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Embedding

From Wikipedia, the free encyclopedia
(Redirected fromIsometric embedding)
"Isometric embedding" redirects here. For related concepts formetric spaces, seeisometry.
For embeddings of graphs in two-dimensional manifolds, seegraph embedding.
For other uses, seeEmbedding (disambiguation).
Inclusion of one mathematical structure in another, preserving properties of interest

Inmathematics, anembedding (orimbedding[1]) is one instance of somemathematical structure contained within another instance, such as agroup that is asubgroup.

When some objectX{\displaystyle X} is said to be embedded in another objectY{\displaystyle Y}, the embedding is given by someinjective and structure-preserving mapf:XY{\displaystyle f:X\rightarrow Y}. The precise meaning of "structure-preserving" depends on the kind of mathematical structure of whichX{\displaystyle X} andY{\displaystyle Y} are instances. In the terminology ofcategory theory, a structure-preserving map is called amorphism.

The fact that a mapf:XY{\displaystyle f:X\rightarrow Y} is an embedding is often indicated by the use of a "hooked arrow" (U+21AA RIGHTWARDS ARROW WITH HOOK);[2] thus:f:XY.{\displaystyle f:X\hookrightarrow Y.} (On the other hand, this notation is sometimes reserved forinclusion maps.)

GivenX{\displaystyle X} andY{\displaystyle Y}, several different embeddings ofX{\displaystyle X} inY{\displaystyle Y} may be possible. In many cases of interest there is a standard (or "canonical") embedding, like those of thenatural numbers in theintegers, the integers in therational numbers, the rational numbers in thereal numbers, and the real numbers in thecomplex numbers. In such cases it is common to identify thedomainX{\displaystyle X} with itsimagef(X){\displaystyle f(X)} contained inY{\displaystyle Y}, so thatXY{\displaystyle X\subseteq Y}.

Topology and geometry

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General topology

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Ingeneral topology, an embedding is ahomeomorphism onto its image.[3] More explicitly, an injectivecontinuous mapf:XY{\displaystyle f:X\to Y} betweentopological spacesX{\displaystyle X} andY{\displaystyle Y} is atopological embedding iff{\displaystyle f} yields a homeomorphism betweenX{\displaystyle X} andf(X){\displaystyle f(X)} (wheref(X){\displaystyle f(X)} carries thesubspace topology inherited fromY{\displaystyle Y}). Intuitively then, the embeddingf:XY{\displaystyle f:X\to Y} lets us treatX{\displaystyle X} as asubspace ofY{\displaystyle Y}. Every embedding is injective andcontinuous. Every map that is injective, continuous and eitheropen orclosed is an embedding; however there are also embeddings that are neither open nor closed. The latter happens if the imagef(X){\displaystyle f(X)} is neither anopen set nor aclosed set inY{\displaystyle Y}.

For a given spaceY{\displaystyle Y}, the existence of an embeddingXY{\displaystyle X\to Y} is atopological invariant ofX{\displaystyle X}. This allows two spaces to be distinguished if one is able to be embedded in a space while the other is not.

Related definitions

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If the domain of a functionf:XY{\displaystyle f:X\to Y} is atopological space then the function is said to belocally injective at a point if there exists someneighborhoodU{\displaystyle U} of this point such that the restrictionf|U:UY{\displaystyle f{\big \vert }_{U}:U\to Y} is injective. It is calledlocally injective if it is locally injective around every point of its domain. Similarly, alocal (topological, resp. smooth) embedding is a function for which every point in its domain has some neighborhood to which its restriction is a (topological, resp. smooth) embedding.

Every injective function is locally injective but not conversely.Local diffeomorphisms,local homeomorphisms, and smoothimmersions are all locally injective functions that are not necessarily injective. Theinverse function theorem gives a sufficient condition for a continuously differentiable function to be (among other things) locally injective. Everyfiber of a locally injective functionf:XY{\displaystyle f:X\to Y} is necessarily adiscrete subspace of itsdomainX.{\displaystyle X.}

Differential topology

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Indifferential topology:LetM{\displaystyle M} andN{\displaystyle N} be smoothmanifolds andf:MN{\displaystyle f:M\to N} be a smooth map. Thenf{\displaystyle f} is called animmersion if itsderivative is everywhere injective. Anembedding, or asmooth embedding, is defined to be an immersion that is an embedding in the topological sense mentioned above (i.e.homeomorphism onto its image).[4]

In other words, the domain of an embedding isdiffeomorphic to its image, and in particular the image of an embedding must be asubmanifold. An immersion is precisely alocal embedding, i.e. for any pointxM{\displaystyle x\in M} there is a neighborhoodxUM{\displaystyle x\in U\subset M} such thatf:UN{\displaystyle f:U\to N} is an embedding.

