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EMBEDDING

:''For other uses of this term, see embedded (disambiguation).''
In mathematics, an 'embedding' (or 'imbedding') is one instance of some mathematical object contained within another instance, such as a group that is a subgroup.

Contents
Abstractly or categorically
Topology and Geometry
General topology
Differential topology
Riemannian geometry
Algebra
Field theory
Domain theory
Metric spaces
Normed spaces
Model theory
See also

Abstractly or categorically


An 'abstract embedding' between two X,Y, objects in a given category mathfrak{C}, is a mathfrak{C}-morphism fcolon X o Y which is injective.

Topology and Geometry


General topology

In general topology, an embedding is a homeomorphism onto its image. More explicitly, a map ''f'' : ''X'' → ''Y'' between topological spaces ''X'' and ''Y'' is an embedding if ''f'' yields a homeomorphism between ''X'' and ''f''(''X'') (where ''f''(''X'') carries the subspace topology inherited from ''Y''). Intuitively then, the embedding ''f'' : ''X'' → ''Y'' lets us treat ''X'' as a subspace of ''Y''. Every embedding is injective and continuous. Every map that is injective, continuous and either open or closed is an embedding; however there are also embeddings which are neither open nor closed. The latter happens if the image ''f''(''X'') is neither an open set nor a closed set in ''Y''.
For a given space X, the existence of an embedding X → Y is a topological invariant of X. This allows two spaces to be distinguished if one is able to be embedded into a space which the other is not.
An embedding is 'proper' if it behaves well w.r.t. boundaries: one requires the map f: X
ightarrow Y to be such that

f(partial X) = f(X) cap partial Y, and

f(X) is transversal to partial Y in any point of f(partial X).
The first condition is equivalent to having f(partial X) subseteq partial Y and f(X setminus partial X) subseteq Y setminus partial Y. The second condition, roughly speaking, says that f(X) is not tangent to the boundary of Y.
Differential topology

In differential topology:
Let ''M'' and ''N'' be smooth manifolds and f:M o N be a smooth map, it is called an immersion if the derivative of ''f'' is everywhere injective. Then an 'embedding', or a 'smooth embedding', is defined to be an immersion which is an embedding in the above sense (i.e. homeomorphism onto its image).
In other words, an embedding is diffeomorphic to its image, and in particular the image of an embedding must be a submanifold. An immersion is a local embedding (i.e. for any point xin M there is a neighborhood xin Usubset M such that f:U o N is an embedding.)
When the manifold is compact, the notion of a smooth embedding is equivalent to that of an injective immersion.
An important case is ''N''='R'n. The interest here is in how large ''n'' must be, in terms of the dimension ''m'' of ''M''. The Whitney embedding theorem states that ''n'' = 2''m'' is enough. For example the real projective plane of dimension 2 requires ''n'' = 4 for an embedding. An immersion of this surface is, however, possible in 'R'3, and one example is Boy's surface—which has self-intersections. The Roman surface fails to be an immersion as it contains cross-caps.
Riemannian geometry

In Riemannian geometry:
Let (''M,g'') and (''N,h'') be Riemannian manifolds.
An 'isometric embedding' is a smooth embedding ''f'' : ''M'' → ''N'' which preserves the metric in the sense that ''g'' is equal to the pullback of ''h'' by ''f'', i.e. ''g'' = ''f''
★ ''h''. Explicitly, for any two tangent vectors
:v,win T_x(M)
we have
:g(v,w)=h(df(v),df(w)).,
Analogously, 'isometric immersion' is an immersion between Riemannian manifolds which preserves the Riemannian metrics.
Equivalently, an isometric embedding (immersion) is a smooth embedding (immersion) which preserves length of curves (cf. Nash embedding theorem).

Algebra


In general, for a category ''C'', an embedding between two ''C''-algebraic structures ''X'' and ''Y'' is a ''C''-morphism ''e:X→Y'' which is injective.
Field theory

In field theory, an 'embedding' of a field ''E'' in a field ''F'' is a ring homomorphism σ : ''E'' → ''F''.
The kernel of σ is an ideal of ''E'' which cannot be the whole field ''E'', because of the condition σ(1)=1. Furthermore, it is a well-known property of fields that their only ideals are the zero ideal and the whole field itself. Therefore, the kernel is 0, so any embedding of fields is a monomorphism. Moreover, ''E'' is isomorphic to the subfield σ(''E'') of ''F''. This justifies the name ''embedding'' for an arbitrary homomorphism of fields.

Domain theory


In domain theory, an 'embedding' of partial orders is F in the function space [X →Y] such that
# orall x_1,x_2in X: x_1leq x_2Leftrightarrow F(x_1)leq F(x_2) and
# orall yin Y:{x: F(x)leq y} is directed.
''Based on an article from FOLDOC, .''

Metric spaces


A mapping phi: X o Y of metric spaces is called an ''embedding''
(with distortion C>0) if
: L d_X(x, y) leq d_Y(phi(x), phi(y)) leq CLd_X(x,y)
for some constant L>0.
Normed spaces

An important special case is that of normed spaces; in this case it is natural to consider linear embeddings.
One of the basic questions that can be asked about a finite-dimensional normed space (X, | cdot |) is, ''what is the maximal dimension k such that the Hilbert space ell_2^k can be linearly embedded into X with constant distortion?''
The answer is given by Dvoretzky's theorem.

Model theory


If L is a first order language and A,B are L-structures, then a map sigma:A o B is an L-embedding iff all the following holds:

sigma is injective,

★ for every n-ary function symbol f in L and a_1,ldots,a_n in A^n, we have sigma(f^A(a_1,ldots,a_n))=f^B(sigma(a_1),ldots,sigma(a_n)),

★ for every n-ary relation symbol R in L and a_1,ldots,a_n in A^n, we have A models R(a_1,ldots,a_n) iff B models R(sigma(a_1),ldots,sigma(a_n)),

★ for every constant symbol c in L, sigma(c^A)=c^B.

See also



Inclusion map

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