Eigenvalues and eigenvectors

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In this shear mapping the red arrow changes direction but the blue arrow does not. The blue arrow is an eigenvector of this shear mapping, and since its length is unchanged its eigenvalue is 1.

An eigenvector of a square matrix A is a non-zero vector v that, when the matrix is multiplied by v, yields a constant multiple of v, the multiplier being commonly denoted by \lambda. That is:

A v = \lambda v

(Because this equation uses post-multiplication by v, it describes a right eigenvector.)

The number \lambda is called the eigenvalue of A corresponding to v.[1]

If 2D space is visualized as a piece of cloth being stretched by the matrix, the eigenvectors would make up the line along the direction the cloth is stretched in and the line of cloth at the center of the stretching, whose direction isn't changed by the stretching either. The eigenvalues for the first line would give the scale to which the cloth is stretched, and for the second line the scale to which it's tightened. A reflection may be viewed as stretching a line to scale -1 while shrinking the axis of reflection to scale 1. For 3D rotations, the eigenvectors form the axis of rotation, and since the scale of the axis is unchanged by the rotation, their eigenvalues are all 1.

In analytic geometry, for example, a three-element vector may be seen as an arrow in three-dimensional space starting at the origin. In that case, an eigenvector v is an arrow whose direction is either preserved or exactly reversed after multiplication by A. The corresponding eigenvalue determines how the length of the arrow is changed by the operation, and whether its direction is reversed or not, determined by whether the eigenvalue is negative or positive.

In abstract linear algebra, these concepts are naturally extended to more general situations, where the set of real scalar factors is replaced by any field of scalars (such as algebraic or complex numbers); the set of Cartesian vectors \mathbb{R}^n is replaced by any vector space (such as the continuous functions, the polynomials or the trigonometric series), and matrix multiplication is replaced by any linear operator that maps vectors to vectors (such as the derivative from calculus). In such cases, the "vector" in "eigenvector" may be replaced by a more specific term, such as "eigenfunction", "eigenmode", "eigenface", or "eigenstate". Thus, for example, the exponential function f(x) = a^x is an eigenfunction of the derivative operator " {}' ", with eigenvalue \lambda = \ln a, since its derivative is f'(x) = (\ln a)a^x = \lambda f(x).

The set of all eigenvectors of a matrix (or linear operator), each paired with its corresponding eigenvalue, is called the eigensystem of that matrix.[2] Any multiple of an eigenvector is also an eigenvector, with the same eigenvalue. An eigenspace of a matrix A is the set of all eigenvectors with the same eigenvalue, together with the zero vector.[1] An eigenbasis for A is any basis for the set of all vectors that consists of linearly independent eigenvectors of A. Not every matrix has an eigenbasis, but every symmetric matrix does.

The terms characteristic vector, characteristic value, and characteristic space are also used for these concepts. The prefix eigen- is adopted from the German word eigen for "self-" or "unique to", "peculiar to", or "belonging to" in the sense of "idiosyncratic" in relation to the originating matrix.

Eigenvalues and eigenvectors have many applications in both pure and applied mathematics. They are used in matrix factorization, in quantum mechanics, and in many other areas.

Definition[edit]

Eigenvectors and eigenvalues of a real matrix[edit]

Matrix A acts by stretching the vector x, not changing its direction, so x is an eigenvector of A.

In many contexts, a vector can be assumed to be a list of real numbers (called elements), written vertically with brackets around the entire list, such as the vectors u and v below. Two vectors are said to be scalar multiples of each other (also called parallel or collinear) if they have the same number of elements, and if every element of one vector is obtained by multiplying each corresponding element in the other vector by the same number (known as a scaling factor, or a scalar). For example, the vectors

u = \begin{bmatrix}1\\3\\4\end{bmatrix}\quad\quad\quad and \quad\quad\quad v = \begin{bmatrix}-20\\-60\\-80\end{bmatrix}

are scalar multiples of each other, because each element of v is −20 times the corresponding element of u.

A vector with three elements, like u or v above, may represent a point in three-dimensional space, relative to some Cartesian coordinate system. It helps to think of such a vector as the tip of an arrow whose tail is at the origin of the coordinate system. In this case, the condition "u is parallel to v" means that the two arrows lie on the same straight line, and may differ only in length and direction along that line.

If we multiply any square matrix A with n rows and n columns by such a vector v, the result will be another vector w = A v , also with n rows and one column. That is,

\begin{bmatrix} v_1 \\ v_2 \\ \vdots \\ v_n \end{bmatrix} \quad\quad is mapped to 
\begin{bmatrix} w_1 \\ w_2 \\ \vdots \\ w_n \end{bmatrix}  \;=\;
 \begin{bmatrix} A_{1,1} & A_{1,2} & \ldots & A_{1,n} \\
A_{2,1} & A_{2,2} & \ldots & A_{2,n} \\
\vdots &  \vdots &  \ddots &  \vdots \\
A_{n,1} & A_{n,2} & \ldots & A_{n,n} \\
\end{bmatrix}
\begin{bmatrix} v_1 \\ v_2 \\ \vdots \\ v_n \end{bmatrix}

where, for each index i,

 w_i = A_{i,1} v_1 + A_{i,2} v_2 + \cdots + A_{i,n} v_n = \sum_{j = 1}^{n} A_{i,j} v_j

In general, if v_j are not all zeros, the vectors v and A v will not be parallel. When they are parallel (that is, when there is some real number \lambda such that A v = \lambda v) we say that v is an eigenvector of A. In that case, the scale factor \lambda is said to be the eigenvalue corresponding to that eigenvector.

In particular, multiplication by a 3×3 matrix A may change both the direction and the magnitude of an arrow v in three-dimensional space. However, if v is an eigenvector of A with eigenvalue \lambda, the operation may only change its length, and either keep its direction or flip it (make the arrow point in the exact opposite direction). Specifically, the length of the arrow will increase if |\lambda| > 1, remain the same if |\lambda| = 1, and decrease it if |\lambda|< 1. Moreover, the direction will be precisely the same if \lambda > 0, and flipped if \lambda < 0. If \lambda = 0, then the length of the arrow becomes zero.

