Immersion (or local embedding)
$ Def: A map f : S → M is
an immersion if (f*)p
is injective for all p
S.
* Idea: This means that f is
locally 1-to-1, but there may be self-intersections globally, as opposed to
what happens with an embedding;
One usually requires
also that f and its local inverse be smooth.
* Results: Any smooth compact n-manifold can be immersed in
R2n–1.
@ References: Whitney AM(44), AM(44); Hirsch TAMS(59);
Smale AM(59); Spring BAMS(05)
[history, 1959–1973].
Immersion with Riemannian Metric > s.a. 2D
manifolds.
* Results: Any n-dimensional
Riemannian manifold with analytic metric can be analytically and isometrically
locally embedded in a Euclidean space
of
n (n +
1) dimensions.
@ References: Pakzad JDG(04)
[Sobolev space of immersions]; Ranjbar-Motlagh JGP(09) [non-existence theorem].
Immersion with Indefinite Signature Metric
* Results: Any pseudo-Riemannian
manifold of signature (p, q),
p + q = n, with analytic metric can be analytically
and isometrically embedded in a flat space
of dimension
n (n +
1) and signature (r, s), r > p, s > q.
@ General references: Friedman RMP(65);
Graves TAMS(79); Xia JGP(09) [Ribaucour transformation
and permutability theorem].
@ And general relativity: Estabrook & Wahlquist CQG(93);
Edelen CQG(02)
[Einstein-Riemann spaces in 6D flat]; Monte IJMPA(09)-a0908 [re Schwarzschild immersion into a 6D Minkowski].
Embedding > s.a. foliations; Hypersurface; Whitney Duality Theorem; [graphs;
knots].
$ Def: A map f : S → M is
an embedding if it is an injective immersion.
* Idea: The map f a globally one-to-one immersion, and f(S)
does not intersect itself in M.
* In addition: Sometimes one wants S to be homeomorphic to f(S)
in the induced topology from M.
@ With metric: Carter CM(97)ht-in, ht/97-in
[formalism]; Pavsic & Tapia gq/00 [references];
> s.a. membranes [dynamics].
@ Embedding diagrams: Romano & Price CQG(95)gq/94 [initial
data for black hole collisions];
Lu & Suen GRG(03)
[extrinsic-curvature-based];
Hledík et al ap/07-in; > s.a. reissner-nordström
spacetime.
Embedding with Riemannian Metric > s.a. [riemannian
geometry]; extrinsic curvature.
* Results: Any compact n-dimensional
C1 Riemannian
manifold (with or without boundary) has a C1 isometric
embedding in 2n-dimensional Euclidean space; Any non-compact one in
2n +
1 dimensions; However, if a compact one has a C1 embedding
in k > n dimensions, then it also has a C1 isometric
embedding there (thus any point has a neighborhood with a C1 isometric
embedding in n +
1 dimensions).
* Ideal embeddings: The embedded manifold receives the least amount
of tension from the surrounding space.
* Results: Any compact, n-dimensional
Cp Riemannian
manifold with p > 2 has
a Cp isometric embedding in
n (3n +
11) dimensional Euclidean space; Any non-compact one in
n (n +
1) (3n + 11) dimensions (often much less).
@ References: Greene 70.
Embedding with Lorentzian Metric > s.a. lorentzian
geometry [hypersurfaces]; extrinsic
curvature;
formulations of general relativity.
* Remark: Obviously,
the Lorentzian, global case in general is not so easy; For example, the metric
may have closed timelike curves.
* In flat spaces: Any
Ck
Lorentzian manifold, with 3
k <
,
can be embedded in a (q + 2)-dimensional flat space (2 are timelike!),
with
q =
n (3n +
11) in the compact case (46 for n =
4), and q = (1/6) n (2n2 +
37) + (5/2) n2 + 1 in the non-compact
case (87 for n = 4); If the spacetime is
globally hyperbolic, q + 1 is enough.
* In Ricci-flat spaces:
(in 4D, Campbell-Magaard theorem) Any n-dimensional (n
3)
Lorentzian manifold can be isometrically and harmonically embedded in a (n +
1)-dimensional semi-Riemannian Ricci-flat space.
* Hyperspace: In general
relativity, the space of embeddings of a hypersurface in spacetime (roughly!).
@ General references: Rosen RMP(65)
[examples]; Clarke PRS(70);
Greene 70; Mueller & Sánchez a0812 [globally
hyperbolic]; Kim CQG(09) [with a non-compact Cauchy surface].
@ Hyperspace: Kuchar JMP(76),
JMP(76), JMP(76),
JMP(77).
@ For 4D Ricci-flat spaces: Romero et al GRG(96),
Lidsey et al CQG(97)gq/99 [4D
solution in 5D]; Mashhoon & Wesson GRG(07) [with a 4D cosmological constant].
@ For 4D spaces with cosmological constant: Ponce de León G&C(08)-a0709 [in
various 5D spaces].
@
Campbell-Magaard theorem: Dahia & Romero JMP(02); Anderson gq/04 [attack];
Dahia & Romero CQG(05)gq [interpretation];
Wesson gq/05 [apology].
@ For n-dimensional Ricci-flat spaces:
Seahra & Wesson CQG(03)gq;
Chervon et al PLA(04);
Anderson gq/04.
@ Codimension-1 embeddings: Anderson & Lidsey CQG(01)gq,
Katzourakis mp/04,
m.DG/05 [in
Einstein spaces]; Dahia & Romero
JMP(02) [with prescribed D+1 Ricci tensor]; Haesen & Verstraelen
JMP(04)gq/03 [ideal
embeddings].
@ Codimension-2 embeddings: Dillen et al JGP(04)
[inequalities intrinsic/extrinsic
curvature].
Embedding with Arbitrary Metric, Global
* Results: For a Cinfty compact
manifold (with possibly degenerate metric), an embedding can be found in 2k = n (n+5)
dimensions, signature (k, k), and
2k = 2 (2n+1) (2n+6) dimensions, signature (k, k),
in the non-compact case.
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