Second fundamental form#Generalization to arbitrary codimension

{{short description|Quadratic form related to curvatures of surfaces}}

In differential geometry, the second fundamental form (or shape tensor) is a quadratic form on the tangent plane of a smooth surface in the three-dimensional Euclidean space, usually denoted by \mathrm{I\!I} (read "two"). Together with the first fundamental form, it serves to define extrinsic invariants of the surface, its principal curvatures. More generally, such a quadratic form is defined for a smooth immersed submanifold in a Riemannian manifold.

Surface in R<sup>3</sup>

=Motivation=

The second fundamental form of a parametric surface {{math|S}} in {{math|R3}} was introduced and studied by Gauss. First suppose that the surface is the graph of a twice continuously differentiable function, {{math|z {{=}} f(x,y)}}, and that the plane {{math|z {{=}} 0}} is tangent to the surface at the origin. Then {{math|f}} and its partial derivatives with respect to {{math|x}} and {{math|y}} vanish at (0,0). Therefore, the Taylor expansion of f at (0,0) starts with quadratic terms:

: z=L\frac{x^2}{2} + Mxy + N\frac{y^2}{2} + \text{higher order terms}\,,

and the second fundamental form at the origin in the coordinates {{math|(x,y)}} is the quadratic form

: L \, dx^2 + 2M \, dx \, dy + N \, dy^2 \,.

For a smooth point {{math|P}} on {{math|S}}, one can choose the coordinate system so that the plane {{math|z {{=}} 0}} is tangent to {{math|S}} at {{math|P}}, and define the second fundamental form in the same way.

=Classical notation=

The second fundamental form of a general parametric surface is defined as follows. Let {{math|1=r = r(u,v)}} be a regular parametrization of a surface in {{math|R3}}, where {{math|r}} is a smooth vector-valued function of two variables. It is common to denote the partial derivatives of {{math|r}} with respect to {{math|u}} and {{math|v}} by {{math|ru}} and {{math|rv}}. Regularity of the parametrization means that {{math|ru}} and {{math|rv}} are linearly independent for any {{math|(u,v)}} in the domain of {{math|r}}, and hence span the tangent plane to {{math|S}} at each point. Equivalently, the cross product {{math|ru × rv}} is a nonzero vector normal to the surface. The parametrization thus defines a field of unit normal vectors {{math|n}}:

:\mathbf{n} = \frac{\mathbf{r}_u\times\mathbf{r}_v}

\mathbf{r}_u\times\mathbf{r}_v
\,.

The second fundamental form is usually written as

:\mathrm{I\!I} = L\, du^2 + 2M\, du\, dv + N\, dv^2 \,,

its matrix in the basis {{math|{ru, rv}}} of the tangent plane is

: \begin{bmatrix}

L&M\\

M&N

\end{bmatrix} \,.

The coefficients {{math|L, M, N}} at a given point in the parametric {{math|uv}}-plane are given by the projections of the second partial derivatives of {{math|r}} at that point onto the normal line to {{math|S}} and can be computed with the aid of the dot product as follows:

:L = \mathbf{r}_{uu} \cdot \mathbf{n}\,, \quad

M = \mathbf{r}_{uv} \cdot \mathbf{n}\,, \quad

N = \mathbf{r}_{vv} \cdot \mathbf{n}\,.

For a signed distance field of Hessian {{math|H}}, the second fundamental form coefficients can be computed as follows:

:L = -\mathbf{r}_u \cdot \mathbf{H} \cdot \mathbf{r}_u\,, \quad

M = -\mathbf{r}_u \cdot \mathbf{H} \cdot \mathbf{r}_v\,, \quad

N = -\mathbf{r}_v \cdot \mathbf{H} \cdot \mathbf{r}_v\,.

=Physicist's notation=

The second fundamental form of a general parametric surface {{math|S}} is defined as follows.