An example[edit]

The transformation matrix \bigl[ \begin{smallmatrix} 2 & 1\\ 1 & 2 \end{smallmatrix} \bigr] preserves the angle of arrows parallel to the lines from the origin to \bigl[ \begin{smallmatrix} 1 \\ 1 \end{smallmatrix} \bigr] (in blue) and to \bigl[ \begin{smallmatrix} 1 \\ -1 \end{smallmatrix} \bigr] (in violet). The points that lie on a line through the origin and an eigenvector remain on the line after the transformation. The arrows in red are not parallel to such a line, therefore their angle is altered by the transformation. See also: An extended version, showing all four quadrants.

For the transformation matrix

A = \begin{bmatrix} 3 & 1\\1 & 3 \end{bmatrix},

the vector

v = \begin{bmatrix} 4 \\ -4 \end{bmatrix}

is an eigenvector with eigenvalue 2. Indeed,

A v = \begin{bmatrix} 3 & 1\\1 & 3 \end{bmatrix} \begin{bmatrix} 4 \\ -4 \end{bmatrix} = \begin{bmatrix} 3 \cdot 4 + 1 \cdot (-4) \\ 1 \cdot 4 + 3 \cdot (-4) \end{bmatrix} = \begin{bmatrix} 8 \\ -8 \end{bmatrix} = 2 \cdot \begin{bmatrix} 4 \\ -4 \end{bmatrix}.

On the other hand the vector

v = \begin{bmatrix} 0 \\ 1 \end{bmatrix}

is not an eigenvector, since

\begin{bmatrix} 3 & 1\\1 & 3 \end{bmatrix} \begin{bmatrix} 0 \\ 1 \end{bmatrix} = \begin{bmatrix} 3 \cdot 0 + 1 \cdot 1 \\ 1 \cdot 0 + 3 \cdot 1 \end{bmatrix} = \begin{bmatrix} 1 \\ 3 \end{bmatrix},

and this vector is not a multiple of the original vector v.

Another example[edit]

For the matrix

A= \begin{bmatrix} 1 & 2 & 0\\0 & 2 & 0\\ 0 & 0 & 3\end{bmatrix},

we have

A \begin{bmatrix} 1\\0\\0 \end{bmatrix} = \begin{bmatrix} 1\\0\\0 \end{bmatrix} = 1 \cdot \begin{bmatrix} 1\\0\\0 \end{bmatrix},\quad\quad
A \begin{bmatrix} 0\\0\\1 \end{bmatrix} = \begin{bmatrix} 0\\0\\3 \end{bmatrix} = 3 \cdot \begin{bmatrix} 0\\0\\1 \end{bmatrix}.\quad\quad

Therefore, the vectors [1,0,0]^\mathsf{T} and [0,0,1]^\mathsf{T} are eigenvectors of A corresponding to the eigenvalues 1 and 3 respectively. (Here the symbol {}^\mathsf{T} indicates matrix transposition, in this case turning the row vectors into column vectors.)

Trivial cases[edit]

The identity matrix I (whose general element I_{i j} is 1 if i = j, and 0 otherwise) maps every vector to itself. Therefore, every vector is an eigenvector of I, with eigenvalue 1.

More generally, if A is a diagonal matrix (with A_{i j} = 0 whenever i \neq j), and v is a vector parallel to axis i (that is, v_i \neq 0, and v_j = 0 if j \neq i), then A v = \lambda v where \lambda = A_{i i}. That is, the eigenvalues of a diagonal matrix are the elements of its main diagonal. This is trivially the case of any 1 ×1 matrix.

General definition[edit]

The concept of eigenvectors and eigenvalues extends naturally to abstract linear transformations on abstract vector spaces. Namely, let V be any vector space over some field K of scalars, and let T be a linear transformation mapping V into V. We say that a non-zero vector v of V is an eigenvector of T if (and only if) there is a scalar \lambda in K such that

T(v)=\lambda v.

This equation is called the eigenvalue equation for T, and the scalar \lambda is the eigenvalue of T corresponding to the eigenvector v. Note that T(v) means the result of applying the operator T to the vector v, while \lambda v means the product of the scalar \lambda by v.[3]

The matrix-specific definition is a special case of this abstract definition. Namely, the vector space V is the set of all column vectors of a certain size n×1, and T is the linear transformation that consists in multiplying a vector by the given n\times n matrix A.

Some authors allow v to be the zero vector in the definition of eigenvector.[4] This is reasonable as long as we define eigenvalues and eigenvectors carefully: If we would like the zero vector to be an eigenvector, then we must first define an eigenvalue of  T as a scalar  \lambda in K such that there is a nonzero vector  v in V with  T(v) = \lambda v . We then define an eigenvector to be a vector  v in V such that there is an eigenvalue  \lambda in K with  T(v) = \lambda v . This way, we ensure that it is not the case that every scalar is an eigenvalue corresponding to the zero vector.

Eigenspace and spectrum[edit]

If v is an eigenvector of T, with eigenvalue \lambda, then any scalar multiple \alpha v of v with nonzero \alpha is also an eigenvector with eigenvalue \lambda, since T(\alpha v) = \alpha T(v) = \alpha(\lambda v) = \lambda(\alpha v). Moreover, if u and v are distinct eigenvectors with the same eigenvalue \lambda, then u+v is also an eigenvector with the same eigenvalue \lambda. Therefore, the set of all eigenvectors with the same eigenvalue \lambda, together with the zero vector, is a linear subspace of V, called the eigenspace of T associated to \lambda.[5][6] If that subspace has dimension 1, it is sometimes called an eigenline.[7]

The geometric multiplicity \gamma_T(\lambda) of an eigenvalue \lambda is the dimension of the eigenspace associated to \lambda, i.e. number of linearly independent eigenvectors with that eigenvalue.

