda I)=I_{D(T)},\,(T-\lambda I)S=I_{X}.}

A complex numberλ is then in thespectrum ifλ is not in the resolvent set.

Forλ to be in the resolvent (i.e. not in the spectrum), just like in the bounded case,TλI{\displaystyle T-\lambda I} must be bijective, since it must have a two-sided inverse. As before, if an inverse exists, then its linearity is immediate, but in general it may not be bounded, so this condition must be checked separately.

By theclosed graph theorem, boundedness of(TλI)1{\displaystyle (T-\lambda I)^{-1}}does follow directly from its existence whenT isclosed. Then, just as in the bounded case, a complex numberλ lies in the spectrum of a closed operatorT if and only ifTλI{\displaystyle T-\lambda I} is not bijective. Note that the class of closed operators includes all bounded operators.

Basic properties

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The spectrum of an unbounded operator is in general a closed, possibly empty, subset of the complex plane.If the operatorT is notclosed, thenσ(T)=C{\displaystyle \sigma (T)=\mathbb {C} }.

The following example indicates that non-closed operators may have empty spectra. LetT{\displaystyle T} denote the differentiation operator onL2([0,1]){\displaystyle L^{2}([0,1])}, whose domain is defined to be the closure ofCc((0,1]){\displaystyle C_{c}^{\infty }((0,1])} with respect to theH1{\displaystyle H^{1}}-Sobolev space norm. This space can be characterized as all functions inH1([0,1]){\displaystyle H^{1}([0,1])} that are zero att=0{\displaystyle t=0}. Then,Tz{\displaystyle T-z} has trivial kernel on this domain, as anyH1([0,1]){\displaystyle H^{1}([0,1])}-function in its kernel is a constant multiple ofezt{\displaystyle e^{zt}}, which is zero att=0{\displaystyle t=0} if and only if it is identically zero. Therefore, the complement of the spectrum is all ofC.{\displaystyle \mathbb {C} .}

Classification of points in the spectrum

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Further information:Decomposition of spectrum (functional analysis)

A bounded operatorT on a Banach space is invertible, i.e. has a bounded inverse, if and only ifT is bounded below, i.e.Txcx,{\displaystyle \|Tx\|\geq c\|x\|,} for somec>0,{\displaystyle c>0,} and has dense range. Accordingly, the spectrum ofT can be divided into the following parts:

  1. λσ(T){\displaystyle \lambda \in \sigma (T)} ifTλI{\displaystyle T-\lambda I} is not bounded below. In particular, this is the case ifTλI{\displaystyle T-\lambda I} is not injective, that is,λ is an eigenvalue. The set of eigenvalues is called thepoint spectrum ofT and denoted byσp(T). Alternatively,TλI{\displaystyle T-\lambda I} could be one-to-one but still not bounded below. Suchλ is not an eigenvalue but still anapproximate eigenvalue ofT (eigenvalues themselves are also approximate eigenvalues). The set of approximate eigenvalues (which includes the point spectrum) is called theapproximate point spectrum ofT, denoted byσap(T).
  2. λσ(T){\displaystyle \lambda \in \sigma (T)} ifTλI{\displaystyle T-\lambda I} does not have dense range. The set of suchλ is called thecompression spectrum ofT, denoted byσcp(T){\displaystyle \sigma _{\mathrm {cp} }(T)}. IfTλI{\displaystyle T-\lambda I} does not have dense range but is injective,λ is said to be in theresidual spectrum ofT, denoted byσr(T){\displaystyle \sigma _{\mathrm {r} }(T)}.

Note that the approximate point spectrum and residual spectrum are not necessarily disjoint[3] (however, the point spectrum and the residual spectrum are).

The following subsections provide more details on the three parts ofσ(T) sketched above.

