# Eigenvalue, eigenvector and eigenspace

File:Eigen.jpg
Fig. 1. In this shear transformation of the Mona Lisa, the picture was deformed in such a way that its central vertical axis was not modified. (Note: The corners have been cropped on the right hand picture.) The blue vector, from her chest to her shoulder, has changed direction, but the red one, from her chest to her chin, is unchanged. The red vector is thus an eigenvector of the transformation and the blue vector is not. Since the red vector was neither stretched nor compressed, its eigenvalue is 1. All vectors along the same vertical line are also eigenvectors, with the same eigenvalue. They form the eigenspace for this eigenvalue.

In mathematics, an eigenvector of a transformation is a non-null vector whose direction is unchanged by that transformation. The factor by which the magnitude is scaled is called the eigenvalue of that vector. A pictorial example is provided in Fig. 1. Often, a transformation is completely described by its eigenvalues and eigenvectors. An eigenspace is a set of eigenvectors with the same eigenvalue.

These concepts play a major role in several branches of both pure and applied mathematics — appearing prominently in linear algebra, functional analysis, and even a variety of nonlinear situations.

The German word eigen was first used in this context by Hilbert in 1904 (there was an earlier related usage by Helmholtz). "Eigen" can be translated as "own", "peculiar to", "characteristic" or "individual"—emphasizing how important eigenvalues are to defining the unique nature of a specific transformation. In English mathematical jargon, the closest translation would be "characteristic"; and some older references do use expressions like "characteristic value" and "characteristic vector", or even "Eigenwert", German for eigenvalue. In the past, the standard translation used to be "proper". Today the more distinctive term "eigenvalue" is standard.

## Definitions

Transformations of space—such as translation (or shifting the origin), rotation, reflection, stretching, compression, or any combination of these; other transformations could also be listed—may be visualized by the effect they produce on vectors. Vectors can be visualised as arrows pointing from one point to another.

• Eigenvectors of transformations are vectors which are either left unaffected or simply multiplied by a scale factor after the transformation.
• An eigenvector's eigenvalue is the scale factor that it has been multiplied by.
• An eigenspace is a space consisting of all eigenvectors which have the same eigenvalue.
• The geometric multiplicity of an eigenvalue is the dimension of the associated eigenspace.
• The spectrum of a transformation is the set of all its eigenvalues.

For instance, an eigenvector of a rotation in three dimensions is a vector located within the axis around which the rotation is performed. The corresponding eigenvalue is 1 and the corresponding eigenspace contains all the vectors parallel to the axis. As this is a one-dimensional space, its geometric multiplicity is one. This is the only eigenvalue of the spectrum (of this rotation) that is a real number.

## Examples

As the Earth rotates, every arrow pointing outward from the center of the Earth also rotates, except those arrows that lie on the axis of rotation. Consider the transformation of the Earth after one hour of rotation: An arrow from the center of the Earth to the Geographic South Pole would be an eigenvector of this transformation, but an arrow from the center of the Earth to anywhere on the equator would not be an eigenvector. Since the arrow pointing at the pole is not stretched by the rotation of the Earth, its eigenvalue is 1.

Another example is provided by a thin metal sheet expanding uniformly about a fixed point in such a way that the distances from any point of the sheet to the fixed point are doubled. This expansion is a transformation with eigenvalue 2. Every vector from the fixed point to a point on the sheet is an eigenvector, and the eigenspace is the set of all these vectors.

File:Standing wave.gif
Fig. 2. A standing wave in a rope fixed at its boundaries can be seen as an example of an eigenvector, or more precisely, an eigenfunction of the transformation corresponding to the passage of time. As time passes, the standing wave is scaled but its shape is not modified. In this case the eigenvalue is time dependent.

However, three-dimensional geometric space is not the only vector space. For example, consider a stressed rope fixed at both ends, like the vibrating strings of a string instrument (Fig. 2). The distances of atoms of the vibrating rope from their positions when the rope is at rest can be seen as the components of a vector in a space with as many dimensions as there are atoms in the rope.

If one considers the transformation of the rope as time passes, its eigenvectors, or eigenfunctions, if one assumes the rope is a continuous medium, are its standing waves—the things that, mediated by the surrounding air, humans can experience as the twang of a bow string or the plink of a guitar. The standing waves correspond to particular oscillations of the rope such that the shape of the rope is scaled by a factor (the eigenvalue) as time passes. Each component of the vector associated with the rope is multiplied by this time-dependent factor. The amplitude (eigenvalues) of the standing waves decrease with time if damping is considered. One can then associate a lifetime with the eigenvector, and relate the concept of an eigenvector to the concept of resonance.