The eigenspaces of T always form a direct sum (and as a consequence any family of eigenvectors for different eigenvalues is always linearly independent). Therefore the sum of the dimensions of the eigenspaces cannot exceed the dimension n of the space on which T operates, and in particular there cannot be more than n distinct eigenvalues.[8]

Any subspace spanned by eigenvectors of T is an invariant subspace of T, and the restriction of T to such a subspace is diagonalizable.

The set of eigenvalues of T is sometimes called the spectrum of T.

Eigenbasis[edit]

An eigenbasis for a linear operator T that operates on a vector space V is a basis for V that consists entirely of eigenvectors of T (possibly with different eigenvalues). Such a basis exists precisely if the direct sum of the eigenspaces equals the whole space, in which case one can take the union of bases chosen in each of the eigenspaces as eigenbasis. The matrix of T in a given basis is diagonal precisely when that basis is an eigenbasis for T, and for this reason T is called diagonalizable if it admits an eigenbasis.

Generalizations to infinite-dimensional spaces[edit]

The definition of eigenvalue of a linear transformation T remains valid even if the underlying space V is an infinite dimensional Hilbert or Banach space. Namely, a scalar \lambda is an eigenvalue if and only if there is some nonzero vector v such that T(v) = \lambda v.

Eigenfunctions[edit]

A widely used class of linear operators acting on infinite dimensional spaces are the differential operators on function spaces. Let D be a linear differential operator in on the space \mathbf{C^\infty} of infinitely differentiable real functions of a real argument t. The eigenvalue equation for D is the differential equation

D f = \lambda f

The functions that satisfy this equation are commonly called eigenfunctions of D. For the derivative operator d/dt, an eigenfunction is a function that, when differentiated, yields a constant times the original function. The solution is an exponential function

f(t) = Ae^{\lambda t} ,

including when \lambda is zero when it becomes a constant function. Eigenfunctions are an essential tool in the solution of differential equations and many other applied and theoretical fields. For instance, the exponential functions are eigenfunctions of the shift operators. This is the basis of Fourier transform methods for solving problems.

Spectral theory[edit]

If \lambda is an eigenvalue of T, then the operator T-\lambda I is not one-to-one, and therefore its inverse (T-\lambda I)^{-1} does not exist. The converse is true for finite-dimensional vector spaces, but not for infinite-dimensional ones. In general, the operator T - \lambda I may not have an inverse, even if \lambda is not an eigenvalue.

For this reason, in functional analysis one defines the spectrum of a linear operator T as the set of all scalars \lambda for which the operator T-\lambda I has no bounded inverse. Thus the spectrum of an operator always contains all its eigenvalues, but is not limited to them.

Associative algebras and representation theory[edit]

More algebraically, rather than generalizing the vector space to an infinite dimensional space, one can generalize the algebraic object that is acting on the space, replacing a single operator acting on a vector space with an algebra representation – an associative algebra acting on a module. The study of such actions is the field of representation theory.

A closer analog of eigenvalues is given by the representation-theoretical concept of weight, with the analogs of eigenvectors and eigenspaces being weight vectors and weight spaces.

Eigenvalues and eigenvectors of matrices[edit]

Characteristic polynomial[edit]

The eigenvalue equation for a matrix A is

A v - \lambda v = 0,

which is equivalent to

(A-\lambda I)v = 0,

where I is the n\times n identity matrix. It is a fundamental result of linear algebra that an equation M v = 0 has a non-zero solution v if, and only if, the determinant \det(M) of the matrix M is zero. It follows that the eigenvalues of A are precisely the real numbers \lambda that satisfy the equation

\det(A-\lambda I) = 0

The left-hand side of this equation can be seen (using Leibniz' rule for the determinant) to be a polynomial function of the variable \lambda. The degree of this polynomial is n, the order of the matrix. Its coefficients depend on the entries of A, except that its term of degree n is always (-1)^n\lambda^n. This polynomial is called the characteristic polynomial of A; and the above equation is called the characteristic equation (or, less often, the secular equation) of A.

For example, let A be the matrix

A =
\begin{bmatrix}
2 & 0 & 0 \\
0 & 3 & 4 \\
0 & 4 & 9
\end{bmatrix}

The characteristic polynomial of A is

\det (A-\lambda I) \;=\; \det \left(\begin{bmatrix}
2 & 0 & 0 \\
0 & 3 & 4 \\
0 & 4 & 9
\end{bmatrix} - \lambda
\begin{bmatrix}
1 & 0 & 0 \\
0 & 1 & 0 \\
0 & 0 & 1
\end{bmatrix}\right) \;=\;
\det \begin{bmatrix}
2 - \lambda & 0 & 0 \\
0 & 3 - \lambda & 4 \\
0 & 4 & 9 - \lambda
\end{bmatrix}

which is

 (2 - \lambda) \bigl[ (3 - \lambda) (9 - \lambda) - 16 \bigr] = -\lambda^3 + 14\lambda^2 - 35\lambda + 22

The roots of this polynomial are 2, 1, and 11. Indeed these are the only three eigenvalues of A, corresponding to the eigenvectors [1,0,0]', [0,2,-1]', and [0,1,2]' (or any non-zero multiples thereof).

In the real domain[edit]

Since the eigenvalues are roots of the characteristic polynomial, an n\times n matrix has at most n eigenvalues. If the matrix has real entries, the coefficients of the characteristic polynomial are all real; but it may have fewer than n real roots, or no real roots at all.

For example, consider the cyclic permutation matrix

A = \begin{bmatrix} 0 & 1 & 0\\0 & 0 & 1\\ 1 & 0 & 0\end{bmatrix}

This matrix shifts the coordinates of the vector up by one position, and moves the first coordinate to the bottom. Its characteristic polynomial is 1 - \lambda^3 which has one real root \lambda_1 = 1. Any vector with three equal non-zero elements is an eigenvector for this eigenvalue. For example,


    A \begin{bmatrix} 5\\5\\5 \end{bmatrix} =
    \begin{bmatrix} 5\\5\\5 \end{bmatrix} =
    1 \cdot \begin{bmatrix} 5\\5\\5 \end{bmatrix}

In the complex domain[edit]

The fundamental theorem of algebra implies that the characteristic polynomial of an n\times n matrix A, being a polynomial of degree n, has exactly n complex roots. More precisely, it can be factored into the product of n linear terms,

 \det(A-\lambda I) = (\lambda_1 - \lambda )(\lambda_2 - \lambda)\cdots(\lambda_n - \lambda)

where each \lambda_i is a complex number. The numbers \lambda_1, \lambda_2, ... \lambda_n, (which may not be all distinct) are roots of the polynomial, and are precisely the eigenvalues of A.