Point spectrum

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If an operator is not injective (so there is some nonzerox withT(x) = 0), then it is clearly not invertible. So ifλ is aneigenvalue ofT, one necessarily hasλ ∈ σ(T). The set of eigenvalues ofT is also called thepoint spectrum ofT, denoted byσp(T). Some authors refer to the closure of the point spectrum as thepure point spectrumσpp(T)=σp(T)¯{\displaystyle \sigma _{pp}(T)={\overline {\sigma _{p}(T)}}} while others simply considerσpp(T):=σp(T).{\displaystyle \sigma _{pp}(T):=\sigma _{p}(T).}[4][5]

Approximate point spectrum

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More generally, by thebounded inverse theorem,T is not invertible if it is not bounded below; that is, if there is noc > 0 such that ||Tx|| ≥ c||x|| for allxX. So the spectrum includes the set ofapproximate eigenvalues, which are thoseλ such thatT -λI is not bounded below; equivalently, it is the set ofλ for which there is a sequence of unit vectorsx1,x2, ... for which

limnTxnλxn=0{\displaystyle \lim _{n\to \infty }\|Tx_{n}-\lambda x_{n}\|=0}.

The set of approximate eigenvalues is known as theapproximate point spectrum, denoted byσap(T){\displaystyle \sigma _{\mathrm {ap} }(T)}.

It is easy to see that the eigenvalues lie in the approximate point spectrum.

For example, consider the bilateral shiftW onl2(Z){\displaystyle l^{2}(\mathbb {Z} )} defined by

W:ejej+1,jZ,{\displaystyle W:\,e_{j}\mapsto e_{j+1},\quad j\in \mathbb {Z} ,}

where(ej)jN{\displaystyle {\big (}e_{j}{\big )}_{j\in \mathbb {N} }} is the standard orthonormal basis inl2(Z){\displaystyle l^{2}(\mathbb {Z} )}. Direct calculation showsW has no eigenvalues, but everyλ with|λ|=1{\displaystyle |\lambda |=1} is an approximate eigenvalue; lettingxn be the vector

1n(,0,1,λ1,λ2,,λ1n,0,){\displaystyle {\frac {1}{\sqrt {n}}}(\dots ,0,1,\lambda ^{-1},\lambda ^{-2},\dots ,\lambda ^{1-n},0,\dots )}

one can see that ||xn|| = 1 for alln, but

Wxnλxn=2n0.{\displaystyle \|Wx_{n}-\lambda x_{n}\|={\sqrt {\frac {2}{n}}}\to 0.}

SinceW is a unitary operator, its spectrum lies on the unit circle. Therefore, the approximate point spectrum ofW is its entire spectrum.

This conclusion is also true for a more general class of operators.A unitary operator isnormal. By thespectral theorem, a bounded operator on a Hilbert space H is normal if and only if it is equivalent (after identification ofH with anL2{\displaystyle L^{2}} space) to amultiplication operator. It can be shown that the approximate point spectrum of a bounded multiplication operator equals its spectrum.

Discrete spectrum

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Thediscrete spectrum is defined as the set ofnormal eigenvalues or, equivalently, as the set of isolated points of the spectrum such that the correspondingRiesz projector is of finite rank. As such, the discrete spectrum is a strict subset of the point spectrum, i.e.,σd(T)σp(T).{\displaystyle \sigma _{d}(T)\subset \sigma _{p}(T).}

Continuous spectrum

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The set of allλ for whichTλI{\displaystyle T-\lambda I} is injective and has dense range, but is not surjective, is called thecontinuous spectrum ofT, denoted byσc(T){\displaystyle \sigma _{\mathbb {c} }(T)}. The continuous spectrum therefore consists of those approximate eigenvalues which are not eigenvalues and do not lie in the residual spectrum. That is,

σc(T)=σap(T)(σr(T)σp(T)){\displaystyle \sigma _{\mathrm {c} }(T)=\sigma _{\mathrm {ap} }(T)\setminus (\sigma _{\mathrm {r} }(T)\cup \sigma _{\mathrm {p} }(T))}.

