|  Embeddings of Manifolds | 
In General > s.a. foliations;
  Hypersurface; immersions.
  $ Def: A map f : S →
    M between two differentiable manifolds 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.
  * Whitney (strong) embedding theorem:
    Any smooth (Hausdorff, second-countable) n-dimensional manifold  can be smoothly
    embedded in 2n-dimensional Euclidean space;
    > s.a. Wikipedia page.
  @ General references: Skopenkov T&A(10)
      [classification of smooth embeddings of 4-manifolds in \(\mathbb R\)7];
    Daverman & Venema 09.
  @ With metric: Carter CM(97)ht-fs,
    ht/97-ln [formalism];
    Pavšič & 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 AIP(06)ap/07;
    > s.a. reissner-nordström spacetime;
      schwarzschild geometry.
  > Related topics: see knots;
    types of graphs [embedded in manifolds]; Whitney
    Duality Theorem; Wild Embeddings.
  > Online resources: see
    Wikipedia page.
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 \(1\over2\)n
    (3n + 11) dimensional Euclidean space; Any non-compact one in \(1\over2\)n
    (n + 1) (3n + 11) dimensions (often much less).
  @ References: Greene 70;
    Arnlind et al a1001 [geometry and algebraic structure];
    Arnlind et al a1003 [in terms of Nambu brackets].
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 = \(1\over2\)n (3n +
  11) in the compact case (46 for n =
  4), and q = \(1\over6\)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 TAMS-a0812 [globally
  hyperbolic]; Kim CQG(09)
  [with a non-compact Cauchy surface]; Ponce de León CQG(15)-a1509;
    Sheykin et al a2004 [explicit embeddings].
  @ Hyperspace: Kuchař 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];
    Avalos et al JMP(17)-a1701 [extension to Weyl manifolds].
  @ For n-dimensional Ricci-flat spaces:
    Seahra & Wesson CQG(03)gq;
    Chervon et al PLA(04);
    Anderson gq/04;
    Avalos et al a1708.
  @ 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];
    Kuhfittig AP(18)-a1805 [applications to wormholes and galaxy rotation curves].
  @ Codimension-2 embeddings: Dillen et al JGP(04) [inequalities intrinsic/extrinsic curvature].
Embedding with Arbitrary Metric, Global
  * Results: For a C∞ 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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