Even if the entries of A are all real numbers, the eigenvalues may still have non-zero imaginary parts (and the elements of the corresponding eigenvectors will therefore also have non-zero imaginary parts). Also, the eigenvalues may be irrational numbers even if all the entries of A are rational numbers, or all are integers. However, if the entries of A are algebraic numbers (which include the rationals), the eigenvalues will be (complex) algebraic numbers too.

The non-real roots of a real polynomial with real coefficients can be grouped into pairs of complex conjugate values, namely with the two members of each pair having the same real part and imaginary parts that differ only in sign. If the degree is odd, then by the intermediate value theorem at least one of the roots will be real. Therefore, any real matrix with odd order will have at least one real eigenvalue; whereas a real matrix with even order may have no real eigenvalues.

In the example of the 3×3 cyclic permutation matrix A, above, the characteristic polynomial 1 - \lambda^3 has two additional non-real roots, namely

\lambda_2 = -1/2 + \mathbf{i}\sqrt{3}/2\quad\quad and \quad\quad\lambda_3 = \lambda_2^* = -1/2 - \mathbf{i}\sqrt{3}/2,

where \mathbf{i}= \sqrt{-1} is the imaginary unit. Note that \lambda_2\lambda_3 = 1, \lambda_2^2 = \lambda_3, and \lambda_3^2 = \lambda_2. Then


  A \begin{bmatrix} 1 \\ \lambda_2 \\ \lambda_3 \end{bmatrix} =
   \begin{bmatrix} \lambda_2\\ \lambda_3 \\1 \end{bmatrix} =
   \lambda_2 \cdot \begin{bmatrix} 1\\ \lambda_2 \\ \lambda_3 \end{bmatrix}
   \quad\quad
  and 
   \quad\quad
   A \begin{bmatrix} 1 \\ \lambda_3 \\ \lambda_2 \end{bmatrix} =
   \begin{bmatrix} \lambda_3 \\ \lambda_2 \\ 1 \end{bmatrix} =
   \lambda_3 \cdot \begin{bmatrix} 1 \\ \lambda_3 \\ \lambda_2 \end{bmatrix}

Therefore, the vectors [1,\lambda_2,\lambda_3]' and [1,\lambda_3,\lambda_2]' are eigenvectors of A, with eigenvalues \lambda_2, and \lambda_3, respectively.

Algebraic multiplicities[edit]

Let \lambda_i be an eigenvalue of an n\times n matrix A. The algebraic multiplicity \mu_A(\lambda_i) of \lambda_i is its multiplicity as a root of the characteristic polynomial, that is, the largest integer k such that (\lambda - \lambda_i)^k divides evenly that polynomial.

Like the geometric multiplicity \gamma_A(\lambda_i), the algebraic multiplicity is an integer between 1 and n; and the sum \boldsymbol{\mu}_A of \mu_A(\lambda_i) over all distinct eigenvalues also cannot exceed n. If complex eigenvalues are considered, \boldsymbol{\mu}_A is exactly n.

It can be proved that the geometric multiplicity \gamma_A(\lambda_i) of an eigenvalue never exceeds its algebraic multiplicity \mu_A(\lambda_i). Therefore, \boldsymbol{\gamma}_A is at most \boldsymbol{\mu}_A.

If \gamma_A(\lambda_i) = \mu_A(\lambda_i), then \lambda_i is said to be a semisimple eigenvalue.

Example[edit]

For the matrix: A= \begin{bmatrix}
2 & 0 & 0 & 0 \\
1 & 2 & 0 & 0 \\
0 & 1 & 3 & 0  \\
0 & 0 & 1 & 3  
\end{bmatrix},

the characteristic polynomial of A is \det (A-\lambda I) \;=\;
\det \begin{bmatrix}
2- \lambda & 0 & 0 & 0 \\
1 & 2- \lambda & 0 & 0 \\
0 & 1 & 3- \lambda & 0  \\
0 & 0 & 1 & 3- \lambda  
\end{bmatrix}=  (2 - \lambda)^2 (3 - \lambda)^2 ,
being the product of the diagonal with a lower triangular matrix.

The roots of this polynomial, and hence the eigenvalues, are 2 and 3. The algebraic multiplicity of each eigenvalue is 2; in other words they are both double roots. On the other hand, the geometric multiplicity of the eigenvalue 2 is only 1, because its eigenspace is spanned by the vector [0,1,-1,1], and is therefore 1-dimensional. Similarly, the geometric multiplicity of the eigenvalue 3 is 1 because its eigenspace is spanned by [0,0,0,1]. Hence, the total algebraic multiplicity of A, denoted \mu_A, is 4, which is the most it could be for a 4 by 4 matrix. The geometric multiplicity \gamma_A is 2, which is the smallest it could be for a matrix which has two distinct eigenvalues.

Diagonalization and eigendecomposition[edit]

If the sum \boldsymbol{\gamma}_A of the geometric multiplicities of all eigenvalues is exactly n, then A has a set of n linearly independent eigenvectors. Let Q be a square matrix whose columns are those eigenvectors, in any order. Then we will have A Q = Q\Lambda , where \Lambda is the diagonal matrix such that \Lambda_{i i} is the eigenvalue associated to column i of Q. Since the columns of Q are linearly independent, the matrix Q is invertible. Premultiplying both sides by Q^{-1} we get Q^{-1}A Q = \Lambda. By definition, therefore, the matrix A is diagonalizable.