For example,A:l2(N)l2(N){\displaystyle A:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )},ejej/j{\displaystyle e_{j}\mapsto e_{j}/j},jN{\displaystyle j\in \mathbb {N} }, is injective and has a dense range, yetRan(A)l2(N){\displaystyle \mathrm {Ran} (A)\subsetneq l^{2}(\mathbb {N} )}.Indeed, ifx=jNcjejl2(N){\textstyle x=\sum _{j\in \mathbb {N} }c_{j}e_{j}\in l^{2}(\mathbb {N} )} withcjC{\displaystyle c_{j}\in \mathbb {C} } such thatjN|cj|2<{\textstyle \sum _{j\in \mathbb {N} }|c_{j}|^{2}<\infty }, one does not necessarily havejN|jcj|2<{\textstyle \sum _{j\in \mathbb {N} }\left|jc_{j}\right|^{2}<\infty }, and thenjNjcjejl2(N){\textstyle \sum _{j\in \mathbb {N} }jc_{j}e_{j}\notin l^{2}(\mathbb {N} )}.

Compression spectrum

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The set ofλC{\displaystyle \lambda \in \mathbb {C} } for whichTλI{\displaystyle T-\lambda I} does not have dense range is known as thecompression spectrum ofT and is denoted byσcp(T){\displaystyle \sigma _{\mathrm {cp} }(T)}.

Residual spectrum

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The set ofλC{\displaystyle \lambda \in \mathbb {C} } for whichTλI{\displaystyle T-\lambda I} is injective but does not have dense range is known as theresidual spectrum ofT and is denoted byσr(T){\displaystyle \sigma _{\mathrm {r} }(T)}:

σr(T)=σcp(T)σp(T).{\displaystyle \sigma _{\mathrm {r} }(T)=\sigma _{\mathrm {cp} }(T)\setminus \sigma _{\mathrm {p} }(T).}

An operator may be injective, even bounded below, but still not invertible. The right shift onl2(N){\displaystyle l^{2}(\mathbb {N} )},R:l2(N)l2(N){\displaystyle R:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )},R:ejej+1,jN{\displaystyle R:\,e_{j}\mapsto e_{j+1},\,j\in \mathbb {N} }, is such an example. This shift operator is anisometry, therefore bounded below by 1. But it is not invertible as it is not surjective (e1Ran(R){\displaystyle e_{1}\not \in \mathrm {Ran} (R)}), and moreoverRan(R){\displaystyle \mathrm {Ran} (R)} is not dense inl2(N){\displaystyle l^{2}(\mathbb {N} )}(e1Ran(R)¯{\displaystyle e_{1}\notin {\overline {\mathrm {Ran} (R)}}}).

Peripheral spectrum

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The peripheral spectrum of an operator is defined as the set of points in its spectrum which have modulus equal to its spectral radius.[6]

Essential spectrum

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There are five similar definitions of theessential spectrum of closed densely defined linear operatorA:XX{\displaystyle A:\,X\to X} which satisfy

σess,1(A)σess,2(A)σess,3(A)σess,4(A)σess,5(A)σ(A).{\displaystyle \sigma _{\mathrm {ess} ,1}(A)\subset \sigma _{\mathrm {ess} ,2}(A)\subset \sigma _{\mathrm {ess} ,3}(A)\subset \sigma _{\mathrm {ess} ,4}(A)\subset \sigma _{\mathrm {ess} ,5}(A)\subset \sigma (A).}

All these spectraσess,k(A), 1k5{\displaystyle \sigma _{\mathrm {ess} ,k}(A),\ 1\leq k\leq 5}, coincide in the case of self-adjoint operators.

