Vector Space

In mathematics and physics, a vector space (also called a linear space) is a set whose elements, often called ''vectors'', may be added together and multiplied ("scaled") by numbers called '' scalars''. Scalars are often real numbers, but can be complex numbers or, more generally, elements of any field. The operations of vector addition and scalar multiplication must satisfy certain requirements, called ''vector axioms''. The terms real vector space and complex vector space are often used to specify the nature of the scalars: real coordinate space or complex coordinate space.

Vector spaces generalize Euclidean vectors, which allow modeling of physical quantities, such as forces and velocity, that have not only a magnitude, but also a direction. The concept of vector spaces is fundamental for linear algebra, together with the concept of matrix, which allows computing in vector spaces. This provides a concise and synthetic way for manipulating and studying systems of linear equations.

Vector spaces are characterized by their dimension, which, roughly speaking, specifies the number of independent directions in the space. This means that, for two vector spaces with the same dimension, the properties that depend only on the vector-space structure are exactly the same (technically the vector spaces are isomorphic). A vector space is finite-dimensional if its dimension is a natural number. Otherwise, it is infinite-dimensional, and its dimension is an infinite cardinal. Finite-dimensional vector spaces occur naturally in geometry and related areas. Infinite-dimensional vector spaces occur in many areas of mathematics. For example, polynomial rings are countably infinite-dimensional vector spaces, and many function spaces have the cardinality of the continuum as a dimension.

Many vector spaces that are considered in mathematics are also endowed with other structures. This is the case of algebras, which include field extensions, polynomial rings, associative algebras and Lie algebras. This is also the case of topological vector spaces, which include function spaces, inner product spaces, normed spaces, Hilbert spaces and Banach spaces.

Definition and basic properties

In this article, vectors are represented in boldface to distinguish them from scalars.It is also common, especially in physics, to denote vectors with an arrow on top: $\vec v.$ It is also common, especially in higher mathematics, to not use any typographical method for distinguishing vectors from other mathematical objects.

A vector space over a field is a set  together with two binary operations that satisfy the eight axioms listed below. In this context, the elements of are commonly called ''vectors'', and the elements of  are called ''scalars''.

* The first operation, called ''vector addition'' or simply ''addition'' assigns to any two vectors  and in a third vector in which is commonly written as , and called the ''sum'' of these two vectors.
* The second operation, called ''scalar multiplication''，assigns to any scalar  in and any vector  in another vector in , which is denoted .Scalar multiplication is not to be confused with the scalar product, which is an additional operation on some specific vector spaces, called inner product spaces. Scalar multiplication is a multiplication of a vector ''by'' a scalar that produces a vector, while the scalar product is a multiplication of two vectors that produces a scalar.

For having a vector space, the eight following axioms must be satisfied for every , and in , and and in .

When the scalar field is the real numbers the vector space is called a ''real vector space''. When the scalar field is the complex numbers, the vector space is called a ''complex vector space''. These two cases are the most common ones, but vector spaces with scalars in an arbitrary field are also commonly considered. Such a vector space is called an -''vector space'' or a ''vector space over ''.

An equivalent definition of a vector space can be given, which is much more concise but less elementary: the first four axioms (related to vector addition) say that a vector space is an abelian group under addition, and the four remaining axioms (related to the scalar multiplication), say that this operation defines a ring homomorphism from the field into the endomorphism ring of this group.

Subtraction of two vectors can be defined as
: $\mathbf - \mathbf = \mathbf + (-\mathbf).$

Direct consequences of the axioms include that, for every $s\in F$ and $\mathbf v\in V,$ one has
*$0\mathbf v = \mathbf 0,$
*$s\mathbf 0=\mathbf 0,$
*$(-1)\mathbf v = -\mathbf v,$
*$s\mathbf v = \mathbf 0$ implies $s=0$ or $\mathbf v= \mathbf 0.$

Related concepts and properties

; Linear combination
: Given a set of elements of a -vector space , a linear combination of elements of is an element of of the form $a_1 \mathbf_1 + a_2 \mathbf_2 + \cdots + a_k \mathbf_k,$ where $a_1, \ldots, a_k\in F$ and $\mathbf_1, \ldots, \mathbf_k\in G.$ The scalars $a_1, \ldots, a_k$ are called the ''coefficients'' of the linear combination.
;Linear independence
:The elements of a subset of a -vector space are said to be ''linearly independent'' if no element of can be written as a linear combination of the other elements of . Equivalently, they are linearly independent if two linear combinations of element of define the same element of if and only if they have the same coefficients. Also equivalently, they are linearly independent if a linear combination results in the zero vector if and only if all its coefficients are zero.
; Linear subspace
:A ''linear subspace'' or ''vector subspace'' of a vector space is a non-empty subset of that is closed under vector addition and scalar multiplication; that is, the sum of two elements of and the product of an element of by a scalar belong to . This implies that every linear combination of elements of belongs to . A linear subspace is a vector space for the induced addition and scalar multiplication; this means that the closure property implies that the axioms of a vector space are satisfied.
The closure property also implies that ''every intersection of linear subspaces is a linear subspace.''
; Linear span
:Given a subset of a vector space , the ''linear span'' or simply the ''span'' of is the smallest linear subspace of that contains , in the sense that it is the intersection of all linear subspaces that contain . The span of is also the set of all linear combinations of elements of .
If is the span of , one says that ''spans'' or ''generates'' , and that is a ''spanning set'' or a ''generating set'' of .
;Basis and dimension
:A subset of a vector space is a ''basis'' if its elements are linearly independent and span the vector space. Every vector space has at least one basis, generally many (see ). Moreover, all bases of a vector space have the same cardinality, which is called the ''dimension'' of the vector space (see Dimension theorem for vector spaces). This is a fundamental property of vector spaces, which is detailed in the remainder of the section.

