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In [[mathematical analysis]], a [[metric space]] ''M'' is called '''complete''' (or a '''Cauchy space''') if every [[Cauchy sequence]] of points in ''M'' has a [[limit of a sequence|limit]] that is also in ''M'' or, alternatively, if every Cauchy sequence in ''M'' converges in ''M''.
 
Intuitively, a space is complete if there are no "points missing" from it (inside or at the boundary). For instance, the set of [[rational number]]s is not complete, because e.g. [[square root of 2|{{sqrt|2}}]] is "missing" from it, even though one can construct a Cauchy sequence of rational numbers that converges to it. (See the examples below.)  It is always possible to "fill all the holes", leading to the ''completion'' of a given space, as explained below.
 
== Examples ==
The space '''Q''' of [[rational number]]s, with the standard metric given by the [[absolute value]] of the [[subtraction|difference]], is not complete. Consider for instance the sequence defined by <math>\scriptstyle x_1 \;=\; 1</math> and <math>\scriptstyle x_{n+1} \;=\; \frac{x_n}{2} \,+\, \frac{1}{x_n}</math>. This is a Cauchy sequence of rational numbers, but it does not converge towards any rational limit: If the sequence did have a limit ''x'', then necessarily ''x''<sup>2</sup>&nbsp;=&nbsp;2, yet no rational number has this property. However, considered as a sequence of [[real number]]s, it does converge to the [[irrational number]] {{sqrt|2}}.
 
The [[interval (mathematics)|open interval]] {{open-open|0,1}}, again with the absolute value metric, is not complete either. The sequence defined by ''x''<sub>''n''</sub> = {{sfrac|1|''n''}} is Cauchy, but does not have a limit in the given space. However the closed interval [[unit interval|{{closed-closed|0,1}}]] is complete; the given sequence does have a limit in this interval and the limit is zero.
 
The space '''R''' of real numbers and the space '''C''' of [[complex number]]s (with the metric given by the absolute value) are complete, and so is [[Euclidean space]] '''R'''<sup>''n''</sup>, with the [[Euclidean distance|usual distance]] metric.  In contrast, infinite-dimensional [[normed vector space]]s may or may not be complete; those that are complete are [[Banach space]]s. The space C{{closed-closed|''a'', ''b''}} of [[continuous functions on a compact Hausdorff space|continuous real-valued functions on a closed and bounded interval]] is a Banach space, and so a complete metric space, with respect to the [[supremum norm]]. However, the supremum norm does not give a norm on the space C{{open-open|''a'', ''b''}} of continuous functions on {{open-open|''a'', ''b''}}, for it may contain unbounded functions. Instead, with the topology of [[compact convergence]], C{{open-open|''a'', ''b''}} can be given the structure of a [[Fréchet space]]: a [[locally convex topological vector space]] whose topology can be induced by a complete translation-invariant metric.
 
The space '''Q'''<sub>''p''</sub> of [[p-adic number|''p''-adic number]]s is complete for any [[prime number]] ''p''. This space completes '''Q''' with the ''p''-adic metric in the same way that '''R''' completes '''Q''' with the usual metric.
 
If ''S'' is an arbitrary set, then the set ''S''<sup>'''N'''</sup> of all [[sequence]]s in ''S'' becomes a complete metric space if we define the distance between the sequences (''x''<sub>''n''</sub>) and (''y''<sub>''n''</sub>) to be {{sfrac|1|''N''}}, where ''N'' is the smallest index for which ''x''<sub>''N''</sub> is [[distinct]] from ''y''<sub>''N''</sub>, or 0 if there is no such index.  This space is [[homeomorphic]] to the [[product topology|product]] of a [[countable]] number of copies of the [[discrete space]] ''S''.
 
==Some theorems==
A metric space ''X'' is complete if and only if every decreasing sequence of non-empty closed subsets of ''X'', with [[Diameter#Generalisations|diameters]] tending to&nbsp;0, has a non-empty intersection: if ''F''<sub>''n''</sub> is closed and non-empty, {{nowrap|''F''<sub>''n'' + 1</sub> &sub; ''F''<sub>''n''</sub>}} for every ''n'',  and diam(''F''<sub>''n''</sub>)&nbsp;→&nbsp;0, then there is a point ''x''&nbsp;∈&nbsp;''X'' common to all sets&nbsp;''F''<sub>''n''</sub>.
 
