|  Extrinsic Curvature | 
In General
  > s.a. curvature; Willmore Surface.
  $ Def: Given an \((n-1)\)-dimensional
    hypersurface Σ in an n-dimensional manifold M, its extrinsic
    curvature or second fundamental form, is the rate of change of the unit normal \(n^a\) to Σ,
Kab:= qam ∇mnb ≡ \({1\over2}{\cal L}\)n qab = \(1\over2\)N−1 (\(\dot q\)ab − \(\cal L\)N qab) ,
    or simply ∇a nb
    if na is the unit tangent
    to the geodesics normal to Σ.
  * Meaning: The tensor \(K_{ab}\)
    has information on the the metric intrinsic to the surface, as well as on the curvature
    due to the embedding of the surface; It is like the "acceleration" of a surface.
  * Applications: Used as a dynamical
    variable in the initial-value formulation of gravity theories, and in boundary terms for the action;
    > s.a. Gauss-Codazzi Equations; action
      and initial-value formulation of general relativity.
  > Online resources:
    see Wikipedia page.
Trace of the Extrinsic Curvature
  > s.a. time in gravity [York time].
  $ Def: Defined by K:=
    qabKab.
  * Properties: It satisfies
∫∂(M) K dS = (∂/∂n) ∫∂(M) dS .
Generalizations > s.a. embeddings.
  * Higher codimension:
    For a submanifold N of codimension k > 1, it can be generalized to
Kabc:= Kab(i) e(i)c ,
where e(i)c, with i = 1, ..., k, are orthonormal vectors normal to N.
Extremal Surface > s.a. Bubbles;
  foliations; Hypersurface.
  $ Def: A hypersurface in a
    manifold such that tr K = 0, with K the extrinsic curvature.
  * In R3:
    Infinite minimal non-intersecting 2-surfaces, solutions to the Plateau problem (finding
    the surface of least area that spans a given rigid boundary curve); The plane, catenoid,
    and helicoid have been known for a long time; A new, countably infinite family has been
    found by D Hoffman and W Meeks, with surfaces that are homeomorphic to a sphere with
    three holes and one or more handles (computers were used for visualization).
  * Applications: Soap bubbles.
  * Lorentzian manifolds: A necessary
    condition for a globally hyperbolic spacetime \(\mathbb R\) × Σ to admit
    a maximal slice is that the Cauchy slice Σ admit a metric with non-negative
    scalar curvature, R ≥ 0; Most Σ do not admit such metrics, for
    topological reasons.
  @ General references: Kanigel ThSc(93)may.
  @ Riemannian manifolds: Pitts 81;
    Colding & Minicozzi AM(04),
    AM(04),
    Meeks et al JDG(04) [3D, finite genus];
    Collin et al JDG(04);
    Meeks & Rosenberg JDG(04);
    Cecil JCP(05) [numerical, arbitrary dimension];
    Frohman & Meeks AM(08) [in \(\mathbb R\)3, classification];
    Tråsdahl & Rønquist JCP(11) [high-order numerical approximations];
    Meeks & Pérez BAMS(11) [classical theory of minimal surfaces];
    Mahadevan PRS(12) [minimal surfaces bounded by elastic lines].
  @ Lorentzian manifolds: Cantor et al CMP(76);
    Marsden & Tipler PRP(80);
    Brill in(83);
    Bartnik CMP(84),
    in(84),
    et al CMP(90);
    Chruściel & Wald CMP(94) [stationary];
    Burnett & Rendall CQG(96)gq/95 [spherically symmetric];
    Aledo et al JGP(07)
      [2+1, positive definite Kab];
    Witt a0908 [topological obstructions];
    Anciaux 10;
    > s.a. schwarzschild-de sitter spacetime.
  @ Maximal slicings of spacetimes:
    Cordero-Carrión et al JPCS(10)-a1003 [spherically symmetric, local existence].
  @ Spacetimes without extremal surfaces:
    Witt PRL(86) [vacuum].
Constant-Mean-Curvature Surfaces
  @ References:
    López 13
      [Riemannian, surfaces of constant mean curvature with boundary];
    López JGP(07) [in Minkowski spacetime];
    Dilts & Holst a1710 [spacetimes, existence results].
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