## Eigenvalue equation

Mathematically, vλ is an eigenvector and λ the corresponding eigenvalue of a transformation ${\mathcal {T}}$ if the equation:

${\mathcal {T}}(\mathbf {v} _{\lambda })=\lambda \,\mathbf {v} _{\lambda }$ is true, where ${\mathcal {T}}(\mathbf {v} _{\lambda })$ is the vector obtained when applying the transformation ${\mathcal {T}}$ to vλ.

Suppose ${\mathcal {T}}$ is a linear transformation (which means that ${\mathcal {T}}(a\mathbf {v} +b\mathbf {w} )=a{\mathcal {T}}(\mathbf {v} )+b{\mathcal {T}}(\mathbf {w} )$ for all scalars a, b, and vectors v, w). Consider a basis in that vector space. Then, ${\mathcal {T}}$ and vλ can be represented relative to that basis by a matrix T—a two-dimensional array—and respectively a column vector vλ—a one-dimensional vertical array. The eigenvalue equation in its matrix representation is written

$T\,v_{\lambda }=\lambda \,v_{\lambda }$ where the juxtaposition is matrix multiplication. This is equivalent to a set of n linear equations, where n is the number of basis vectors in the basis set. In this equation both the eigenvalue λ and the n components of vλ are unknowns.

However, it is sometimes unnatural or even impossible to write down the eigenvalue equation in a matrix form. This occurs for instance when the vector space is infinite dimensional, for example, in the case of the rope above. Depending on the nature of the transformation ${\mathcal {T}}$ and the space to which it applies, it can be advantageous to represent the eigenvalue equation as a set of differential equations depending on the nature of the transformation ${\mathcal {T}}$ and the space to which it applies. If ${\mathcal {T}}$ is a differential operator, the eigenvectors are commonly called eigenfunctions of the differential operator representing ${\mathcal {T}}$ . For example, differentiation itself is a linear transformation since (if M and N are differentiable functions, and a and b are constants)

$d(aM+bN)/dt=adM/dt+bdN/dt$ Consider differentiation with respect to time, $t$ . Its eigenfunctions obey the eigenvalue equation:

${dN/dt}=\lambda N$ ,

where λ is the eigenvalue associated with the function. Such a function of time is constant if $\lambda =0$ , grows proportionally to itself if $\lambda$ is positive, and decays proportionally to itself if $\lambda$ is negative. For example, an idealized population of rabbits breeds faster the more rabbits there are, and thus satisfies the equation with a positive lambda.

The solution to the eigenvalue equation is $N=\exp(\lambda t)$ , the exponential function; thus that function is an eigenfunction of the differential operator d/dt with the eigenvalue λ. If λ is negative, we call the evolution of N an exponential decay; if it is positive, an exponential growth. The value of λ can be any complex number. The spectrum of d/dt is therefore the whole complex plane. In this example the vector space in which the operator d/dt acts is the space of the differentiable functions of one variable. This space has an infinite dimension (because it is not possible to express any differentiable function as a linear combination of a finite number of basis functions). However, the eigenspace associated with any given eigenvalue λ is one dimensional. It is the set of all functions $N=N_{0}\exp(\lambda t)$ . N0 is an arbitrary constant, the initial population at t=0.

## Spectral theorem

For more details on this topic, see spectral theorem.

The spectral theorem depicts the whole importance of the eigenvalues and eigenvectors for characterizing a linear transformation in a unique way. In its simplest version, the spectral theorem states that, under precise conditions, a linear transformation of a vector can be expressed as the linear combination of the eigenvectors with coefficients equal to the eigenvalues times the scalar product (or dot product) of the eigenvectors with the vector on which the transformation is applied. Mathematically, it can be written as:

${\mathcal {T}}(\mathbf {v} )=\lambda _{1}(\mathbf {v} _{1}\cdot \mathbf {v} )\mathbf {v} _{1}+\lambda _{2}(\mathbf {v} _{2}\cdot \mathbf {v} )\mathbf {v} _{2}+\dots$ where $\mathbf {v} _{1},\mathbf {v} _{2},\dots$ and $\lambda _{1},\lambda _{2},\dots$ stand for the eigenvectors and eigenvalues of ${\mathcal {T}}$ . The simplest case in which the theorem is valid is the case where the linear transformation is given by a real symmetric matrix or complex Hermitian matrix.