''Bases'' are a fundamental tool for the study of vector spaces, especially when the dimension is finite. In the infinite-dimensional case, the existence of infinite bases, often called Hamel bases, depend on the axiom of choice. It follows that, in general, no base can be explicitly described. For example, the real numbers form an infinite-dimensional vector space over the rational numbers, for which no specific basis is known.

Consider a basis $(\mathbf_1, \mathbf_2 , \ldots, \mathbf_n)$ of a vector space of dimension over a field . The definition of a basis implies that every $\mathbf v \in V$ may be written
:$\mathbf v = a_1\mathbf b_1 +\cdots +a_n \mathbf b_n,$
with $a_1,\dots, a_n$ in , and that this decomposition is unique. The scalars $a_1, \ldots, a_n$ are called the ''coordinates'' of on the basis. They are also said to be the ''coefficients'' of the decomposition of on the basis. One also says that the -tuple of the coordinates is the coordinate vector of on the basis, since the set $F^n$ of the -tuples of elements of is a vector space for componentwise addition and scalar multiplication, whose dimension is .

The one-to-one correspondence between vectors and their coordinate vectors maps vector addition to vector addition and scalar multiplication to scalar multiplication. It is thus a vector space isomorphism, which allows translating reasonings and computations on vectors into reasonings and computations on their coordinates. If, in turn, these coordinates are arranged as matrices, these reasonings and computations on coordinates can be expressed concisely as reasonings and computations on matrices. Moreover, a linear equation relating matrices can be expanded into a system of linear equations, and, conversely, every such system can be compacted into a linear equation on matrices.

So, in summary, finite-dimensional linear algebra may be expressed in three equivalent languages:
*''Vector spaces'', which provide concise and coordinate-free statements,
*''Matrices'', which are convenient for expressing concisely explicit computations,
*''Systems of linear equations,'' which provide more elementary formulations.

History

Vector spaces stem from affine geometry, via the introduction of coordinates in the plane or three-dimensional space. Around 1636, French mathematicians René Descartes and Pierre de Fermat founded analytic geometry by identifying solutions to an equation of two variables with points on a plane curve. To achieve geometric solutions without using coordinates, Bolzano introduced, in 1804, certain operations on points, lines and planes, which are predecessors of vectors. introduced the notion of barycentric coordinates. introduced the notion of a bipoint, i.e., an oriented segment one of whose ends is the origin and the other one a target. Vectors were reconsidered with the presentation of complex numbers by Argand and Hamilton and the inception of quaternions by the latter. They are elements in R² and R⁴; treating them using linear combinations goes back to Laguerre in 1867, who also defined systems of linear equations.

In 1857, Cayley introduced the matrix notation which allows for a harmonization and simplification of linear maps. Around the same time, Grassmann studied the barycentric calculus initiated by Möbius. He envisaged sets of abstract objects endowed with operations. In his work, the concepts of linear independence and dimension, as well as scalar products are present. Actually Grassmann's 1844 work exceeds the framework of vector spaces, since his considering multiplication, too, led him to what are today called algebras. Italian mathematician Peano was the first to give the modern definition of vector spaces and linear maps in 1888, although he called them "linear systems".

An important development of vector spaces is due to the construction of function spaces by Henri Lebesgue. This was later formalized by Banach and Hilbert, around 1920. At that time, algebra and the new field of functional analysis began to interact, notably with key concepts such as spaces of ''p''-integrable functions and Hilbert spaces. Also at this time, the first studies concerning infinite-dimensional vector spaces were done.

Examples

Arrows in the plane

The first example of a vector space consists of arrows in a fixed plane, starting at one fixed point. This is used in physics to describe forces or velocities. Given any two such arrows, and , the parallelogram spanned by these two arrows contains one diagonal arrow that starts at the origin, too. This new arrow is called the ''sum'' of the two arrows, and is denoted . In the special case of two arrows on the same line, their sum is the arrow on this line whose length is the sum or the difference of the lengths, depending on whether the arrows have the same direction. Another operation that can be done with arrows is scaling: given any positive real number , the arrow that has the same direction as , but is dilated or shrunk by multiplying its length by , is called ''multiplication'' of by . It is denoted . When is negative, is defined as the arrow pointing in the opposite direction instead.

The following shows a few examples: if , the resulting vector has the same direction as , but is stretched to the double length of (right image below). Equivalently, is the sum . Moreover, has the opposite direction and the same length as (blue vector pointing down in the right image).