  1. The essential spectrumσess,1(A){\displaystyle \sigma _{\mathrm {ess} ,1}(A)} is defined as the set of pointsλ{\displaystyle \lambda } of the spectrum such thatAλI{\displaystyle A-\lambda I} is notsemi-Fredholm. (The operator issemi-Fredholm if its range is closed and either its kernel or cokernel (or both) is finite-dimensional.)
    Example 1:λ=0σess,1(A){\displaystyle \lambda =0\in \sigma _{\mathrm {ess} ,1}(A)} for the operatorA:l2(N)l2(N){\displaystyle A:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )},A:ejej/j, jN{\displaystyle A:\,e_{j}\mapsto e_{j}/j,~j\in \mathbb {N} } (because the range of this operator is not closed: the range does not include all ofl2(N){\displaystyle l^{2}(\mathbb {N} )} although its closure does).
    Example 2:λ=0σess,1(N){\displaystyle \lambda =0\in \sigma _{\mathrm {ess} ,1}(N)} forN:l2(N)l2(N){\displaystyle N:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )},N:v0{\displaystyle N:\,v\mapsto 0} for anyvl2(N){\displaystyle v\in l^{2}(\mathbb {N} )} (because both kernel and cokernel of this operator are infinite-dimensional).
  2. The essential spectrumσess,2(A){\displaystyle \sigma _{\mathrm {ess} ,2}(A)} is defined as the set of pointsλ{\displaystyle \lambda } of the spectrum such that the operator eitherAλI{\displaystyle A-\lambda I} has infinite-dimensional kernel or has a range which is not closed. It can also be characterized in terms ofWeyl's criterion: there exists asequence(xj)jN{\displaystyle (x_{j})_{j\in \mathbb {N} }} in the spaceX such thatxj=1{\displaystyle \Vert x_{j}\Vert =1},limj(AλI)xj=0,{\textstyle \lim _{j\to \infty }\left\|(A-\lambda I)x_{j}\right\|=0,} and such that(xj)jN{\displaystyle (x_{j})_{j\in \mathbb {N} }} contains no convergentsubsequence. Such a sequence is called asingular sequence (or asingular Weyl sequence).
    Example:λ=0σess,2(B){\displaystyle \lambda =0\in \sigma _{\mathrm {ess} ,2}(B)} for the operatorB:l2(N)l2(N){\displaystyle B:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )},B:ejej/2{\displaystyle B:\,e_{j}\mapsto e_{j/2}} ifj is even andej0{\displaystyle e_{j}\mapsto 0} whenj is odd (kernel is infinite-dimensional; cokernel is zero-dimensional). Note thatλ=0σess,1(B){\displaystyle \lambda =0\not \in \sigma _{\mathrm {ess} ,1}(B)}.
  3. The essential spectrumσess,3(A){\displaystyle \sigma _{\mathrm {ess} ,3}(A)} is defined as the set of pointsλ{\displaystyle \lambda } of the spectrum such thatAλI{\displaystyle A-\lambda I} is notFredholm. (The operator isFredholm if its range is closed and both its kernel and cokernel are finite-dimensional.)
    Example:λ=0σess,3(J){\displaystyle \lambda =0\in \sigma _{\mathrm {ess} ,3}(J)} for the operatorJ:l2(N)l2(N){\displaystyle J:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )},J:eje2j{\displaystyle J:\,e_{j}\mapsto e_{2j}} (kernel is zero-dimensional, cokernel is infinite-dimensional). Note thatλ=0σess,2(J){\displaystyle \lambda =0\not \in \sigma _{\mathrm {ess} ,2}(J)}.