Conversely, if A is diagonalizable, let Q be a non-singular square matrix such that Q^{-1} A Q is some diagonal matrix D. Multiplying both sides on the left by Q we get A Q = Q D . Therefore each column of Q must be an eigenvector of A, whose eigenvalue is the corresponding element on the diagonal of D. Since the columns of Q must be linearly independent, it follows that \boldsymbol{\gamma}_A = n. Thus \boldsymbol{\gamma}_A is equal to n if and only if A is diagonalizable.

If A is diagonalizable, the space of all n-element vectors can be decomposed into the direct sum of the eigenspaces of A. This decomposition is called the eigendecomposition of A, and it is preserved under change of coordinates.

A matrix that is not diagonalizable is said to be defective. For defective matrices, the notion of eigenvector can be generalized to generalized eigenvectors, and that of diagonal matrix to a Jordan form matrix. Over an algebraically closed field, any matrix A has a Jordan form and therefore admits a basis of generalized eigenvectors, and a decomposition into generalized eigenspaces

Further properties[edit]

Let A be an arbitrary n\times n matrix of complex numbers with eigenvalues \lambda_1, \lambda_2, ... \lambda_n. (Here it is understood that an eigenvalue with algebraic multiplicity \mu occurs \mu times in this list.) Then

  • The trace of A, defined as the sum of its diagonal elements, is also the sum of all eigenvalues:
\operatorname{tr}(A) = \sum_{i=1}^n A_{i i} = \sum_{i=1}^n \lambda_i = \lambda_1+ \lambda_2 +\cdots+ \lambda_n.
  • The determinant of A is the product of all eigenvalues:
\operatorname{det}(A) = \prod_{i=1}^n \lambda_i=\lambda_1\lambda_2\cdots\lambda_n.
  • The eigenvalues of the kth power of A, i.e. the eigenvalues of A^k, for any positive integer k, are \lambda_1^k,\lambda_2^k,\dots,\lambda_n^k
  • The matrix A is invertible if and only if all the eigenvalues \lambda_i are nonzero.
  • If A is invertible, then the eigenvalues of A^{-1} are 1/\lambda_1,1/\lambda_2,\dots,1/\lambda_n
  • If A is equal to its conjugate transpose A^* (in other words, if A is Hermitian), then every eigenvalue is real. The same is true of any a symmetric real matrix. If A is also positive-definite, positive-semidefinite, negative-definite, or negative-semidefinite every eigenvalue is positive, non-negative, negative, or non-positive respectively.
  • Every eigenvalue of a unitary matrix has absolute value |\lambda|=1.

Left and right eigenvectors[edit]

The use of matrices with a single column (rather than a single row) to represent vectors is traditional in many disciplines. For that reason, the word "eigenvector" almost always means a right eigenvector, namely a column vector that must be placed to the right of the matrix A in the defining equation

A v = \lambda v.

There may be also single-row vectors that are unchanged when they occur on the left side of a product with a square matrix A; that is, which satisfy the equation

u A = \lambda u

Any such row vector u is called a left eigenvector of A.

The left eigenvectors of A are transposes of the right eigenvectors of the transposed matrix A^\mathsf{T}, since their defining equation is equivalent to

A^\mathsf{T} u^\mathsf{T}  = \lambda u^\mathsf{T}

It follows that, if A is Hermitian, its left and right eigenvectors are complex conjugates. In particular if A is a real symmetric matrix, they are the same except for transposition.

Variational characterization[edit]

In the Hermitian case, eigenvalues can be given a variational characterization. The largest eigenvalue of  H is the maximum value of the quadratic form  x^T H x/x^T x . A value of  x that realizes that maximum, is an eigenvector. For more information, see Min-max theorem.

Calculation[edit]

Computing the eigenvalues[edit]

The eigenvalues of a matrix A can be determined by finding the roots of the characteristic polynomial. Explicit algebraic formulas for the roots of a polynomial exist only if the degree n is 4 or less. According to the Abel–Ruffini theorem there is no general, explicit and exact algebraic formula for the roots of a polynomial with degree 5 or more.

It turns out that any polynomial with degree n is the characteristic polynomial of some companion matrix of order n. Therefore, for matrices of order 5 or more, the eigenvalues and eigenvectors cannot be obtained by an explicit algebraic formula, and must therefore be computed by approximate numerical methods.

In theory, the coefficients of the characteristic polynomial can be computed exactly, since they are sums of products of matrix elements; and there are algorithms that can find all the roots of a polynomial of arbitrary degree to any required accuracy.[9] However, this approach is not viable in practice because the coefficients would be contaminated by unavoidable round-off errors, and the roots of a polynomial can be an extremely sensitive function of the coefficients (as exemplified by Wilkinson's polynomial).[9]

Efficient, accurate methods to compute eigenvalues and eigenvectors of arbitrary matrices were not known until the advent of the QR algorithm in 1961. [9] Combining the Householder transformation with the LU decomposition results in an algorithm with better convergence than the QR algorithm.[citation needed] For large Hermitian sparse matrices, the Lanczos algorithm is one example of an efficient iterative method to compute eigenvalues and eigenvectors, among several other possibilities.[9]

Computing the eigenvectors[edit]

Once the (exact) value of an eigenvalue is known, the corresponding eigenvectors can be found by finding non-zero solutions of the eigenvalue equation, that becomes a system of linear equations with known coefficients. For example, once it is known that 6 is an eigenvalue of the matrix

A = \begin{bmatrix} 4 & 1\\6 & 3 \end{bmatrix}

we can find its eigenvectors by solving the equation A v = 6 v, that is

\begin{bmatrix} 4 & 1\\6 & 3 \end{bmatrix}\begin{bmatrix}x\\y\end{bmatrix} = 6 \cdot \begin{bmatrix}x\\y\end{bmatrix}

This matrix equation is equivalent to two linear equations


  \left\{\begin{matrix} 4x + {\ }y &{}= 6x\\6x + 3y &{}=6 y\end{matrix}\right.
  \quad\quad\quad that is 
  \left\{\begin{matrix} -2x+ {\ }y &{}=0\\+6x-3y &{}=0\end{matrix}\right.