Second example: ordered pairs of numbers

A second key example of a vector space is provided by pairs of real numbers and . (The order of the components and is significant, so such a pair is also called an ordered pair.) Such a pair is written as . The sum of two such pairs and multiplication of a pair with a number is defined as follows:

:$(x_1 , y_1) + (x_2 , y_2) = (x_1 + x_2, y_1 + y_2)$

and

:$a(x, y)=(ax, ay) .$

The first example above reduces to this example, if an arrow is represented by a pair of Cartesian coordinates of its endpoint.

Coordinate space

The simplest example of a vector space over a field is the field itself (as it is an abelian group for addition, a part of the requirements to be a field), equipped with its addition (It becomes vector addition.) and multiplication (It becomes scalar multiplication.). More generally, all -tuples (sequences of length )
:
of elements of form a vector space that is usually denoted and called a coordinate space.
The case is the above-mentioned simplest example, in which the field is also regarded as a vector space over itself. The case and (so R²) was discussed in the introduction above.

Complex numbers and other field extensions

The set of complex numbers , that is, numbers that can be written in the form for real numbers and where is the imaginary unit, form a vector space over the reals with the usual addition and multiplication: and for real numbers , , , and . The various axioms of a vector space follow from the fact that the same rules hold for complex number arithmetic.

In fact, the example of complex numbers is essentially the same as (that is, it is ''isomorphic'' to) the vector space of ordered pairs of real numbers mentioned above: if we think of the complex number as representing the ordered pair in the complex plane then we see that the rules for addition and scalar multiplication correspond exactly to those in the earlier example.

More generally, field extensions provide another class of examples of vector spaces, particularly in algebra and algebraic number theory: a field containing a smaller field is an -vector space, by the given multiplication and addition operations of . For example, the complex numbers are a vector space over , and the field extension $\mathbf(i\sqrt)$ is a vector space over .

Function spaces

Functions from any fixed set to a field also form vector spaces, by performing addition and scalar multiplication pointwise. That is, the sum of two functions and is the function given by
:,
and similarly for multiplication. Such function spaces occur in many geometric situations, when is the real line or an interval, or other subsets of . Many notions in topology and analysis, such as continuity, integrability or differentiability are well-behaved with respect to linearity: sums and scalar multiples of functions possessing such a property still have that property. Therefore, the set of such functions are vector spaces, whose study belongs to functional analysis.

Linear equations

Systems of homogeneous linear equations are closely tied to vector spaces. For example, the solutions of
:
are given by triples with arbitrary , , and . They form a vector space: sums and scalar multiples of such triples still satisfy the same ratios of the three variables; thus they are solutions, too. Matrices can be used to condense multiple linear equations as above into one vector equation, namely
:,
where $A = \begin 1 & 3 & 1 \\ 4 & 2 & 2\end$ is the matrix containing the coefficients of the given equations, is the vector , denotes the matrix product, and is the zero vector. In a similar vein, the solutions of homogeneous ''linear differential equations'' form vector spaces. For example,
:
yields , where and are arbitrary constants, and is the natural exponential function.

Linear maps and matrices

The relation of two vector spaces can be expressed by ''linear map'' or ''linear transformation''. They are functions that reflect the vector space structure, that is, they preserve sums and scalar multiplication:
:$f(\mathbf v + \mathbf w) = f(\mathbf v) + f(\mathbf w)$ and for all and in , all in .

An ''isomorphism'' is a linear map such that there exists an inverse map , which is a map such that the two possible compositions and are identity maps. Equivalently, is both one-to-one ( injective) and onto ( surjective). If there exists an isomorphism between and , the two spaces are said to be ''isomorphic''; they are then essentially identical as vector spaces, since all identities holding in are, via , transported to similar ones in , and vice versa via .

For example, the "arrows in the plane" and "ordered pairs of numbers" vector spaces in the introduction are isomorphic: a planar arrow departing at the origin of some (fixed) coordinate system can be expressed as an ordered pair by considering the - and -component of the arrow, as shown in the image at the right. Conversely, given a pair , the arrow going by to the right (or to the left, if is negative), and up (down, if is negative) turns back the arrow .

Linear maps between two vector spaces form a vector space , also denoted , or . The space of linear maps from to is called the ''dual vector space'', denoted . Via the injective natural map , any vector space can be embedded into its ''bidual''; the map is an isomorphism if and only if the space is finite-dimensional.

Once a basis of is chosen, linear maps are completely determined by specifying the images of the basis vectors, because any element of is expressed uniquely as a linear combination of them. If , a 1-to-1 correspondence between fixed bases of and gives rise to a linear map that maps any basis element of to the corresponding basis element of . It is an isomorphism, by its very definition. Therefore, two vector spaces are isomorphic if their dimensions agree and vice versa. Another way to express this is that any vector space is ''completely classified'' ( up to isomorphism) by its dimension, a single number. In particular, any ''n''-dimensional -vector space is isomorphic to . There is, however, no "canonical" or preferred isomorphism; actually an isomorphism is equivalent to the choice of a basis of , by mapping the standard basis of to , via . The freedom of choosing a convenient basis is particularly useful in the infinite-dimensional context; see below.