If one defines the nth power of a transformation as the result of applying it n times in succession, one can also define polynomials of transformations. A more general version of the theorem is that any polynomial P of ${\mathcal {T}}$ is equal to:

$P({\mathcal {T}})(\mathbf {v} )=P(\lambda _{1})(\mathbf {v} _{1}\cdot \mathbf {v} )\mathbf {v} _{1}+P(\lambda _{2})(\mathbf {v} _{2}\cdot \mathbf {v} )\mathbf {v} _{2}+\dots$ The theorem can be extended to other functions of transformations like analytic functions, the most general case being Borel functions.

## Eigenvalues and eigenvectors of matrices

### Computing eigenvalues and eigenvectors of matrices

Suppose that we want to compute the eigenvalues of a given matrix. If the matrix is small, we can compute them symbolically using the characteristic polynomial. However, this is often impossible for larger matrices, in which case we must use a numerical method.

#### Symbolic computations

For more details on this topic, see symbolic computation of matrix eigenvalues.
Finding eigenvalues

An important tool for describing eigenvalues of square matrices is the characteristic polynomial: saying that λ is an eigenvalue of A is equivalent to stating that the system of linear equations (AλI) v = 0 (where I is the identity matrix) has a non-zero solution v (an eigenvector), and so it is equivalent to the determinant:

$\det(A-\lambda I)=0\!\$ The function p(λ) = det(AλI) is a polynomial in λ since determinants are defined as sums of products. This is the characteristic polynomial of A: the eigenvalues of a matrix are the zeros of its characteristic polynomial.

All the eigenvalues of a matrix A can be computed by solving the equation $p_{A}(\lambda )=0$ . If A is an n×n matrix, then $p_{A}$ has degree n and A can therefore have at most n eigenvalues. Conversely, the fundamental theorem of algebra says that this equation has exactly n roots (zeroes), counted with multiplicity. All real polynomials of odd degree have a real number as a root, so for odd n, every real matrix has at least one real eigenvalue. In the case of a real matrix, for even and odd n, the non-real eigenvalues come in conjugate pairs.

Finding eigenvectors

Once the eigenvalues λ are known, the eigenvectors can then be found by solving:

$(A-\lambda I)v=0\!\$ An example of a matrix with no real eigenvalues is the 90-degree clockwise rotation:

${\begin{bmatrix}0&1\\-1&0\end{bmatrix}}$ whose characteristic polynomial is $\lambda ^{2}+1$ and so its eigenvalues are the pair of complex conjugates i, -i. The associated eigenvectors are also not real.

#### Numerical computations

For more details on this topic, see eigenvalue algorithm.

In practice, eigenvalues of large matrices are not computed using the characteristic polynomial. Computing the polynomial becomes expensive in itself, and exact (symbolic) roots of a high-degree polynomial can be difficult to compute and express: the Abel–Ruffini theorem implies that the roots of high-degree (5 and above) polynomials cannot be expressed simply using $n$ th roots. Effective numerical algorithms for approximating roots of polynomials exist, but small errors in the eigenvalues can lead to large errors in the eigenvectors. Therefore, general algorithms to find eigenvectors and eigenvalues, are iterative. The easiest method is the power method: a random vector v is chosen and computed as Av, $A^{2}v$ , $A^{3}v$ , ... This sequence will after normalization almost always converge to an eigenvector corresponding to the dominant eigenvalue. This algorithm is easy, but not very useful by itself. However, popular methods such as the QR algorithm are based on it.

### Properties

#### Algebraic multiplicity

The algebraic multiplicity of an eigenvalue λ of A is the order of λ as a zero of the characteristic polynomial of A; in other words, if λ is one root of the polynomial, it is the number of factors (tλ) in the characteristic polynomial after factorization. An n×n matrix has n eigenvalues, counted according to their algebraic multiplicity, because its characteristic polynomial has degree n.

An eigenvalue of algebraic multiplicity 1 is called a "simple eigenvalue".

In an article on matrix theory, a statement like the one below might be encountered:

"the eigenvalues of a matrix A are 4,4,3,3,3,2,2,1,"

meaning that the algebraic multiplicity of 4 is two, of 3 is three, of 2 is two and of 1 is one. This style is used because algebraic multiplicity is the key to many mathematical proofs in matrix theory.

