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Bingarten Map 📂Geometry

Bingarten Map

Definition1

Let MM be a surface, and pMp \in M be a point on the surface. The map L:TpMR3L : T_{p}M \to \mathbb{R}^{3}, defined as follows, is called the Weingarten map.

L(X)=Xn L (\mathbf{X}) = - \mathbf{X}\mathbf{n}

Here, XTpM\mathbf{X} \in T_{p}M is a tangent vector, n\mathbf{n} is a unit normal, and Xn\mathbf{X}\mathbf{n} is the directional derivative of n\mathbf{n}.

Properties

  1. LL is a linear transformation that is L:TpMTpML : T_{p}M \to T_{p}M.

  2. Since {x1,x2}\left\{ \mathbf{x}_{1}, \mathbf{x}_{2} \right\} is a basis for TpMT_{p}M, if we denote it as L(xk)=lLlkxlL(\mathbf{x}_{k}) = \sum\limits_{l}{L^{l}}_{k}\mathbf{x}_{l}, the following holds:

    Llk=iLikgil=iLkigil{L^{l}}_{k} = \sum_{i}L_{ik}g^{il} = \sum_{i}L_{ki}g^{il}

    Where, LijL_{ij} is the coefficient of the second fundamental form, and [gkl][g^{kl}] is the inverse matrix of the first fundamental form coefficients. When expressed as a matrix,

    [Llk]=[L11L12L21L22]=[gli][Lik] \begin{bmatrix} {L^{l}}_{k} \end{bmatrix} = \begin{bmatrix} {L^{1}}_{1} & {L^{1}}_{2} \\ {L^{2}}_{1} & {L^{2}}_{2} \end{bmatrix} = \begin{bmatrix} g^{li} \end{bmatrix} \begin{bmatrix} L_{ik} \end{bmatrix}

Explanation

The minus sign in the definition is there for convenience.

The Weingarten map can be understood as an operator that measures the rate of change of n\mathbf{n} in each tangent direction at each point pp. For this reason, it is also referred to as a shape operator.

  1. By definition, LL is defined as a map that sends TpMT_{p}M to R3\mathbb{R}^{3}, but in fact, it can be seen that it sends it to TpMT_{p}M.

  2. In other words, Llk{L^{l}}_{k} is the coefficient of the ll-th basis of L(xk)L(\mathbf{x_{k}}). That is, if expressed as a coordinate vector for the basis B={x1,x2}B = \left\{ \mathbf{x}_{1}, \mathbf{x}_{2} \right\}, it is as follows. L(xk)=L1kx1+L2kx2 L(\mathbf{x}_{k}) = {L^{1}}_{k}\mathbf{x}_{1} + {L^{2}}_{k}\mathbf{x}_{2} [L(xk)]B=[L1kL2k] \left[ L(\mathbf{x}_{k}) \right]_{B} = \begin{bmatrix} {L^{1}}_{k} \\ {L^{2}}_{k} \end{bmatrix} Therefore, the matrix representation of LL is as follows. [L]B=[L11L12L21L22] [L]_{B} = \begin{bmatrix} {L^{1}}_{1} & {L^{1}}_{2} \\ {L^{2}}_{1} & {L^{2}}_{2} \end{bmatrix} Furthermore, due to the properties of the first fundamental form, the following holds. Lij=lLilδlj=l,kLilglkgkj=l,kLliglkgkj=kLkigkj L_{ij} = \sum_{l}L_{il}\delta_{lj} = \sum\limits_{l,k} L_{il}g^{lk}g_{kj} = \sum\limits_{l,k} L_{li}g^{lk}g_{kj} = \sum\limits_{k}{L^{k}}_{i}g_{kj}

Since LL is a linear transformation between finite-dimensional vector spaces, trL\tr{L} and det(L)\det(L) are invariants, and are respectively called the mean curvature and the Gaussian curvature.


  1. Richard S. Millman and George D. Parker, Elements of Differential Geometry (1977), p125 ↩︎