Matrices

''Matrices'' are a useful notion to encode linear maps. They are written as a rectangular array of scalars as in the image at the right. Any -by- matrix gives rise to a linear map from to , by the following
:$\mathbf x = (x_1, x_2, \ldots, x_n) \mapsto \left(\sum_^n a_x_j, \sum_^n a_x_j, \ldots, \sum_^n a_x_j \right)$, where $\sum$ denotes summation,
or, using the matrix multiplication of the matrix with the coordinate vector :
:.
Moreover, after choosing bases of and , ''any'' linear map is uniquely represented by a matrix via this assignment.

The determinant of a square matrix is a scalar that tells whether the associated map is an isomorphism or not: to be so it is sufficient and necessary that the determinant is nonzero. The linear transformation of corresponding to a real ''n''-by-''n'' matrix is orientation preserving if and only if its determinant is positive.

Eigenvalues and eigenvectors

Endomorphisms, linear maps , are particularly important since in this case vectors can be compared with their image under , . Any nonzero vector satisfying , where is a scalar, is called an ''eigenvector'' of with ''eigenvalue'' .The nomenclature derives from German "eigen", which means own or proper. Equivalently, is an element of the kernel of the difference (where Id is the identity map . If is finite-dimensional, this can be rephrased using determinants: having eigenvalue is equivalent to
:.
By spelling out the definition of the determinant, the expression on the left hand side can be seen to be a polynomial function in , called the characteristic polynomial of . If the field is large enough to contain a zero of this polynomial (which automatically happens for algebraically closed, such as ) any linear map has at least one eigenvector. The vector space may or may not possess an eigenbasis, a basis consisting of eigenvectors. This phenomenon is governed by the Jordan canonical form of the map.See also Jordan–Chevalley decomposition. The set of all eigenvectors corresponding to a particular eigenvalue of forms a vector space known as the ''eigenspace'' corresponding to the eigenvalue (and ) in question. To achieve the spectral theorem, the corresponding statement in the infinite-dimensional case, the machinery of functional analysis is needed, see below.

Basic constructions

In addition to the above concrete examples, there are a number of standard linear algebraic constructions that yield vector spaces related to given ones. In addition to the definitions given below, they are also characterized by universal properties, which determine an object by specifying the linear maps from to any other vector space.

Subspaces and quotient spaces

A nonempty subset ''W'' of a vector space ''V'' that is closed under addition and scalar multiplication (and therefore contains the 0-vector of ''V'') is called a ''linear subspace'' of ''V'', or simply a ''subspace'' of ''V'', when the ambient space is unambiguously a vector space.This is typically the case when a vector space is also considered as an affine space. In this case, a linear subspace contains the zero vector, while an affine subspace does not necessarily contain it. Subspaces of ''V'' are vector spaces (over the same field) in their own right. The intersection of all subspaces containing a given set ''S'' of vectors is called its span, and it is the smallest subspace of ''V'' containing the set ''S''. Expressed in terms of elements, the span is the subspace consisting of all the linear combinations of elements of ''S''.

A linear subspace of dimension 1 is a vector line. A linear subspace of dimension 2 is a vector plane. A linear subspace that contains all elements but one of a basis of the ambient space is a vector hyperplane. In a vector space of finite dimension , a vector hyperplane is thus a subspace of dimension .

The counterpart to subspaces are ''quotient vector spaces''. Given any subspace , the quotient space ''V''/''W'' ("''V'' modulo ''W''") is defined as follows: as a set, it consists of where v is an arbitrary vector in ''V''. The sum of two such elements and is and scalar multiplication is given by . The key point in this definition is that if and only if the difference of v₁ and v₂ lies in ''W''.Some authors (such as ) choose to start with this equivalence relation and derive the concrete shape of ''V''/''W'' from this. This way, the quotient space "forgets" information that is contained in the subspace ''W''.

The kernel ker(''f'') of a linear map consists of vectors v that are mapped to 0 in ''W''. The kernel and the image are subspaces of ''V'' and ''W'', respectively. The existence of kernels and images is part of the statement that the category of vector spaces (over a fixed field ''F'') is an abelian category, that is, a corpus of mathematical objects and structure-preserving maps between them (a category) that behaves much like the category of abelian groups. Because of this, many statements such as the first isomorphism theorem (also called rank–nullity theorem in matrix-related terms)
:''V'' / ker(''f'') ≡ im(''f'').
and the second and third isomorphism theorem can be formulated and proven in a way very similar to the corresponding statements for groups.

An important example is the kernel of a linear map for some fixed matrix ''A'', as above. The kernel of this map is the subspace of vectors x such that , which is precisely the set of solutions to the system of homogeneous linear equations belonging to ''A''. This concept also extends to linear differential equations
:$a_0 f + a_1 \frac + a_2 \frac + \cdots + a_n \frac = 0$, where the coefficients ''a''_''i'' are functions in ''x'', too.
In the corresponding map
:$f \mapsto D(f) = \sum_^n a_i \frac$,
the derivatives of the function ''f'' appear linearly (as opposed to ''f''′′(''x'')², for example). Since differentiation is a linear procedure (that is, and for a constant ) this assignment is linear, called a linear differential operator. In particular, the solutions to the differential equation form a vector space (over or ).