The algebraic multiplicity can also be thought of as a dimension: it is the dimension of the associated generalized eigenspace (1st sense), which is the nullspace of the matrix (λI − A)k for any sufficiently large k. That is, it is the space of generalized eigenvectors (1st sense), where a generalized eigenvector is any vector which eventually becomes 0 if λI − A is applied to it enough times successively. Any eigenvector is a generalized eigenvector, and so each eigenspace is contained in the associated generalized eigenspace. This provides an easy proof that the geometric multiplicity is always less than or equal to the algebraic multiplicity. The first sense should not to be confused with generalized eigenvalue problem as stated below.

For example:

$A={\begin{bmatrix}1&1\\0&1\end{bmatrix}}.$ It has only one eigenvalue, namely λ = 1. The characteristic polynomial is $(\lambda -1)^{2}$ , so this eigenvalue has algebraic multiplicity 2. However, the associated eigenspace is the axis usually called the x axis, spanned by the unit vector ${\begin{bmatrix}1\\0\end{bmatrix}}$ , so the geometric multiplicity is only 1.

#### Decomposition theorem

The decomposition theorem is a version of the spectral theorem in the particular case of matrices. This theorem is usually introduced in terms of coordinate transformation. If U is an invertible matrix, it can be seen as a transformation from one coordinate system to another. In this new system the coordinates of the vector $\mathbf {v}$ are labeled $v'$ . The latter are obtained from the coordinates v in the original coordinate system by the relation $v'=Uv$ and, the other way around, we have $v=U^{-1}v'$ . Applying successively $v'=Uv$ , $w'=Uw$ and $U^{-1}U=I$ , to the relation $Av=w$ defining the matrix multiplication provides $A'v'=w'$ with $A'=UAU^{-1}$ , the representation of A in the new basis. The columns of U being the components of the new basis vectors within the old basis set. The decomposition theorem states that, if one chooses as columns of U n linearly independent eigenvectors of A, the new matrix $A'=UAU^{-1}$ is diagonal and its diagonal elements are the eigenvalues of A. If this is possible the matrix A is diagonalizable. An example of non-diagonalizable matrix is given by the matrix A above.

There are several generalizations of this decomposition which can cope with the non-diagonalizable case, suited for different purposes:

• the singular value decomposition, $A=U\Sigma V^{*}$ where $\Sigma$ is diagonal but U is not necessarily equal to V;
• the Jordan normal form, where $A=U\Lambda U^{-1}$ where $\Lambda$ is not diagonal but of a simple form with non vanishing entries only along the diagonal and one element above;
• any matrix A can be written uniquely as A = S + N where S is diagonalizable, N is nilpotent (i.e., such that Nq=0 for some q), and S commutes with N (SN=NS).
• any invertible matrix A can be written uniquely as A = SJ where S is diagonalizable and J is unipotent (i.e., such that the characteristic polynomial is a power of (λ-1), and S commutes with J).

#### Other theorems

The spectrum is invariant under similarity transformations: the matrices A and P-1AP have the same eigenvalues for any matrix A and any invertible matrix P. The spectrum is also invariant under transposition: the matrices A and AT have the same eigenvalues.

A matrix is invertible if and only if zero is not an eigenvalue of the matrix.

A matrix is diagonalizable if and only if the algebraic and geometric multiplicities coincide for all its eigenvalues. In particular, an n×n matrix which has n different eigenvalues is always diagonalizable.

The vector space on which the matrix acts is always the direct sum of the generalized eigenspaces (i.e., is spanned by them and they are independent). This is true of the ordinary (non-generalized) eigenspaces if and only if they are equal to the generalized eigenspaces, i.e., if and only if the matrix is diagonalizable.

The location of the spectrum is often restricted if the matrix has a special form:

Generally, the trace, or the sum of the elements on the main diagonal of a matrix, equals the sum of the eigenvalues, and the determinant equals the product of the eigenvalues (counted according to algebraic multiplicity).

Suppose that A is an m×n matrix, with mn, and that B is an n×m matrix. Then BA has the same eigenvalues as AB plus nm eigenvalues equal to zero.