Both equations reduce to the single linear equation y=2x. Therefore, any vector of the form [a,2a]', for any non-zero real number a, is an eigenvector of A with eigenvalue \lambda = 6.

The matrix A above has another eigenvalue \lambda=1. A similar calculation shows that the corresponding eigenvectors are the non-zero solutions of 3x+y=0, that is, any vector of the form [b,-3b]', for any non-zero real number b.

Some numeric methods that compute the eigenvalues of a matrix also determine a set of corresponding eigenvectors as a by-product of the computation.

History[edit]

Eigenvalues are often introduced in the context of linear algebra or matrix theory. Historically, however, they arose in the study of quadratic forms and differential equations.

In the 18th century Euler studied the rotational motion of a rigid body and discovered the importance of the principal axes. Lagrange realized that the principal axes are the eigenvectors of the inertia matrix.[10] In the early 19th century, Cauchy saw how their work could be used to classify the quadric surfaces, and generalized it to arbitrary dimensions.[11] Cauchy also coined the term racine caractéristique (characteristic root) for what is now called eigenvalue; his term survives in characteristic equation.[12]

Fourier used the work of Laplace and Lagrange to solve the heat equation by separation of variables in his famous 1822 book Théorie analytique de la chaleur.[13] Sturm developed Fourier's ideas further and brought them to the attention of Cauchy, who combined them with his own ideas and arrived at the fact that real symmetric matrices have real eigenvalues.[11] This was extended by Hermite in 1855 to what are now called Hermitian matrices.[12] Around the same time, Brioschi proved that the eigenvalues of orthogonal matrices lie on the unit circle,[11] and Clebsch found the corresponding result for skew-symmetric matrices.[12] Finally, Weierstrass clarified an important aspect in the stability theory started by Laplace by realizing that defective matrices can cause instability.[11]

In the meantime, Liouville studied eigenvalue problems similar to those of Sturm; the discipline that grew out of their work is now called Sturm–Liouville theory.[14] Schwarz studied the first eigenvalue of Laplace's equation on general domains towards the end of the 19th century, while Poincaré studied Poisson's equation a few years later.[15]

At the start of the 20th century, Hilbert studied the eigenvalues of integral operators by viewing the operators as infinite matrices.[16] He was the first to use the German word eigen to denote eigenvalues and eigenvectors in 1904, though he may have been following a related usage by Helmholtz. For some time, the standard term in English was "proper value", but the more distinctive term "eigenvalue" is standard today.[17]

The first numerical algorithm for computing eigenvalues and eigenvectors appeared in 1929, when Von Mises published the power method. One of the most popular methods today, the QR algorithm, was proposed independently by John G.F. Francis[18] and Vera Kublanovskaya[19] in 1961.[20]

Applications[edit]

Eigenvalues of geometric transformations[edit]

The following table presents some example transformations in the plane along with their 2×2 matrices, eigenvalues, and eigenvectors.

scaling unequal scaling rotation horizontal shear hyperbolic rotation
illustration Equal scaling (homothety) Vertical shrink () and horizontal stretch () of a unit square. Rotation by 50 degrees
Horizontal shear mapping
matrix  \begin{bmatrix}k & 0\\0 & k\end{bmatrix}
 
 
 \begin{bmatrix}k_1 & 0\\0 & k_2\end{bmatrix}
 
 
 \begin{bmatrix}c & -s \\ s & c\end{bmatrix}
c=\cos\theta
s=\sin\theta
 \begin{bmatrix}1 & k\\ 0 & 1\end{bmatrix}
 
 
\begin{bmatrix} c & s \\ s & c \end{bmatrix}
c=\cosh \varphi
s=\sinh \varphi
characteristic
polynomial
\ (\lambda - k)^2 (\lambda - k_1)(\lambda - k_2) \lambda^2 - 2c\lambda + 1 \ (\lambda - 1)^2 \lambda^2 - 2c\lambda + 1
eigenvalues \lambda_i \lambda_1 = \lambda_2 = k \lambda_1 = k_1
\lambda_2 = k_2
\lambda_1 = e^{\mathbf{i}\theta}=c+s\mathbf{i}
\lambda_2 = e^{-\mathbf{i}\theta}=c-s\mathbf{i}
\lambda_1 = \lambda_2 = 1 \lambda_1 = e^\varphi
\lambda_2 = e^{-\varphi},
algebraic multipl.
\mu_i=\mu(\lambda_i)
\mu_1 = 2 \mu_1 = 1
\mu_2 = 1
\mu_1 = 1
\mu_2 = 1
\mu_1 = 2 \mu_1 = 1
\mu_2 = 1
geometric multipl.
\gamma_i = \gamma(\lambda_i)
\gamma_1 = 2 \gamma_1 = 1
\gamma_2 = 1
\gamma_1 = 1
\gamma_2 = 1
\gamma_1 = 1 \gamma_1 = 1
\gamma_2 = 1
eigenvectors All non-zero vectors u_1 = \begin{bmatrix}1\\0\end{bmatrix}
u_2 = \begin{bmatrix}0\\1\end{bmatrix}
u_1 = \begin{bmatrix}{\ }1\\-\mathbf{i}\end{bmatrix}
u_2 = \begin{bmatrix}{\ }1\\ +\mathbf{i}\end{bmatrix}
u_1 = \begin{bmatrix}1\\0\end{bmatrix} u_1 = \begin{bmatrix}{\ }1\\{\ }1\end{bmatrix}
u_2 = \begin{bmatrix}{\ }1\\-1\end{bmatrix}.

Note that the characteristic equation for a rotation is a quadratic equation with discriminant D = -4(\sin\theta)^2, which is a negative number whenever \theta is not an integer multiple of 180°. Therefore, except for these special cases, the two eigenvalues are complex numbers, \cos\theta \pm \mathbf{i}\sin\theta; and all eigenvectors have non-real entries. Indeed, except for those special cases, a rotation changes the direction of every nonzero vector in the plane.