Direct product and direct sum

The ''direct product'' of vector spaces and the ''direct sum'' of vector spaces are two ways of combining an indexed family of vector spaces into a new vector space.

The ''direct product'' $\textstyle$ of a family of vector spaces ''V''_''i'' consists of the set of all tuples (, which specify for each index ''i'' in some index set ''I'' an element v_''i'' of ''V''_''i''. Addition and scalar multiplication is performed componentwise. A variant of this construction is the ''direct sum'' $\bigoplus_ V_i$ (also called coproduct and denoted $\coprod_V_i$), where only tuples with finitely many nonzero vectors are allowed. If the index set ''I'' is finite, the two constructions agree, but in general they are different.

Tensor product

The ''tensor product'' , or simply , of two vector spaces ''V'' and ''W'' is one of the central notions of multilinear algebra which deals with extending notions such as linear maps to several variables. A map is called bilinear if ''g'' is linear in both variables v and w. That is to say, for fixed w the map is linear in the sense above and likewise for fixed v.

The tensor product is a particular vector space that is a ''universal'' recipient of bilinear maps ''g'', as follows. It is defined as the vector space consisting of finite (formal) sums of symbols called tensors
:v₁ ⊗ w₁ + v₂ ⊗ w₂ + ⋯ + v_''n'' ⊗ w_''n'',
subject to the rules
: ''a'' · (v ⊗ w) = (''a'' · v) ⊗ w = v ⊗ (''a'' · w), where ''a'' is a scalar,
:(v₁ + v₂) ⊗ w = v₁ ⊗ w + v₂ ⊗ w, and
:v ⊗ (w₁ + w₂) = v ⊗ w₁ + v ⊗ w₂.

These rules ensure that the map ''f'' from the to that maps a tuple to is bilinear. The universality states that given ''any'' vector space ''X'' and ''any'' bilinear map , there exists a unique map ''u'', shown in the diagram with a dotted arrow, whose composition with ''f'' equals ''g'': . This is called the universal property of the tensor product, an instance of the method—much used in advanced abstract algebra—to indirectly define objects by specifying maps from or to this object.

Vector spaces with additional structure

From the point of view of linear algebra, vector spaces are completely understood insofar as any vector space is characterized, up to isomorphism, by its dimension. However, vector spaces ''per se'' do not offer a framework to deal with the question—crucial to analysis—whether a sequence of functions converges to another function. Likewise, linear algebra is not adapted to deal with infinite series, since the addition operation allows only finitely many terms to be added. Therefore, the needs of functional analysis require considering additional structures.

A vector space may be given a partial order ≤, under which some vectors can be compared. For example, ''n''-dimensional real space R^''n'' can be ordered by comparing its vectors componentwise. Ordered vector spaces, for example Riesz spaces, are fundamental to Lebesgue integration, which relies on the ability to express a function as a difference of two positive functions
:$f = f^ - f^$,
where $f^$ denotes the positive part of $f$ and $f^$ the negative part.

Normed vector spaces and inner product spaces

"Measuring" vectors is done by specifying a norm, a datum which measures lengths of vectors, or by an inner product, which measures angles between vectors. Norms and inner products are denoted $, \mathbf v,$ and respectively. The datum of an inner product entails that lengths of vectors can be defined too, by defining the associated norm Vector spaces endowed with such data are known as ''normed vector spaces'' and ''inner product spaces'', respectively.

Coordinate space ''F''^''n'' can be equipped with the standard dot product:
:$\lang \mathbf x , \mathbf y \rang = \mathbf x \cdot \mathbf y = x_1 y_1 + \cdots + x_n y_n.$
In R², this reflects the common notion of the angle between two vectors x and y, by the law of cosines:
:$\mathbf x \cdot \mathbf y = \cos\left(\angle (\mathbf x, \mathbf y)\right) \cdot , \mathbf x, \cdot , \mathbf y, .$
Because of this, two vectors satisfying $\lang \mathbf x , \mathbf y \rang = 0$ are called orthogonal. An important variant of the standard dot product is used in Minkowski space: R⁴ endowed with the Lorentz product
:$\lang \mathbf x , \mathbf y \rang = x_1 y_1 + x_2 y_2 + x_3 y_3 - x_4 y_4.$
In contrast to the standard dot product, it is not positive definite: $\lang \mathbf x , \mathbf x \rang$ also takes negative values, for example, for $\mathbf x = (0, 0, 0, 1)$. Singling out the fourth coordinate— corresponding to time, as opposed to three space-dimensions—makes it useful for the mathematical treatment of special relativity.

Topological vector spaces

Convergence questions are treated by considering vector spaces ''V'' carrying a compatible topology, a structure that allows one to talk about elements being close to each other. Compatible here means that addition and scalar multiplication have to be continuous maps. Roughly, if x and y in ''V'', and ''a'' in ''F'' vary by a bounded amount, then so do and .This requirement implies that the topology gives rise to a uniform structure, To make sense of specifying the amount a scalar changes, the field ''F'' also has to carry a topology in this context; a common choice are the reals or the complex numbers.

