Laplace–Beltrami operator

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Not to be confused with Beltrami operator. ‹See Tfd›

In differential geometry, the Laplace operator, named after Pierre-Simon Laplace, can be generalized to operate on functions defined on surfaces in Euclidean space and, more generally, on Riemannian and pseudo-Riemannian manifolds. This more general operator goes by the name Laplace–Beltrami operator, after Laplace and Eugenio Beltrami. Like the Laplacian, the Laplace–Beltrami operator is defined as the divergence of the gradient, and is a linear operator taking functions into functions. The operator can be extended to operate on tensors as the divergence of the covariant derivative. Alternatively, the operator can be generalized to operate on differential forms using the divergence and exterior derivative. The resulting operator is called the Laplace–de Rham operator (named after Georges de Rham).

The Laplace–Beltrami operator, like the Laplacian, is the divergence of the gradient:

\Delta f = \operatorname{div}\operatorname{grad} f.

An explicit formula in local coordinates is possible.

Suppose first that M is an oriented Riemannian manifold. The orientation allows one to specify a definite volume form on M, given in an oriented coordinate system xi by

\mathrm{vol}_n := \sqrt{|g|} \;dx^1\wedge \ldots \wedge dx^n

where the dxi are the 1-forms forming the dual basis to the basis vectors

\partial_i := \frac {\partial}{\partial x^i}

and \wedge is the wedge product. Here |g| := |det(gij)| is the absolute value of the determinant of the metric tensor gij. The divergence div X of a vector field X on the manifold is then defined as the scalar function with the property


(\mbox{div} X) \; \mathrm{vol}_n := L_X \mathrm{vol}_n

where LX is the Lie derivative along the vector field X. In local coordinates, one obtains


\mbox{div} X = \frac{1}{\sqrt{|g|}} \partial_i \left(\sqrt {|g|} X^i\right)

where the Einstein notation is implied, so that the repeated index i is summed over. The gradient of a scalar function ƒ is the vector field grad f that may be defined through the inner product \langle\cdot,\cdot\rangle on the manifold, as

\langle \mbox{grad} f(x) , v_x \rangle = df(x)(v_x)

for all vectors vx anchored at point x in the tangent space TxM of the manifold at point x. Here, dƒ is the exterior derivative of the function ƒ; it is a 1-form taking argument vx. In local coordinates, one has

 \left(\mbox{grad} f\right)^i = 
\partial^i f = g^{ij} \partial_j f

where gij are the components of the inverse of the metric tensor, so that gijgjk = δik with δik the Kronecker delta.

Combining the definitions of the gradient and divergence, the formula for the Laplace–Beltrami operator Δ applied to a scalar function ƒ is, in local coordinates

\Delta f = \operatorname{div}\;\operatorname{grad} f = 
\frac{1}{\sqrt {|g|}} \partial_i \left(\sqrt{|g|} g^{ij} \partial_j f \right).

If M is not oriented, then the above calculation carries through exactly as presented, except that the volume form must instead be replaced by a volume element (a density rather than a form). Neither the gradient nor the divergence actually depends on the choice of orientation, and so the Laplace–Beltrami operator itself does not depend on this additional structure.

Formal self-adjointness[edit]

The exterior derivative d and −div are formal adjoints, in the sense that for ƒ a compactly supported function

\int_M df(X) \;\mathrm{vol}_n = - \int_M f \mathrm{div} X \;\mathrm{vol}_n     (proof)

where the last equality is an application of Stokes' theorem. Dualizing gives

\int_M f \,\Delta h\,\mathrm{vol}_n = -\int_M \langle df, dh\rangle\, \mathrm{vol}_n

 

 

 

 

(2)

for all compactly supported functions ƒ and h. Conversely, (2) characterizes Δ completely, in the sense that it is the only operator with this property.

As a consequence, the Laplace–Beltrami operator is negative and formally self-adjoint, meaning that for compactly supported functions ƒ and h,

\int_M f\,\Delta h \;\mathrm{vol}_n = -\int_M \langle d f, d h \rangle \;\mathrm{vol}_n = \int_M h\,\Delta f \;\mathrm{vol}_n.

Because the Laplace–Beltrami operator, as defined in this manner, is negative rather than positive, often it is defined with the opposite sign.

Tensor Laplacian[edit]

The Laplace–Beltrami operator can be written using the trace of the iterated covariant derivative associated with the Levi-Civita connection. From this perspective, let Xi be a basis of tangent vector fields (not necessarily induced by a coordinate system). Then the Hessian of a function f is the symmetric 2-tensor whose components are given by

H(f)_{ij}=H_f(X_i, X_j) =\nabla_{X_i}\nabla_{X_j} f - \nabla_{\nabla_{X_i}X_j} f

This is easily seen to transform tensorially, since it is linear in each of the arguments Xi, Xj. The Laplace–Beltrami operator is then the trace of the Hessian with respect to the metric:

\Delta f = \sum_{ij} g^{ij} H(f)_{ij}.

In abstract indices, the operator is often written

\Delta f = \nabla^a \nabla_a f

provided it is understood implicitly that this trace is in fact the trace of the Hessian tensor.

Because the covariant derivative extends canonically to arbitrary tensors, the Laplace–Beltrami operator defined on a tensor T by

\Delta T = g^{ij}\left( \nabla_{X_i}\nabla_{X_j} T - \nabla_{\nabla_{X_i}X_j} T\right)

is well-defined.

Laplace–de Rham operator[edit]

More generally, one can define a Laplacian differential operator on sections of the bundle of differential forms on a pseudo-Riemannian manifold. On a Riemannian manifold it is an elliptic operator, while on a Lorentzian manifold it is hyperbolic. The Laplace–de Rham operator is defined by

\Delta= \mathrm{d}\delta+\delta\mathrm{d} = (\mathrm{d}+\delta)^2,\;

where d is the exterior derivative or differential and δ is the codifferential, acting as (−1)kn+n+1d on k-forms where ∗ is the Hodge star.