When the domain manifold is compact, the notion of a smooth embedding is equivalent to that of an injective immersion.

An important case isN=Rn{\displaystyle N=\mathbb {R} ^{n}}. The interest here is in how largen{\displaystyle n} must be for an embedding, in terms of the dimensionm{\displaystyle m} ofM{\displaystyle M}. TheWhitney embedding theorem[5] states thatn=2m{\displaystyle n=2m} is enough, and is the best possible linear bound. For example, thereal projective spaceRPm{\displaystyle \mathbb {R} \mathrm {P} ^{m}} of dimensionm{\displaystyle m}, wherem{\displaystyle m} is a power of two, requiresn=2m{\displaystyle n=2m} for an embedding. However, this does not apply to immersions; for instance,RP2{\displaystyle \mathbb {R} \mathrm {P} ^{2}} can be immersed inR3{\displaystyle \mathbb {R} ^{3}} as is explicitly shown byBoy's surface—which has self-intersections. TheRoman surface fails to be an immersion as it containscross-caps.

An embedding isproper if it behaves well with respect toboundaries: one requires the mapf:XY{\displaystyle f:X\rightarrow Y} to be such that

The first condition is equivalent to havingf(X)Y{\displaystyle f(\partial X)\subseteq \partial Y} andf(XX)YY{\displaystyle f(X\setminus \partial X)\subseteq Y\setminus \partial Y}. The second condition, roughly speaking, says thatf(X){\displaystyle f(X)} is not tangent to the boundary ofY{\displaystyle Y}.

Riemannian and pseudo-Riemannian geometry

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InRiemannian geometry and pseudo-Riemannian geometry:Let(M,g){\displaystyle (M,g)} and(N,h){\displaystyle (N,h)} beRiemannian manifolds or more generallypseudo-Riemannian manifolds.Anisometric embedding is a smooth embeddingf:MN{\displaystyle f:M\rightarrow N} that preserves the (pseudo-)metric in the sense thatg{\displaystyle g} is equal to thepullback ofh{\displaystyle h} byf{\displaystyle f}, i.e.g=fh{\displaystyle g=f^{*}h}. Explicitly, for any two tangent vectorsv,wTx(M){\displaystyle v,w\in T_{x}(M)} we have

g(v,w)=h(df(v),df(w)).{\displaystyle g(v,w)=h(df(v),df(w)).}

Analogously,isometric immersion is an immersion between (pseudo)-Riemannian manifolds that preserves the (pseudo)-Riemannian metrics.

Equivalently, in Riemannian geometry, an isometric embedding (immersion) is a smooth embedding (immersion) that preserves length ofcurves (cf.Nash embedding theorem).[6]

Algebra

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In general, for analgebraic categoryC{\displaystyle C}, an embedding between twoC{\displaystyle C}-algebraic structuresX{\displaystyle X} andY{\displaystyle Y} is aC{\displaystyle C}-morphisme:XY{\displaystyle e:X\rightarrow Y} that is injective.

Field theory

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Infield theory, anembedding of afieldE{\displaystyle E} in a fieldF{\displaystyle F} is aring homomorphismσ:EF{\displaystyle \sigma :E\rightarrow F}.

Thekernel ofσ{\displaystyle \sigma } is anideal ofE{\displaystyle E}, which cannot be the whole fieldE{\displaystyle E}, because of the condition1=σ(1)=1{\displaystyle 1=\sigma (1)=1}. Furthermore, any field has as ideals only the zero ideal and the whole field itself (because if there is any non-zero field element in an ideal, it is invertible, showing the ideal is the whole field). Therefore, the kernel is0{\displaystyle 0}, so any embedding of fields is amonomorphism. Hence,E{\displaystyle E} isisomorphic to thesubfieldσ(E){\displaystyle \sigma (E)} ofF{\displaystyle F}. This justifies the nameembedding for an arbitrary homomorphism of fields.

Universal algebra and model theory

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Further information:Substructure (mathematics) andElementary equivalence

Ifσ{\displaystyle \sigma } is asignature andA,B{\displaystyle A,B} areσ{\displaystyle \sigma }-structures (also calledσ{\displaystyle \sigma }-algebras inuniversal algebra or models inmodel theory), then a maph:AB{\displaystyle h:A\to B} is aσ{\displaystyle \sigma }-embedding exactly if all of the following hold:

HereAR(a1,,an){\displaystyle A\models R(a_{1},\ldots ,a_{n})} is a model theoretical notation equivalent to(a1,,an)RA{\displaystyle (a_{1},\ldots ,a_{n})\in R^{A}}. In model theory there is also a stronger notion ofelementary embedding.