  4. The essential spectrumσess,4(A){\displaystyle \sigma _{\mathrm {ess} ,4}(A)} is defined as the set of pointsλ{\displaystyle \lambda } of the spectrum such thatAλI{\displaystyle A-\lambda I} is notFredholm of index zero. It could also be characterized as the largest part of the spectrum ofA which is preserved bycompact perturbations. In other words,σess,4(A)=KB0(X)σ(A+K){\textstyle \sigma _{\mathrm {ess} ,4}(A)=\bigcap _{K\in B_{0}(X)}\sigma (A+K)}; hereB0(X){\displaystyle B_{0}(X)} denotes the set of all compact operators onX.
    Example:λ=0σess,4(R){\displaystyle \lambda =0\in \sigma _{\mathrm {ess} ,4}(R)} whereR:l2(N)l2(N){\displaystyle R:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )} is the right shift operator,R:l2(N)l2(N){\displaystyle R:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )},R:ejej+1{\displaystyle R:\,e_{j}\mapsto e_{j+1}} forjN{\displaystyle j\in \mathbb {N} } (its kernel is zero, its cokernel is one-dimensional). Note thatλ=0σess,3(R){\displaystyle \lambda =0\not \in \sigma _{\mathrm {ess} ,3}(R)}.
  5. The essential spectrumσess,5(A){\displaystyle \sigma _{\mathrm {ess} ,5}(A)} is the union ofσess,1(A){\displaystyle \sigma _{\mathrm {ess} ,1}(A)} with all components ofCσess,1(A){\displaystyle \mathbb {C} \setminus \sigma _{\mathrm {ess} ,1}(A)} that do not intersect with the resolvent setCσ(A){\displaystyle \mathbb {C} \setminus \sigma (A)}. It can also be characterized asσ(A)σd(A){\displaystyle \sigma (A)\setminus \sigma _{\mathrm {d} }(A)}.
    Example: consider the operatorT:l2(Z)l2(Z){\displaystyle T:\,l^{2}(\mathbb {Z} )\to l^{2}(\mathbb {Z} )},T:ejej1{\displaystyle T:\,e_{j}\mapsto e_{j-1}} forj0{\displaystyle j\neq 0},T:e00{\displaystyle T:\,e_{0}\mapsto 0}. SinceT=1{\displaystyle \Vert T\Vert =1}, one hasσ(T)D1¯{\displaystyle \sigma (T)\subset {\overline {\mathbb {D} _{1}}}}. For anyzC{\displaystyle z\in \mathbb {C} } with|z|=1{\displaystyle |z|=1}, the range ofTzI{\displaystyle T-zI} is dense but not closed, hence the boundary of the unit disc is in the first type of the essential spectrum:D1σess,1(T){\displaystyle \partial \mathbb {D} _{1}\subset \sigma _{\mathrm {ess} ,1}(T)}. For anyzC{\displaystyle z\in \mathbb {C} } with|z|<1{\displaystyle |z|<1},TzI{\displaystyle T-zI} has a closed range, one-dimensional kernel, and one-dimensional cokernel, sozσ(T){\displaystyle z\in \sigma (T)} althoughzσess,k(T){\displaystyle z\not \in \sigma _{\mathrm {ess} ,k}(T)} for1k4{\displaystyle 1\leq k\leq 4}; thus,σess,k(T)=D1{\displaystyle \sigma _{\mathrm {ess} ,k}(T)=\partial \mathbb {D} _{1}} for1k4{\displaystyle 1\leq k\leq 4}. There are two components ofCσess,1(T){\displaystyle \mathbb {C} \setminus \sigma _{\mathrm {ess} ,1}(T)}:{zC:|z|>1}{\displaystyle \{z\in \mathbb {C} :\,|z|>1\}} and{zC:|z|<1}{\displaystyle \{z\in \mathbb {C} :\,|z|<1\}}. The component{|z|<1}{\displaystyle \{|z|<1\}} has no intersection with the resolvent set; by definition,σess,5(T)=σess,1(T){zC:|z|<1}={zC:|z|1}{\displaystyle \sigma _{\mathrm {ess} ,5}(T)=\sigma _{\mathrm {ess} ,1}(T)\cup \{z\in \mathbb {C} :\,|z|<1\}=\{z\in \mathbb {C} :\,|z|\leq 1\}}.