### Conjugate eigenvector

A conjugate eigenvector or coneigenvector is a vector sent after transformation to a scalar multiple of its conjugate, where the scalar is called the conjugate eigenvalue or coneigenvalue of the linear transformation. The coneigenvectors and coneigenvalues represent essentially the same information and meaning as the regular eigenvectors and eigenvalues, but arise when a alternative coordinate system is used. The corresponding equation is

$Av=\lambda v^{*}.\,$ For example, in coherent electromagnetic scattering theory, the linear transformation A represents the action performed by the scattering object, and the eigenvectors represent polarization states of the electromagnetic wave. In optics, the coordinate system is defined from the wave's viewpoint, known as the Forward Scattering Alignment (FSA), and gives rise to a regular eigenvalue equation, whereas in radar, the coordinate system is defined from the radar's viewpoint, known as the Back Scattering Alignment (BSA), and gives rise to a coneigenvalue equation.

### Generalized eigenvalue problem

A generalized eigenvalue problem (2nd sense) is of the form

$Av=\lambda Bv\quad \quad$ where A and B are matrices. The generalized eigenvalues (2nd sense) λ can be obtained by solving the equation

$\det(A-\lambda B)=0.\,$ The set of matrices of the form $A-\lambda B$ , where $\lambda$ is a complex number, is called a pencil. If B is invertible, then the original problem can be written in the form

$B^{-1}Av=\lambda v\quad \quad$ which is a standard eigenvalue problem. However, in most situations it is preferable not to perform the inversion, and solve the generalized eigenvalue problem as stated originally.

If A and B are symmetric matrices with real entries, then the eigenvalues are real. This would have not been easy to see from the second equivalent formulation, because the matrix $B^{-1}A$ is not necessarily symmetric if A and B are.

An example is provided by the molecular orbital application below.

### Entries from a ring

In the case of a square matrix A with entries in a ring, λ is called a right eigenvalue if there exists a column vector x such that Axx, or a left eigenvalue if there exists a nonzero row vector y such that yA=yλ.

If the ring is commutative, the left eigenvalues are equal to the right eigenvalues and are just called eigenvalues. If not, for instance if the ring is the set of quaternions, they may be different.

## Infinite-dimensional spaces

File:Discrete-continuum.gif
Fig. 3.Absorption spectrum (cross section) of atomic Chlorine. The sharp lines obtained in theory correspond to the discrete spectrum (Rydberg series) of the Hamiltonian; the broad structure on the right is associated to the continuous spectrum (ionization). The associated experimental results have been obtained by measuring the intensity of X-rays absorbed by a gas of atoms as a function of the incident photon energy in eV.

If the vector space is infinite dimensional, it may be advantageous to define the concept of spectral values. The spectral values are the set of scalars λ for which the Green's operator, $\left({\mathcal {T}}-\lambda \right)^{-1}$ , associated to the transformation is not defined, that is such that ${\mathcal {T}}-\lambda$ is not invertible (i.e., the inverse transformation to ${\mathcal {T}}-\lambda$ does not exist).

If λ is an eigenvalue of ${\mathcal {T}}$ , λ is also a spectral value of it. However, the reverse relation is not true: any spectral value is not an eigenvalue. There are operators on Hilbert or Banach spaces which have no eigenvectors at all. This can be seen on the following example. The bilateral shift on the Hilbert space $\ell ^{2}(\mathbf {Z} )$ (the space of all sequences of scalars $\dots a_{-1},a_{0},a_{1},a_{2},\dots$ such that $\dots |a_{-1}|^{2}+|a_{0}|^{2}+|a_{1}|^{2}+|a_{2}|^{2}+\dots$ converge) has no eigenvalue but has spectral values.

In functional analysis, the spectrum of an operator is defined as the set of all its spectral values. This is a key concept in scattering theory.

In infinite-dimensional spaces, the spectrum of an operator can be discrete or continuous. The former case occurs if the spectrum is a countable set of scalars; the latter if not. The exponential growth or decay provides an example of a continuous spectrum and the vibrating string an example above. The hydrogen atom is an example where both type of spectra appear. The bound states of the hydrogen atom correspond to the discrete part of the spectrum while the ionization processes are described by the continuous part. Fig. 3 exemplifies this concept in the case of the Chlorine atom.