Every [[compact space|compact]] metric space is complete, though complete spaces need not be compact. In fact, a metric space is compact [[if and only if]] it is complete and [[totally bounded]]. This is a generalization of the [[Heine–Borel theorem]], which states that any closed and bounded subspace ''S'' of '''R'''<sup>''n''</sup> is compact and therefore complete.<ref>Introduction to Metric and Topological Spaces, Wilson A. Sutherland, ISBN 978-0-19-853161-6</ref>
 
A closed subspace of a complete space is complete.<ref>http://planetmath.org/encyclopedia/AClosedSubsetOfACompleteMetricSpaceIsComplete.html</ref> Conversely, a complete subset of a metric space is closed.<ref>http://planetmath.org/encyclopedia/ACompleteSubspaceOfAMetricSpaceIsClosed.html</ref>
 
If ''X'' is a [[Set (mathematics)|set]] and ''M'' is a complete metric space, then the set B(''X'',&#8239;''M'') of all [[bounded function]]s ''f'' from ''X'' to ''M'' is a complete metric space. Here we define the distance in B(''X'',&#8239;''M'') in terms of the distance in ''M'' with the [[supremum norm]]
 
:<math>d(f, g) \equiv \sup\left\{d[f(x), g(x)]: x \in X \right\}</math>
 
If ''X'' is a [[topological space]] and ''M'' is a complete metric space, then the set C<sub>b</sub>(''X'',&#8239;''M'') consisting of all [[continuous function (topology)|continuous]] bounded functions ''f'' from ''X'' to ''M'' is a closed subspace of B(''X'',&#8239;''M'') and hence also complete.
 
The [[Baire category theorem]] says that every complete metric space is a [[Baire space]]. That is, the [[union (set theory)|union]] of [[countable|countably many]] [[nowhere dense]] subsets of the space has [[empty set|empty]] [[interior (topology)|interior]].
 
The [[Banach fixed point theorem]] states that a contraction mapping on a complete metric space admits a fixed point. The fixed point theorem is often used to prove the [[inverse function theorem]] on complete metric spaces such as Banach spaces.
 
The [[expansion constant]] of a metric space is the [[infimum]] of all constants <math>\scriptstyle \mu</math> such that whenever the family <math>\scriptstyle \left\{ \overline{B}(x_\alpha,\, r_\alpha) \right\}</math> intersects pairwise, the intersection
:<math>\bigcap_\alpha \overline{B}(x_\alpha, \mu r_\alpha)</math>
 
is nonempty. A metric space is complete if and only if its expansion constant is ≤&nbsp;2.<ref>B. Grünbaum, ''[http://projecteuclid.org/DPubS/Repository/1.0/Disseminate?view=body&id=pdf_1&handle=euclid.pjm/1103038634 Some applications of expansion constants.]'' Pacific J. Math. Volume 10, Number 1 (1960), 193–201.</ref>
 
==Completion==
For any metric space ''M'', one can construct a complete metric space ''M′'' (which is also denoted as {{overline|M}}), which contains ''M'' as a [[dense subspace]]. It has the following [[universal property]]: if ''N'' is any complete metric space and ''f'' is any [[uniformly continuous function]] from ''M'' to ''N'', then there exists a [[unique]] uniformly continuous function ''f′'' from ''M′'' to ''N'', which extends ''f''. The space ''M''' is determined [[up to]] [[isometry]] by this property, and is called the ''completion'' of ''M''.
 
The completion of ''M'' can be constructed as a set of [[equivalence class]]es of Cauchy sequences in ''M''. For any two Cauchy sequences (''x''<sub>''n''</sub>)<sub>''n''</sub> and (''y''<sub>''n''</sub>)<sub>''n''</sub> in ''M'', we may define their distance as
: <math>d(x, y) = \lim_n d\left(x_n, y_n\right)</math>
 
(This limit exists because the real numbers are complete.) This is only a [[pseudometric space|pseudometric]], not yet a metric, since two different Cauchy sequences may have the distance 0. But "having distance 0" is an [[equivalence relation]] on the set of all Cauchy sequences, and the set of equivalence classes is a metric space, the completion of ''M''.  The original space is embedded in this space via the identification of an element ''x'' of ''M'' with the equivalence class of sequences converging to ''x'' (i.e., the equivalence class containing the sequence with constant value ''x'').  This defines an [[isometry]] onto a dense subspace, as required. Notice, however, that this construction makes explicit use of the completeness of the real numbers, so completion of the rational numbers needs a slightly different treatment.
 
[[Georg Cantor|Cantor]]'s construction of the real numbers is similar to the above construction; the real numbers are the completion of the rational numbers using the ordinary absolute value to measure distances. The additional subtlety to contend with is that it is not logically permissible to use the completeness of the real numbers in their own construction. Nevertheless, equivalence classes of Cauchy sequences are defined as above, and the set of equivalence classes is easily shown to be a [[Field (mathematics)|field]] that has the rational numbers as a subfield. This field is complete, admits a natural [[total ordering]], and is the unique totally ordered complete field (up to isomorphism). It is ''defined'' as the field of real numbers (see also [[Construction of the real numbers]] for more details). One way to visualize this identification with the real numbers as usually viewed is that the equivalence class consisting of those Cauchy sequences of rational numbers that "ought" to have a given real limit is identified with that real number. The truncations of the decimal expansion give just one choice of Cauchy sequence in the relevant equivalence class.
 