Example: Hydrogen atom

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Thehydrogen atom provides an example of different types of the spectra. Thehydrogen atom Hamiltonian operatorH=ΔZ|x|{\displaystyle H=-\Delta -{\frac {Z}{|x|}}},Z>0{\displaystyle Z>0}, with domainD(H)=H1(R3){\displaystyle D(H)=H^{1}(\mathbb {R} ^{3})} has a discrete set of eigenvalues (the discrete spectrumσd(H){\displaystyle \sigma _{\mathrm {d} }(H)}, which in this case coincides with the point spectrumσp(H){\displaystyle \sigma _{\mathrm {p} }(H)} since there are no eigenvalues embedded into the continuous spectrum) that can be computed by theRydberg formula. Their correspondingeigenfunctions are calledeigenstates, or thebound states. The result of theionization process is described by the continuous part of the spectrum (the energy of the collision/ionization is not "quantized"), represented byσcont(H)=[0,+){\displaystyle \sigma _{\mathrm {cont} }(H)=[0,+\infty )} (it also coincides with the essential spectrum,σess(H)=[0,+){\displaystyle \sigma _{\mathrm {ess} }(H)=[0,+\infty )}).[citation needed][clarification needed]

Spectrum of the adjoint operator

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LetX be a Banach space andT:XX{\displaystyle T:\,X\to X} aclosed linear operator with dense domainD(T)X{\displaystyle D(T)\subset X}.IfX* is the dual space ofX, andT:XX{\displaystyle T^{*}:\,X^{*}\to X^{*}} is thehermitian adjoint ofT, then

σ(T)=σ(T)¯:={zC:z¯σ(T)}.{\displaystyle \sigma (T^{*})={\overline {\sigma (T)}}:=\{z\in \mathbb {C} :{\bar {z}}\in \sigma (T)\}.}

TheoremFor a bounded (or, more generally, closed and densely defined) operatorT,

σcp(T)=σp(T)¯{\displaystyle \sigma _{\mathrm {cp} }(T)={\overline {\sigma _{\mathrm {p} }(T^{*})}}}.

In particular,σr(T)σp(T)¯σr(T)σp(T){\displaystyle \sigma _{\mathrm {r} }(T)\subset {\overline {\sigma _{\mathrm {p} }(T^{*})}}\subset \sigma _{\mathrm {r} }(T)\cup \sigma _{\mathrm {p} }(T)}.

Proof

Suppose thatRan(TλI){\displaystyle \mathrm {Ran} (T-\lambda I)} is not dense inX. By theHahn–Banach theorem, there exists a non-zeroφX{\displaystyle \varphi \in X^{*}} that vanishes onRan(TλI){\displaystyle \mathrm {Ran} (T-\lambda I)}. For allxX,

φ,(TλI)x=(Tλ¯I)φ,x=0.{\displaystyle \langle \varphi ,(T-\lambda I)x\rangle =\langle (T^{*}-{\bar {\lambda }}I)\varphi ,x\rangle =0.}

Therefore,(Tλ¯I)φ=0X{\displaystyle (T^{*}-{\bar {\lambda }}I)\varphi =0\in X^{*}} andλ¯{\displaystyle {\bar {\lambda }}} is an eigenvalue ofT*.

Conversely, suppose thatλ¯{\displaystyle {\bar {\lambda }}} is an eigenvalue ofT*. Then there exists a non-zeroφX{\displaystyle \varphi \in X^{*}} such that(Tλ¯I)φ=0{\displaystyle (T^{*}-{\bar {\lambda }}I)\varphi =0}, i.e.

xX,(Tλ¯I)φ,x=φ,(TλI)x=0.{\displaystyle \forall x\in X,\;\langle (T^{*}-{\bar {\lambda }}I)\varphi ,x\rangle =\langle \varphi ,(T-\lambda I)x\rangle =0.}

IfRan(TλI){\displaystyle \mathrm {Ran} (T-\lambda I)} is dense inX, thenφ must be the zero functional, a contradiction. The claim is proved.

We also getσp(T)σr(T)σp(T)¯{\displaystyle \sigma _{\mathrm {p} }(T)\subset {\overline {\sigma _{\mathrm {r} }(T^{*})\cup \sigma _{\mathrm {p} }(T^{*})}}} by the following argument:X embeds isometrically intoX**. Therefore, for every non-zero element in the kernel ofTλI{\displaystyle T-\lambda I} there exists a non-zero element inX** which vanishes onRan(Tλ¯I){\displaystyle \mathrm {Ran} (T^{*}-{\bar {\lambda }}I)}. ThusRan(Tλ¯I){\displaystyle \mathrm {Ran} (T^{*}-{\bar {\lambda }}I)} can not be dense.

Furthermore, ifX is reflexive, we haveσr(T)¯σp(T){\displaystyle {\overline {\sigma _{\mathrm {r} }(T^{*})}}\subset \sigma _{\mathrm {p} }(T)}.