Schrödinger equation[edit]

The wavefunctions associated with 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 with eigenvalues interpreted as their energies (increasing downward: n=1,2,3,\ldots) and angular momentum (increasing across: s, p, d, ...). The illustration shows 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 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 where one is interested only in the bound state solutions of the Schrödinger equation, one looks for \psi_E within the space of square integrable functions. Since this space is a Hilbert space with a well-defined scalar product, one 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 one to represent the Schrödinger equation in a matrix form.

The bra–ket notation is often used in this context. A vector, which represents a state of the system, in the Hilbert space of square integrable functions is represented by |\Psi_E\rangle. In this notation, the Schrödinger equation is:

H|\Psi_E\rangle = E|\Psi_E\rangle

where |\Psi_E\rangle is an eigenstate of H. It is a self adjoint operator, the infinite dimensional analog of Hermitian matrices (see Observable). As in the matrix case, in the equation above H|\Psi_E\rangle is understood to be the vector obtained by application of the transformation H to |\Psi_E\rangle.

Molecular orbitals[edit]

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 on the orbitals and their eigenvalues. If one wants to underline this aspect one speaks of nonlinear eigenvalue problem. 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.

Geology and glaciology[edit]

In geology, especially in the study of glacial till, eigenvectors and eigenvalues are used as a method by which a mass of information of a clast fabric's constituents' orientation and dip can be summarized in a 3-D space by six numbers. In the field, a geologist may collect such data for hundreds or thousands of clasts in a soil sample, which can only be compared graphically such as in a Tri-Plot (Sneed and Folk) diagram,[21][22] or as a Stereonet on a Wulff Net.[23]

The output for the orientation tensor is in the three orthogonal (perpendicular) axes of space. The three eigenvectors are ordered v_1, v_2, v_3 by their eigenvalues E_1 \geq E_2 \geq E_3;[24] v_1 then is the primary orientation/dip of clast, v_2 is the secondary and v_3 is the tertiary, in terms of strength. The clast orientation is defined as the direction of the eigenvector, on a compass rose of 360°. Dip is measured as the eigenvalue, the modulus of the tensor: this is valued from 0° (no dip) to 90° (vertical). The relative values of E_1, E_2, and E_3 are dictated by the nature of the sediment's fabric. If E_1 = E_2 = E_3, the fabric is said to be isotropic. If E_1 = E_2 > E_3, the fabric is said to be planar. If E_1 > E_2 > E_3, the fabric is said to be linear.[25]

Principal components analysis[edit]

PCA of the multivariate Gaussian distribution centered at (1,3) with a standard deviation of 3 in roughly the (0.878,0.478) direction and of 1 in the orthogonal direction. The vectors shown are unit eigenvectors of the (symmetric, positive-semidefinite) covariance matrix scaled by the square root of the corresponding eigenvalue. (Just as in the one-dimensional case, the square root is taken because the standard deviation is more readily visualized than the variance.

The eigendecomposition of a symmetric positive semidefinite (PSD) matrix yields an orthogonal basis of eigenvectors, each of which has a nonnegative eigenvalue. The orthogonal decomposition of a PSD matrix is used in multivariate analysis, where the sample covariance matrices are PSD. This orthogonal decomposition is called principal components analysis (PCA) in statistics. PCA studies linear relations among variables. PCA is performed on the covariance matrix or the correlation matrix (in which each variable is scaled to have its sample variance equal to one). For the covariance or correlation matrix, the eigenvectors correspond to principal components and the eigenvalues to the variance explained by the principal components. Principal component analysis of the correlation matrix provides an orthonormal eigen-basis for the space of the observed data: In this basis, the largest eigenvalues correspond to the principal-components that are associated with most of the covariability among a number of observed data.

Principal component analysis is used to study large data sets, such as those encountered in data mining, chemical research, psychology, and in marketing. PCA is popular especially in psychology, in the field of psychometrics. In Q methodology, the eigenvalues of the correlation matrix determine the Q-methodologist's judgment of practical significance (which differs from the statistical significance of hypothesis testing; cf. criteria for determining the number of factors). More generally, principal component analysis can be used as a method of factor analysis in structural equation modeling.

Vibration analysis[edit]

1st lateral bending (See vibration for more types of vibration)

Eigenvalue problems occur naturally in the vibration analysis of mechanical structures with many degrees of freedom. The eigenvalues are used to determine the natural frequencies (or eigenfrequencies) of vibration, and the eigenvectors determine the shapes of these vibrational modes. In particular, undamped vibration is governed by

m\ddot x + kx = 0

or

m\ddot x = -k x

that is, acceleration is proportional to position (i.e., we expect x to be sinusoidal in time).

In n dimensions, m becomes a mass matrix and k a stiffness matrix. Admissible solutions are then a linear combination of solutions to the generalized eigenvalue problem

-k x = \omega^2 m x

where \omega^2 is the eigenvalue and \omega is the angular frequency. Note that the principal vibration modes are different from the principal compliance modes, which are the eigenvectors of k alone. Furthermore, damped vibration, governed by

m\ddot x + c \dot x + kx = 0

leads to what is called a so-called quadratic eigenvalue problem,

(\omega^2 m + \omega c + k)x = 0.

This can be reduced to a generalized eigenvalue problem by clever use of algebra at the cost of solving a larger system.

The orthogonality properties of the eigenvectors allows decoupling of the differential equations so that the system can be represented as linear summation of the eigenvectors. The eigenvalue problem of complex structures is often solved using finite element analysis, but neatly generalize the solution to scalar-valued vibration problems.

Eigenfaces[edit]

Eigenfaces as examples of eigenvectors

In image processing, processed images of faces can be seen as vectors whose components are the brightnesses of each pixel.[26] The dimension of this vector space is the number of pixels. The eigenvectors of the covariance matrix associated with a large set of normalized pictures of faces are called eigenfaces; this is an example of principal components analysis. They are very useful for expressing any face image as a linear combination of some of them. In the facial recognition branch of biometrics, eigenfaces provide a means of applying data compression to faces for identification purposes. Research related to eigen vision systems determining hand gestures has also been made.