In such ''topological vector spaces'' one can consider series of vectors. The infinite sum
:$\sum_^ f_i$
denotes the limit of the corresponding finite partial sums of the sequence (''f''_''i'')_''i''∈N of elements of ''V''. For example, the ''f''_''i'' could be (real or complex) functions belonging to some function space ''V'', in which case the series is a function series. The mode of convergence of the series depends on the topology imposed on the function space. In such cases, pointwise convergence and uniform convergence are two prominent examples.

A way to ensure the existence of limits of certain infinite series is to restrict attention to spaces where any Cauchy sequence has a limit; such a vector space is called complete. Roughly, a vector space is complete provided that it contains all necessary limits. For example, the vector space of polynomials on the unit interval ,1 equipped with the topology of uniform convergence is not complete because any continuous function on ,1can be uniformly approximated by a sequence of polynomials, by the Weierstrass approximation theorem. In contrast, the space of ''all'' continuous functions on ,1with the same topology is complete. A norm gives rise to a topology by defining that a sequence of vectors v_''n'' converges to v if and only if
:$\lim_ , \mathbf v_n - \mathbf v, = 0.$
Banach and Hilbert spaces are complete topological vector spaces whose topologies are given, respectively, by a norm and an inner product. Their study—a key piece of functional analysis—focuses on infinite-dimensional vector spaces, since all norms on finite-dimensional topological vector spaces give rise to the same notion of convergence. The image at the right shows the equivalence of the 1-norm and ∞-norm on R²: as the unit "balls" enclose each other, a sequence converges to zero in one norm if and only if it so does in the other norm. In the infinite-dimensional case, however, there will generally be inequivalent topologies, which makes the study of topological vector spaces richer than that of vector spaces without additional data.

From a conceptual point of view, all notions related to topological vector spaces should match the topology. For example, instead of considering all linear maps (also called functionals) , maps between topological vector spaces are required to be continuous. In particular, the (topological) dual space consists of continuous functionals (or to ). The fundamental Hahn–Banach theorem is concerned with separating subspaces of appropriate topological vector spaces by continuous functionals.

Banach spaces

''Banach spaces'', introduced by Stefan Banach, are complete normed vector spaces.

A first example is the vector space $\ell^p$ consisting of infinite vectors with real entries
$\mathbf = \left(x_1, x_2, \ldots, x_n, \ldots\right)$
whose $p$-norm
$(1\leq\leq\infty)$
given by
:$\left\, \mathbf\right\, _p := \left(\sum_i \left\vert x_i\right\vert^p\right)^\frac$ for $p < \infty$   and   $\left\, \mathbf x\right\, _ := \sup_i \left, x_i \$.

The topologies on the infinite-dimensional space $\ell^p$
are inequivalent for different $p$. For example, the sequence of vectors
$\mathbf_n = \left(2^, 2^, \ldots, 2^, 0, 0, \ldots\right)$,
in which the first $2^n$ components are $2^$ and the following ones are $0$, converges to the zero vector for
$p = \infty$,
but does not for
$p = 1$:
:$\left\Vert\mathbf_\right\Vert_ = \sup (2^, 0) = 2^ \rightarrow 0$, but $\left\Vert\mathbf_\right\Vert_ = \sum_^ 2^ = 2^n \cdot 2^ = 1.$

More generally than sequences of real numbers, functions
$f\colon \Omega \to \mathbb$
are endowed with a norm that replaces the above sum by the Lebesgue integral
:$\left\Vert\right\Vert_ := \left( \int_ \left\vert\left(x\right)\right\vert^ \, \right)^\frac.$

The space of integrable functions on a given domain
$\Omega$ (for example an interval) satisfying
$\left\Vert\right\Vert_ < \infty$,
and equipped with this norm are called Lebesgue spaces, denoted $L^\left(\Omega\right)$.The triangle inequality for
$\left\Vert\right\Vert_ \leq \left\Vert\right\Vert_ + \left\Vert\right\Vert_$
is provided by the Minkowski inequality. For technical reasons, in the context of functions one has to identify functions that agree almost everywhere to get a norm, and not only a seminorm.

These spaces are complete. (If one uses the Riemann integral instead, the space is ''not'' complete, which may be seen as a justification for Lebesgue's integration theory.
"Many functions in
$L^$
of Lebesgue measure, being unbounded, cannot be integrated with the classical Riemann integral. So spaces of Riemann integrable functions would not be complete in the
$L^$
norm, and the orthogonal decomposition would not apply to them. This shows one of the advantages of Lebesgue integration.",
) Concretely this means that for any sequence of Lebesgue-integrable functions  
$f_, f_, \ldots, f_, \ldots$  
with
$\left\Vert_\right\Vert_<\infty$,
satisfying the condition
:$\lim_\int_ \left\vert_(x) - _(x)\right\vert^ \, = 0$

there exists a function $\left(x\right)$ belonging to the vector space $L^\left(\Omega\right)$ such that
:$\lim_\int_ \left\vert\left(x\right) - _\left(x\right)\right\vert^ \, = 0.$

Imposing boundedness conditions not only on the function, but also on its derivatives leads to Sobolev spaces.