Spectra of particular classes of operators

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Compact operators

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IfT is acompact operator, or, more generally, aninessential operator, then it can be shown that the spectrum is countable, that zero is the only possibleaccumulation point, and that any nonzeroλ in the spectrum is an eigenvalue.

Quasinilpotent operators

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A bounded operatorA:XX{\displaystyle A:\,X\to X} isquasinilpotent ifAn1/n0{\displaystyle \lVert A^{n}\rVert ^{1/n}\to 0} asn{\displaystyle n\to \infty } (in other words, if the spectral radius ofA equals zero). Such operators could equivalently be characterized by the condition

σ(A)={0}.{\displaystyle \sigma (A)=\{0\}.}

An example of such an operator isA:l2(N)l2(N){\displaystyle A:\,l^{2}(\mathbb {N} )\to l^{2}(\mathbb {N} )},ejej+1/2j{\displaystyle e_{j}\mapsto e_{j+1}/2^{j}} forjN{\displaystyle j\in \mathbb {N} }.

Self-adjoint operators

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IfX is aHilbert space andT is aself-adjoint operator (or, more generally, anormal operator), then a remarkable result known as thespectral theorem gives an analogue of the diagonalisation theorem for normal finite-dimensional operators (Hermitian matrices, for example).

For self-adjoint operators, one can usespectral measures to define adecomposition of the spectrum into absolutely continuous, pure point, and singular parts.

Spectrum of a real operator

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The definitions of the resolvent and spectrum can be extended to any continuous linear operatorT{\displaystyle T} acting on a Banach spaceX{\displaystyle X} over the real fieldR{\displaystyle \mathbb {R} } (instead of the complex fieldC{\displaystyle \mathbb {C} }) via itscomplexificationTC{\displaystyle T_{\mathbb {C} }}. In this case we define the resolvent setρ(T){\displaystyle \rho (T)} as the set of allλC{\displaystyle \lambda \in \mathbb {C} } such thatTCλI{\displaystyle T_{\mathbb {C} }-\lambda I} is invertible as an operator acting on the complexified spaceXC{\displaystyle X_{\mathbb {C} }}; then we defineσ(T)=Cρ(T){\displaystyle \sigma (T)=\mathbb {C} \setminus \rho (T)}.

Real spectrum

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Thereal spectrum of a continuous linear operatorT{\displaystyle T} acting on a real Banach spaceX{\displaystyle X}, denotedσR(T){\displaystyle \sigma _{\mathbb {R} }(T)}, is defined as the set of allλR{\displaystyle \lambda \in \mathbb {R} } for whichTλI{\displaystyle T-\lambda I} fails to be invertible in the real algebra of bounded linear operators acting onX{\displaystyle X}. In this case we haveσ(T)R=σR(T){\displaystyle \sigma (T)\cap \mathbb {R} =\sigma _{\mathbb {R} }(T)}. Note that the real spectrum may or may not coincide with the complex spectrum. In particular, the real spectrum could be empty.

Spectrum of a unital Banach algebra

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This sectionneeds expansion. You can help byadding missing information.(June 2009)

LetB be a complexBanach algebra containing aunite. Then we define the spectrumσ(x) (or more explicitlyσB(x)) of an elementx ofB to be the set of thosecomplex numbersλ for whichλe − x is not invertible inB. This extends the definition for bounded linear operatorsB(X) on a Banach spaceX, sinceB(X) is a unital Banach algebra.

See also

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Notes

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  1. ^Kreyszig, Erwin.Introductory Functional Analysis with Applications.
  2. ^Theorem 3.3.3 of Kadison & Ringrose, 1983,Fundamentals of the Theory of Operator Algebras, Vol. I: Elementary Theory, New York: Academic Press, Inc.
  3. ^"Nonempty intersection between approximate point spectrum and residual spectrum".
  4. ^Teschl 2014, p. 115.
  5. ^Simon 2005, p. 44.
  6. ^Zaanen, Adriaan C. (2012).Introduction to Operator Theory in Riesz Spaces. Springer Science & Business Media. p. 304.ISBN 9783642606373. Retrieved8 September 2017.

References

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