## Applications

Schrödinger equation
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Fig. 4. The wavefunctions associated to the bound states of an electron in a hydrogen atom can be seen as the eigenvectors of the hydrogen atom Hamiltonian as well as of the angular momentum operator. They are associated to eigenvalues interpreted as their energies (increasing downward: n=1,2,3,...) and angular momentum (increasing across: s, p, d,...). Here are plotted the square of the absolute value of the wavefunctions. Brighter areas correspond to higher probability density for a position measurement. The center of each figure is the atomic nucleus, a proton

An example of an eigenvalue equation where the transformation ${\mathcal {T}}$ is represented in terms of a differential operator is the time-independent Schrödinger equation in quantum mechanics

$H\Psi _{E}=E\Psi _{E}$ where H, the Hamiltonian, is a second-order differential operator and $\Psi _{E}$ , the wavefunction, is one of its eigenfunctions corresponding to the eigenvalue E, interpreted as its energy.

However, in the case we only look for the bound state solutions of the Schrödinger equation, as is usually the case in quantum chemistry, we look for $\Psi _{E}$ within the space of square integrable functions. Since this space is a Hilbert space, with a well-defined scalar product, we can introduce a basis set in which $\Psi _{E}$ and H can be represented as a one-dimensional array and a matrix respectively. This allows us to represent the Schrödinger equation in a matrix form. (Fig. 4 presents the lowest eigenfunctions of the Hydrogen atom Hamiltonian.)

The Dirac notation often used in this context stresses the difference between the vector or state $|\Psi _{E}\rangle$ and its representation, the function $\Psi _{E}$ . In this context one writes the Schrödinger equation

$H|\Psi _{E}\rangle =E|\Psi _{E}\rangle$ and call $|\Psi _{E}\rangle$ an eigenstate of H (sometimes written ${\hat {H}}$ in introductory textbooks) which is seen as a transformation (see Observable) instead of particular representation of it in terms of differential operators. In the equation above $H|\Psi _{E}\rangle$ is understood as the vector obtained by application of the transformation H to $|\Psi _{E}\rangle$ .

Molecular orbitals

In quantum mechanics, and in particular in atomic and molecular physics, within the Hartree-Fock theory, the atomic and molecular orbitals can be defined by the eigenvectors of the Fock operator. The corresponding eigenvalues are interpreted as ionization potentials via Koopmans' theorem. In this case, the term eigenvector is used in a somewhat more general meaning, since the Fock operator is explicitly dependent of the orbitals and their eigenvalues. If one wants to underline this aspect one speaks of implicit eigenvalue equation. Such equations are usually solved by an iteration procedure, called in this case self-consistent field method. In quantum chemistry, one often represents the Hartree-Fock equation in a non-orthogonal basis set. This particular representation is a generalized eigenvalue problem called Roothaan equations.

Factor analysis

In factor analysis, the eigenvectors of a covariance matrix correspond to factors, and eigenvalues to factor loadings. Factor analysis is a statistical technique used in the social sciences and in marketing, product management, operations research, and other applied sciences that deal with large quantities of data. The objective is to explain most of the variability among a number of observable random variables in terms of a smaller number of unobservable random variables called factors. The observable random variables are modeled as linear combinations of the factors, plus "error" terms.

File:Eigenfaces.png
Fig. 5. Eigenfaces as examples of eigenvectors
Eigenfaces

In image processing, processed images of faces can be seen as vectors whose components are the brightnesses of each pixel. The dimension of this vector space is the number of pixels. The eigenvectors of the covariance matrix associated to a large set of normalized pictures of faces are called eigenfaces. They are very useful for expressing any face image as a linear combination of some of them. Eigenfaces provide a means of applying data compression to faces for identification purposes.

Tensor of inertia

In mechanics, the eigenvectors of the inertia tensor define the principal axes of a rigid body. The tensor of inertia is a key quantity required in order to determine the rotation of a rigid body around its center of mass.

Stress tensor

In solid mechanics, the stress tensor is symmetric and so can be decomposed into a diagonal tensor with the eigenvalues on the diagonal and eigenvectors as a basis. Because it is diagonal, in this orientation, the stress tensor has no shear components; the components it does have are the principal components.

Eigenvalues of a graph

In spectral graph theory, an eigenvalue of a graph is defined as an eigenvalue of the graph's adjacency matrix A, or (increasingly) of the graph's Laplacian matrix $I-T^{-1/2}AT^{-1/2}$ , where T is a diagonal matrix holding the degree of each vertex, and in $T^{-1/2}$ , 0 is substituted for $0^{-1/2}$ . The principal eigenvector of a graph is used to measure the centrality of its vertices. An example is Google's PageRank algorithm. The principal eigenvector of a modified adjacency matrix of the www-graph gives the page ranks as its components.