Order theory and domain theory

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Inorder theory, an embedding ofpartially ordered sets is a functionF{\displaystyle F} between partially ordered setsX{\displaystyle X} andY{\displaystyle Y} such that

x1,x2X:x1x2F(x1)F(x2).{\displaystyle \forall x_{1},x_{2}\in X:x_{1}\leq x_{2}\iff F(x_{1})\leq F(x_{2}).}

Injectivity ofF{\displaystyle F}follows quickly from this definition. Indomain theory, an additional requirement is that

yY:{xF(x)y}{\displaystyle \forall y\in Y:\{x\mid F(x)\leq y\}} isdirected.

Metric spaces

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A mappingϕ:XY{\displaystyle \phi :X\to Y} ofmetric spaces is called anembedding(withdistortionC>0{\displaystyle C>0}) if

LdX(x,y)dY(ϕ(x),ϕ(y))CLdX(x,y){\displaystyle Ld_{X}(x,y)\leq d_{Y}(\phi (x),\phi (y))\leq CLd_{X}(x,y)}

for everyx,yX{\displaystyle x,y\in X} and some constantL>0{\displaystyle L>0}.

Normed spaces

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An important special case is that ofnormed spaces; in this case it is natural to consider linear embeddings.

One of the basic questions that can be asked about a finite-dimensionalnormed space(X,){\displaystyle (X,\|\cdot \|)} is,what is the maximal dimensionk{\displaystyle k} such that theHilbert space2k{\displaystyle \ell _{2}^{k}} can be linearly embedded intoX{\displaystyle X} with constant distortion?

The answer is given byDvoretzky's theorem.

Category theory

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Incategory theory, there is no satisfactory and generally accepted definition of embeddings that is applicable in all categories. One would expect that all isomorphisms and all compositions of embeddings are embeddings, and that all embeddings are monomorphisms. Other typical requirements are: anyextremal monomorphism is an embedding and embeddings are stable underpullbacks.

Ideally the class of all embeddedsubobjects of a given object, up to isomorphism, should also besmall, and thus anordered set. In this case, the category is said to be well powered with respect to the class of embeddings. This allows defining new local structures in the category (such as aclosure operator).

In aconcrete category, anembedding is a morphismf:AB{\displaystyle f:A\rightarrow B} that is an injective function from the underlying set ofA{\displaystyle A} to the underlying set ofB{\displaystyle B} and is also aninitial morphism in the following sense:Ifg{\displaystyle g} is a function from the underlying set of an objectC{\displaystyle C} to the underlying set ofA{\displaystyle A}, and if its composition withf{\displaystyle f} is a morphismfg:CB{\displaystyle fg:C\rightarrow B}, theng{\displaystyle g} itself is a morphism.

Afactorization system for a category also gives rise to a notion of embedding. If(E,M){\displaystyle (E,M)} is a factorization system, then the morphisms inM{\displaystyle M} may be regarded as the embeddings, especially when the category is well powered with respect toM{\displaystyle M}. Concrete theories often have a factorization system in whichM{\displaystyle M} consists of the embeddings in the previous sense. This is the case of the majority of the examples given in this article.

As usual in category theory, there is adual concept, known as quotient. All the preceding properties can be dualized.

An embedding can also refer to anembedding functor.

See also

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Notes

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  1. ^Spivak 1999, p. 49 suggests that "the English" (i.e. the British) use "embedding" instead of "imbedding".
  2. ^"Arrows – Unicode"(PDF). Retrieved2017-02-07.
  3. ^Hocking & Young 1988, p. 73.Sharpe 1997, p. 16.
  4. ^Bishop & Crittenden 1964, p. 21.Bishop & Goldberg 1968, p. 40.Crampin & Pirani 1994, p. 243.do Carmo 1994, p. 11.Flanders 1989, p. 53.Gallot, Hulin & Lafontaine 2004, p. 12.Kobayashi & Nomizu 1963, p. 9.Kosinski 2007, p. 27.Lang 1999, p. 27.Lee 1997, p. 15.Spivak 1999, p. 49.Warner 1983, p. 22.
  5. ^Whitney H.,Differentiable manifolds, Ann. of Math. (2),37 (1936), pp. 645–680
  6. ^Nash J.,The embedding problem for Riemannian manifolds, Ann. of Math. (2),63 (1956), 20–63.

References

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External links

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