Hilbert spaces

Complete inner product spaces are known as ''Hilbert spaces'', in honor of David Hilbert. The Hilbert space ''L''²(Ω), with inner product given by
:$\langle f\ , \ g \rangle = \int_\Omega f(x) \overline \, dx,$
where $\overline$ denotes the complex conjugate of ''g''(''x''),For ''p'' ≠2, ''L''^''p''(Ω) is not a Hilbert space. is a key case.

By definition, in a Hilbert space any Cauchy sequence converges to a limit. Conversely, finding a sequence of functions ''f''_''n'' with desirable properties that approximates a given limit function, is equally crucial. Early analysis, in the guise of the Taylor approximation, established an approximation of differentiable functions ''f'' by polynomials. By the Stone–Weierstrass theorem, every continuous function on can be approximated as closely as desired by a polynomial. A similar approximation technique by trigonometric functions is commonly called Fourier expansion, and is much applied in engineering, see below. More generally, and more conceptually, the theorem yields a simple description of what "basic functions", or, in abstract Hilbert spaces, what basic vectors suffice to generate a Hilbert space ''H'', in the sense that the '' closure'' of their span (that is, finite linear combinations and limits of those) is the whole space. Such a set of functions is called a ''basis'' of ''H'', its cardinality is known as the Hilbert space dimension.A basis of a Hilbert space is not the same thing as a basis in the sense of linear algebra above. For distinction, the latter is then called a Hamel basis. Not only does the theorem exhibit suitable basis functions as sufficient for approximation purposes, but also together with the Gram–Schmidt process, it enables one to construct a basis of orthogonal vectors. Such orthogonal bases are the Hilbert space generalization of the coordinate axes in finite-dimensional Euclidean space.

The solutions to various differential equations can be interpreted in terms of Hilbert spaces. For example, a great many fields in physics and engineering lead to such equations and frequently solutions with particular physical properties are used as basis functions, often orthogonal. As an example from physics, the time-dependent Schrödinger equation in quantum mechanics describes the change of physical properties in time by means of a partial differential equation, whose solutions are called wavefunctions. Definite values for physical properties such as energy, or momentum, correspond to eigenvalues of a certain (linear) differential operator and the associated wavefunctions are called eigenstates. The spectral theorem decomposes a linear compact operator acting on functions in terms of these eigenfunctions and their eigenvalues.

Algebras over fields

General vector spaces do not possess a multiplication between vectors. A vector space equipped with an additional bilinear operator defining the multiplication of two vectors is an ''algebra over a field''. Many algebras stem from functions on some geometrical object: since functions with values in a given field can be multiplied pointwise, these entities form algebras. The Stone–Weierstrass theorem, for example, relies on Banach algebras which are both Banach spaces and algebras.

Commutative algebra makes great use of rings of polynomials in one or several variables, introduced above. Their multiplication is both commutative and associative. These rings and their quotients form the basis of algebraic geometry, because they are rings of functions of algebraic geometric objects.

Another crucial example are ''Lie algebras'', which are neither commutative nor associative, but the failure to be so is limited by the constraints ( denotes the product of and ):
* (anticommutativity), and
* (Jacobi identity).
Examples include the vector space of ''n''-by-''n'' matrices, with , the commutator of two matrices, and , endowed with the cross product.

The tensor algebra T(''V'') is a formal way of adding products to any vector space ''V'' to obtain an algebra. As a vector space, it is spanned by symbols, called simple tensors
:, where the degree varies.
The multiplication is given by concatenating such symbols, imposing the distributive law under addition, and requiring that scalar multiplication commute with the tensor product ⊗, much the same way as with the tensor product of two vector spaces introduced above. In general, there are no relations between and . Forcing two such elements to be equal leads to the symmetric algebra, whereas forcing yields the exterior algebra.

When a field, is explicitly stated, a common term used is -algebra.

Related structures

Vector bundles

A ''vector bundle'' is a family of vector spaces parametrized continuously by a topological space ''X''. More precisely, a vector bundle over ''X'' is a topological space ''E'' equipped with a continuous map
:Ï€ : ''E'' → ''X''
such that for every ''x'' in ''X'', the fiber Ï€^−1(''x'') is a vector space. The case dim is called a line bundle. For any vector space ''V'', the projection makes the product into a "trivial" vector bundle. Vector bundles over ''X'' are required to be locally a product of ''X'' and some (fixed) vector space ''V'': for every ''x'' in ''X'', there is a neighborhood ''U'' of ''x'' such that the restriction of Ï€ to Ï€^−1(''U'') is isomorphicThat is, there is a homeomorphism from Ï€^−1(''U'') to which restricts to linear isomorphisms between fibers. to the trivial bundle . Despite their locally trivial character, vector bundles may (depending on the shape of the underlying space ''X'') be "twisted" in the large (that is, the bundle need not be (globally isomorphic to) the trivial bundle ). For example, the Möbius strip can be seen as a line bundle over the circle ''S''¹ (by identifying open intervals with the real line). It is, however, different from the cylinder , because the latter is orientable whereas the former is not.