For a prime ''p'', the [[p-adic number|''p''-adic number]]s arise by completing the rational numbers with respect to a different metric.
 
If the earlier completion procedure is applied to a [[normed vector space]], the result is a [[Banach space]] containing the original space as a dense subspace, and if it is applied to an [[inner product space]], the result is a [[Hilbert space]] containing the original space as a dense subspace.
 
==Topologically complete spaces==
Note that completeness is a property of the ''metric'' and not of the ''[[topology]]'', meaning that a complete metric space can be [[homeomorphic]] to a non-complete one.  An example is given by the real numbers, which are complete but homeomorphic to the open interval {{open-open|0,1}}, which is not complete. 
 
In [[topology]] one considers ''[[completely metrizable space]]s'', spaces for which there exists at least one complete metric inducing the given topology. Completely metrizable spaces can be characterized as those spaces that can be written as an [[intersection (set theory)|intersection]] of countably many open subsets of some complete metric space. Since the conclusion of the [[Baire category theorem]] is purely topological, it applies to these spaces as well.
 
Completely metrizable spaces are often called ''topologically complete''. However, the latter term is somewhat arbitrary since metric is not the most general structure on a topological space for which one can talk about completeness (see the section [[#Alternatives and generalizations|Alternatives and generalizations]]). Indeed, some authors use the term ''topologically complete'' for a wider class of topological spaces, the [[completely uniformizable space]]s.<ref>Kelley, Problem 6.L, p. 208</ref>
 
A topological space homeomorphic to a separable complete metric space is called a [[Polish space]].
 
==Alternatives and generalizations==
Since [[Cauchy sequence]]s can also be defined in general [[topological group]]s, an alternative to relying on a metric structure for defining completeness and constructing the completion of a space is to use a group structure. This is most often seen in the context of [[topological vector space]]s, but requires only the existence of a continuous "subtraction" operation.  In this setting, the distance between two points ''x'' and ''y'' is gauged not by a real number ''ε'' via the metric ''d'' in the comparison ''d''(''x'',&#8239;''y'')&nbsp;&lt;&nbsp;''ε'', but by an open neighbourhood ''N'' of 0 via subtraction in the comparison ''x''&nbsp;−&nbsp;''y''&nbsp;∈&nbsp;''N''.
 
A common generalisation of these definitions can be found in the context of a [[uniform space]], where an [[Uniform space#Entourage definition|entourage]] is a set of all pairs of points that are at no more than a particular "distance" from each other.
 
It is also possible to replace Cauchy ''sequences'' in the definition of completeness by Cauchy ''[[net (mathematics)|net]]s'' or [[filter (mathematics)#Filters in uniform spaces|Cauchy filters]].  If every Cauchy net (or equivalently every Cauchy filter) has a limit in ''X'', then ''X'' is called complete.  One can furthermore construct a completion for an arbitrary uniform space similar to the completion of metric spaces. The most general situation in which Cauchy nets apply is [[Cauchy space]]s; these too have a notion of completeness and completion just like uniform spaces.
 
==See also==
*[[Knaster–Tarski theorem]]
*[[Completion (ring theory)]]
 
== Notes ==
{{reflist}}
 
==References==
 
* {{Cite book | last=Kelley | first=John L. | title=General Topology | isbn=0-387-90125-6 | publisher=Springer | year=1975}}
* Kreyszig, Erwin, ''Introductory functional analysis with applications'' (Wiley, New York, 1978). ISBN 0-471-03729-X
* Lang, Serge, "Real and Functional Analysis" ISBN 0-387-94001-4
* {{cite book
  | last      = Meise
  | first    = Reinhold
  | coauthors = Vogt, Dietmar; translated by Ramanujan, M.S.
  | title    = Introduction to functional analysis
  | publisher = Oxford: Clarendon Press; New York: Oxford University Press
  | year      = 1997
  | pages    =
  | isbn      = 0-19-851485-9
}}
 
==External links==
* [http://www.encyclopediaofmath.org/index.php/Complete_metric_space Complete metric space] at [http://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]
* [http://www.encyclopediaofmath.org/index.php/Completion Completion] at [http://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]
 
{{DEFAULTSORT:Complete Metric Space}}
[[Category:Metric geometry]]

Latest revision as of 15:36, 14 November 2014

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