Similar to this concept, eigenvoices represent the general direction of variability in human pronunciations of a particular utterance, such as a word in a language. Based on a linear combination of such eigenvoices, a new voice pronunciation of the word can be constructed. These concepts have been found useful in automatic speech recognition systems, for speaker adaptation.

Tensor of moment of inertia[edit]

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

Stress tensor[edit]

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[edit]

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 (see also Discrete Laplace operator), which is either T - A (sometimes called the combinatorial Laplacian) or I - T^{-1/2}A T^{-1/2} (sometimes called the normalized Laplacian), where T is a diagonal matrix with T_{i i} equal to the degree of vertex v_i, and in T^{-1/2}, the ith diagonal entry is 1/\sqrt{\operatorname{deg}(v_i)}. The kth principal eigenvector of a graph is defined as either the eigenvector corresponding to the kth largest or kth smallest eigenvalue of the Laplacian. The first principal eigenvector of the graph is also referred to merely as the principal eigenvector.

The principal eigenvector 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 World Wide Web graph gives the page ranks as its components. This vector corresponds to the stationary distribution of the Markov chain represented by the row-normalized adjacency matrix; however, the adjacency matrix must first be modified to ensure a stationary distribution exists. The second smallest eigenvector can be used to partition the graph into clusters, via spectral clustering. Other methods are also available for clustering.

Basic reproduction number[edit]

See Basic reproduction number

The basic reproduction number (R_0) is a fundamental number in the study of how infectious diseases spread. If one infectious person is put into a population of completely susceptible people, then R_0 is the average number of people that one typical infectious person will infect. The generation time of an infection is the time, t_G, from one person becoming infected to the next person becoming infected. In a heterogeneous population, the next generation matrix defines how many people in the population will become infected after time t_G has passed. R_0 is then the largest eigenvalue of the next generation matrix.[27][28]

See also[edit]

Notes[edit]

  1. ^ a b Wolfram Research, Inc. (2010) Eigenvector. Accessed on 2010-01-29.
  2. ^ William H. Press, Saul A. Teukolsky, William T. Vetterling, Brian P. Flannery (2007), Numerical Recipes: The Art of Scientific Computing, Chapter 11: Eigensystems., pages=563–597. Third edition, Cambridge University Press. ISBN 9780521880688
  3. ^ See Korn & Korn 2000, Section 14.3.5a; Friedberg, Insel & Spence 1989, p. 217
  4. ^ Axler, Sheldon, "Ch. 5", Linear Algebra Done Right (2nd ed.), p. 77 
  5. ^ Shilov 1977, p. 109
  6. ^ Lemma for the eigenspace
  7. ^ Schaum's Easy Outline of Linear Algebra, p. 111
  8. ^ For a proof of this lemma, see Roman 2008, Theorem 8.2 on p. 186; Shilov 1977, p. 109; Hefferon 2001, p. 364; Beezer 2006, Theorem EDELI on p. 469; and Lemma for linear independence of eigenvectors
  9. ^ a b c d Trefethen, Lloyd N.; Bau, David (1997), Numerical Linear Algebra, SIAM 
  10. ^ See Hawkins 1975, §2
  11. ^ a b c d See Hawkins 1975, §3
  12. ^ a b c See Kline 1972, pp. 807–808
  13. ^ See Kline 1972, p. 673
  14. ^ See Kline 1972, pp. 715–716
  15. ^ See Kline 1972, pp. 706–707
  16. ^ See Kline 1972, p. 1063
  17. ^ See Aldrich 2006
  18. ^ Francis, J. G. F. (1961), "The QR Transformation, I (part 1)", The Computer Journal 4 (3): 265–271, doi:10.1093/comjnl/4.3.265  and Francis, J. G. F. (1962), "The QR Transformation, II (part 2)", The Computer Journal 4 (4): 332–345, doi:10.1093/comjnl/4.4.332 
  19. ^ Kublanovskaya, Vera N. (1961), "On some algorithms for the solution of the complete eigenvalue problem", USSR Computational Mathematics and Mathematical Physics 3: 637–657 . Also published in: Zhurnal Vychislitel'noi Matematiki i Matematicheskoi Fiziki 1 (4), 1961: 555–570 
  20. ^ See Golub & van Loan 1996, §7.3; Meyer 2000, §7.3
  21. ^ Graham, D.; Midgley, N. (2000), "Graphical representation of particle shape using triangular diagrams: an Excel spreadsheet method", Earth Surface Processes and Landforms 25 (13): 1473–1477, doi:10.1002/1096-9837(200012)25:13<1473::AID-ESP158>3.0.CO;2-C 
  22. ^ Sneed, E. D.; Folk, R. L. (1958), "Pebbles in the lower Colorado River, Texas, a study of particle morphogenesis", Journal of Geology 66 (2): 114–150, doi:10.1086/626490 
  23. ^ Knox-Robinson, C; Gardoll, Stephen J (1998), "GIS-stereoplot: an interactive stereonet plotting module for ArcView 3.0 geographic information system", Computers & Geosciences 24 (3): 243, doi:10.1016/S0098-3004(97)00122-2 
  24. ^ Stereo32 software
  25. ^ Benn, D.; Evans, D. (2004), A Practical Guide to the study of Glacial Sediments, London: Arnold, pp. 103–107 
  26. ^ Xirouhakis, A.; Votsis, G.; Delopoulus, A. (2004), Estimation of 3D motion and structure of human faces (PDF), Online paper in PDF format, National Technical University of Athens 
  27. ^ Diekmann O, Heesterbeek JAP, Metz JAJ (1990), "On the definition and the computation of the basic reproduction ratio R0 in models for infectious diseases in heterogeneous populations", Journal of Mathematical Biology 28 (4): 365–382, doi:10.1007/BF00178324, PMID 2117040 
  28. ^ Odo Diekmann and J. A. P. Heesterbeek (2000), Mathematical epidemiology of infectious diseases, Wiley series in mathematical and computational biology, West Sussex, England: John Wiley & Sons 

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External links[edit]

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