When computing Δƒ for a scalar function ƒ, we have δƒ = 0, so that

\Delta f = \delta \, df. \,

Up to an overall sign, The Laplace–de Rham operator is equivalent to the previous definition of the Laplace–Beltrami operator when acting on a scalar function; see the proof for details. On functions, the Laplace–de Rham operator is actually the negative of the Laplace–Beltrami operator, as the conventional normalization of the codifferential assures that the Laplace–de Rham operator is (formally) positive definite, whereas the Laplace–Beltrami operator is typically negative. The sign is a pure convention, however, and both are common in the literature. The Laplace–de Rham operator differs more significantly from the tensor Laplacian restricted to act on skew-symmetric tensors. Apart from the incidental sign, the two operators differ by a Weitzenböck identity that explicitly involves the Ricci curvature tensor.

Examples[edit]

Many examples of the Laplace–Beltrami operator can be worked out explicitly.

Euclidean space

In the usual (orthonormal) Cartesian coordinates xi on Euclidean space, the metric is reduced to the Kronecker delta, and one therefore has |g| = 1. Consequently, in this case

\Delta f = \frac{1}{\sqrt{|g|}} \partial_i \sqrt{|g|}\partial^i f = \partial_i \partial^i f

which is the ordinary Laplacian. In curvilinear coordinates, such as spherical or cylindrical coordinates, one obtains alternative expressions.

Similarly, the Laplace–Beltrami operator corresponding to the Minkowski metric with signature (−+++) is the D'Alembertian.

Spherical Laplacian

The spherical Laplacian is the Laplace–Beltrami operator on the (n − 1)-sphere with its canonical metric of constant sectional curvature 1. It is convenient to regard the sphere as isometrically embedded into Rn as the unit sphere centred at the origin. Then for a function ƒ on Sn−1, the spherical Laplacian is defined by

\Delta_{S^{n-1}}f(x) = \Delta f(x/|x|)

where ƒ(x/|x|) is the degree zero homogeneous extension of the function ƒ to Rn − {0}, and Δ is the Laplacian of the ambient Euclidean space. Concretely, this is implied by the well-known formula for the Euclidean Laplacian in spherical polar coordinates:

\Delta f = r^{1-n}\frac{\partial}{\partial r}\left(r^{n-1}\frac{\partial f}{\partial r}\right) + r^{-2}\Delta_{S^{n-1}}f.

More generally, one can formulate a similar trick using the normal bundle to define the Laplace–Beltrami operator of any Riemannian manifold isometrically embedded as a hypersurface of Euclidean space.

One can also give an intrinsic description of the Laplace–Beltrami operator on the sphere in a normal coordinate system. Let (tξ) be spherical coordinates on the sphere with respect to a particular point p of the sphere (the "north pole"), that is geodesic polar coordinates with respect to p. Here t represents the latitude measurement along a unit speed geodesic from p, and ξ a parameter representing the choice of direction of the geodesic in Sn−1. Then the spherical Laplacian has the form:

\Delta_{S^{n-1}} f(t,\xi) = \sin(t)^{2-n} \frac{\partial}{\partial t}\left(\sin(t)^{n-2}\frac{\partial f}{\partial t}\right) + \sin(t)^{-2}\Delta_\xi f

where \Delta_\xi is the Laplace–Beltrami operator on the ordinary unit (n − 2)-sphere. In particular, for the ordinary 2-sphere using standard notation for polar coordinates we get:

\Delta_{S^{2}} f(r,\theta) = \sin(r)^{-1} \frac{\partial}{\partial r}\left(\sin(r)\frac{\partial f}{\partial r}\right) + \sin(r)^{-2} \frac{\partial^2}{\partial \theta^2}f
Hyperbolic space

A similar technique works in hyperbolic space. Here the hyperbolic space Hn−1 can be embedded into the n dimensional Minkowski space, a real vector space equipped with the quadratic form

q(x) = x_1^2 - x_2^2-\cdots - x_n^2.

Then Hn is the subset of the future null cone in Minkowski space given by

H^n = \{ x | q(x) = 1, x_1>1\}. \,

Then

\Delta_{H^{n-1}} f = \Box f\left(x/q(x)^{1/2}\right)|_{H^{n-1}}

Here f(x/q(x)^{1/2}) is the degree zero homogeneous extension of f to the interior of the future null cone and □ is the wave operator

\Box = \frac{\partial^2}{\partial x_1^2} - \cdots - \frac{\partial^2}{\partial x_n^2}.

The operator can also be written in polar coordinates. Let (tξ) be spherical coordinates on the sphere with respect to a particular point p of Hn−1 (say, the center of the Poincaré disc). Here t represents the hyperbolic distance from p and ξ a parameter representing the choice of direction of the geodesic in Sn−1. Then the hyperbolic Laplacian has the form:

\Delta_{H^{n-1}} f(t,\xi) = \sinh(t)^{2-n} \frac{\partial}{\partial t}\left(\sinh(t)^{n-2}\frac{\partial f}{\partial t}\right) + \sinh(t)^{-2}\Delta_\xi f

where \Delta_\xi is the Laplace–Beltrami operator on the ordinary unit (n − 2)-sphere. In particular, for the hyperbolic plane using standard notation for polar coordinates we get:

\Delta_{H^{2}} f(r,\theta) = \sinh(r)^{-1} \frac{\partial}{\partial r}\left(\sinh(r)\frac{\partial f}{\partial r}\right) + \sinh(r)^{-2} \frac{\partial^2}{\partial \theta^2}f

See also[edit]

References[edit]