Let {{math|r {{=}} r(u1,u2)}} be a regular parametrization of a surface in {{math|R3}}, where {{math|r}} is a smooth vector-valued function of two variables. It is common to denote the partial derivatives of {{math|r}} with respect to {{math|uα}} by {{math|rα}}, {{math|α {{=}} 1, 2}}. Regularity of the parametrization means that {{math|r1}} and {{math|r2}} are linearly independent for any {{math|(u1,u2)}} in the domain of {{math|r}}, and hence span the tangent plane to {{math|S}} at each point. Equivalently, the cross product {{math|r1 × r2}} is a nonzero vector normal to the surface. The parametrization thus defines a field of unit normal vectors {{math|n}}:

:\mathbf{n} = \frac{\mathbf{r}_1\times\mathbf{r}_2}

\mathbf{r}_1\times\mathbf{r}_2
\,.

The second fundamental form is usually written as

:\mathrm{I\!I} = b_{\alpha \beta} \, du^{\alpha} \, du^{\beta} \,.

The equation above uses the Einstein summation convention.

The coefficients {{math|bαβ}} at a given point in the parametric {{math|u1u2}}-plane are given by the projections of the second partial derivatives of {{math|r}} at that point onto the normal line to {{math|S}} and can be computed in terms of the normal vector {{math|n}} as follows:

:b_{\alpha \beta} = r_{,\alpha \beta}^{\ \ \,\gamma} n_{\gamma}\,.

Hypersurface in a Riemannian manifold

In Euclidean space, the second fundamental form is given by

:\mathrm{I\!I}(v,w) = -\langle d\nu(v),w\rangle\nu

where \nu is the Gauss map, and d\nu the differential of \nu regarded as a vector-valued differential form, and the brackets denote the metric tensor of Euclidean space.

More generally, on a Riemannian manifold, the second fundamental form is an equivalent way to describe the shape operator (denoted by {{math|S}}) of a hypersurface,

:\mathrm I\!\mathrm I(v,w)=\langle S(v),w\rangle = -\langle \nabla_v n,w\rangle=\langle n,\nabla_v w\rangle \,,

where {{math|∇vw}} denotes the covariant derivative of the ambient manifold and {{math|n}} a field of normal vectors on the hypersurface. (If the affine connection is torsion-free, then the second fundamental form is symmetric.)

The sign of the second fundamental form depends on the choice of direction of {{math|n}} (which is called a co-orientation of the hypersurface - for surfaces in Euclidean space, this is equivalently given by a choice of orientation of the surface).

= Generalization to arbitrary codimension =

The second fundamental form can be generalized to arbitrary codimension. In that case it is a quadratic form on the tangent space with values in the normal bundle and it can be defined by

:\mathrm{I\!I}(v,w)=(\nabla_v w)^\bot\,,

where (\nabla_v w)^\bot denotes the orthogonal projection of covariant derivative \nabla_v w onto the normal bundle.

In Euclidean space, the curvature tensor of a submanifold can be described by the following formula:

:\langle R(u,v)w,z\rangle =\mathrm I\!\mathrm I(u,z)\mathrm I\!\mathrm I(v,w)-\mathrm I\!\mathrm I(u,w)\mathrm I\!\mathrm I(v,z).

This is called the Gauss equation, as it may be viewed as a generalization of Gauss's Theorema Egregium.

For general Riemannian manifolds one has to add the curvature of ambient space; if {{math|N}} is a manifold embedded in a Riemannian manifold {{math|(M,g)}} then the curvature tensor {{math|RN}} of {{math|N}} with induced metric can be expressed using the second fundamental form and {{math|RM}}, the curvature tensor of {{math|M}}:

:\langle R_N(u,v)w,z\rangle = \langle R_M(u,v)w,z\rangle+\langle \mathrm I\!\mathrm I(u,z),\mathrm I\!\mathrm I(v,w)\rangle-\langle \mathrm I\!\mathrm I(u,w),\mathrm I\!\mathrm I(v,z)\rangle\,.

See also

References

  • {{cite book|first=Heinrich|last=Guggenheimer|title=Differential Geometry|year=1977|publisher=Dover|chapter=Chapter 10. Surfaces|isbn=0-486-63433-7}}
  • {{cite book |author1=Kobayashi, Shoshichi |author2=Nomizu, Katsumi |name-list-style=amp | title = Foundations of Differential Geometry, Vol. 2 | publisher=Wiley-Interscience | year=1996 |edition=New |isbn = 0-471-15732-5}}
  • {{cite book|last=Spivak|first=Michael|title=A Comprehensive introduction to differential geometry (Volume 3)|year=1999|publisher=Publish or Perish|isbn=0-914098-72-1}}