Properties of certain vector bundles provide information about the underlying topological space. For example, the tangent bundle consists of the collection of tangent spaces parametrized by the points of a differentiable manifold. The tangent bundle of the circle ''S''¹ is globally isomorphic to , since there is a global nonzero vector field on ''S''¹.A line bundle, such as the tangent bundle of ''S''¹ is trivial if and only if there is a section that vanishes nowhere, see . The sections of the tangent bundle are just vector fields. In contrast, by the hairy ball theorem, there is no (tangent) vector field on the 2-sphere ''S''² which is everywhere nonzero. K-theory studies the isomorphism classes of all vector bundles over some topological space. In addition to deepening topological and geometrical insight, it has purely algebraic consequences, such as the classification of finite-dimensional real division algebras: R, C, the quaternions H and the octonions O.

The cotangent bundle of a differentiable manifold consists, at every point of the manifold, of the dual of the tangent space, the cotangent space. Sections of that bundle are known as differential one-forms.

Modules

''Modules'' are to rings what vector spaces are to fields: the same axioms, applied to a ring ''R'' instead of a field ''F'', yield modules. The theory of modules, compared to that of vector spaces, is complicated by the presence of ring elements that do not have multiplicative inverses. For example, modules need not have bases, as the Z-module (that is, abelian group) Z/2Z shows; those modules that do (including all vector spaces) are known as free modules. Nevertheless, a vector space can be compactly defined as a module over a ring which is a field, with the elements being called vectors. Some authors use the term ''vector space'' to mean modules over a division ring. The algebro-geometric interpretation of commutative rings via their spectrum allows the development of concepts such as locally free modules, the algebraic counterpart to vector bundles.

Affine and projective spaces

Roughly, ''affine spaces'' are vector spaces whose origins are not specified. More precisely, an affine space is a set with a free transitive vector space action. In particular, a vector space is an affine space over itself, by the map
:.
If ''W'' is a vector space, then an affine subspace is a subset of ''W'' obtained by translating a linear subspace ''V'' by a fixed vector ; this space is denoted by (it is a coset of ''V'' in ''W'') and consists of all vectors of the form for An important example is the space of solutions of a system of inhomogeneous linear equations
:
generalizing the homogeneous case above, which can be found by setting in this equation. The space of solutions is the affine subspace where x is a particular solution of the equation, and ''V'' is the space of solutions of the homogeneous equation (the nullspace of ''A'').

The set of one-dimensional subspaces of a fixed finite-dimensional vector space ''V'' is known as ''projective space''; it may be used to formalize the idea of parallel lines intersecting at infinity. Grassmannians and flag manifolds generalize this by parametrizing linear subspaces of fixed dimension ''k'' and flags of subspaces, respectively.

Related concepts

;Specific vectors in a vector space
* Zero vector (sometimes also called ''null vector'' and denoted by $\mathbf$), the additive identity in a vector space. In a normed vector space, it is the unique vector of norm zero. In a Euclidean vector space, it is the unique vector of length zero.
* Basis vector, an element of a given basis of a vector space.
* Unit vector, a vector in a normed vector space whose norm is 1, or a Euclidean vector of length one.
* Isotropic vector or null vector, in a vector space with a quadratic form, a non-zero vector for which the form is zero. If a null vector exists, the quadratic form is said an isotropic quadratic form.

;Vectors in specific vector spaces
* Column vector, a matrix with only one column. The column vectors with a fixed number of rows form a vector space.
* Row vector, a matrix with only one row. The row vectors with a fixed number of columns form a vector space.
* Coordinate vector, the -tuple of the coordinates of a vector on a basis of elements. For a vector space over a field , these -tuples form the vector space $F^n$ (where the operation are pointwise addition and scalar multiplication).
* Displacement vector, a vector that specifies the change in position of a point relative to a previous position. Displacement vectors belong to the vector space of translations.
* Position vector of a point, the displacement vector from a reference point (called the ''origin'') to the point. A position vector represents the position of a point in a Euclidean space or an affine space.
* Velocity vector, the derivative, with respect to time, of the position vector. It does not depend of the choice of the origin, and, thus belongs to the vector space of translations.
* Pseudovector, also called ''axial vector''
* Covector, an element of the dual of a vector space. In an inner product space, the inner product defines an isomorphism between the space and its dual, which may make difficult to distinguish a covector from a vector. The distinction becomes apparent when one changes coordinates (non-orthogonally).
* Tangent vector, an element of the tangent space of a curve, a surface or, more generally, a differential manifold at a given point (these tangent spaces are naturally endowed with a structure of vector space)
* Normal vector or simply ''normal'', in a Euclidean space or, more generally, in an inner product space, a vector that is perpendicular to a tangent space at a point.
* Gradient, the coordinates vector of the partial derivatives of a function of several real variables. In a Euclidean space the gradient gives the magnitude and direction of maximum increase of a scalar field. The gradient is a covector that is normal to a level curve.
* Four-vector, in the theory of relativity, a vector in a four-dimensional real vector space called Minkowski space

See also

*Vector (mathematics and physics), for a list of various kinds of vectors

* Cartesian coordinate system
* Graded vector space
*Metric space
*P-vector
*Riesz–Fischer theorem
* Space (mathematics)
*Ordered vector space

Notes

Citations

References

Algebra

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Analysis

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Historical references

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* Peano, G. (1901) Formulario mathematico

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