Laplace operator

In mathematics and physics, the Laplace operator or Laplacian, denoted by Δ, is a differential operator, specifically an important case of an elliptic operator (or a hyperbolic operator when defined on pseudo-Riemannian manifolds), with many applications in mathematics and physics. In physics, it is used in modeling of wave propagation and heat flow; it occurs in the Helmholtz equation; it is central in electrostatics and represents the kinetic energy term of the Schrödinger equation. In mathematics, functions with vanishing Laplacian are called harmonic functions; the Laplacian is at the core of Hodge theory and the results of de Rham cohomology.



The Laplace operator is a second order differential operator, defined as the divergence of the gradient:

<math>\Delta = \nabla^2 = \nabla \cdot \nabla <math>

In the n-dimensional Euclidean space, it is the sum of all the unmixed second partial derivatives:

<math>\Delta = \sum_{i=1}^n \frac {\partial^2}{\partial x^2_i}<math>.

Here, it is understood that the <math>x_i<math> are Cartesian coordinates on the space; the equation takes a different form in spherical coordinates and cylindrical coordinates, as shown below.

In the three-dimensional space the Laplacian is commonly written as

<math>\Delta =

\frac{\partial^2} {\partial x^2} + \frac{\partial^2} {\partial y^2} + \frac{\partial^2} {\partial z^2}. <math>

The Laplacian can be generalized to non-Euclidean spaces, where it may be elliptic or hyperbolic. For example, in the Minkowski spacetime the Laplacian becomes the d'Alembert operator or d'Alembertian

<math>\square =

{\partial^2 \over \partial x^2 } + {\partial^2 \over \partial y^2 } + {\partial^2 \over \partial z^2 } - \frac {1}{c^2}{\partial^2 \over \partial t^2 } <math>

This operator is often used to express the Klein-Gordon equation and the four-dimensional wave equation. The sign in front of the fourth term is negative, while it would have been positive in the Euclidean space. The additional factor of c is required because space and time are usually measured in different units; a similar factor would be required if, for example, the x direction was measured in inches, and the y direction was measured in centimeters. Indeed, physicists usually work in units such that c=1 in order to simplify the equation.

Coordinate expressions

In three dimensions, it is common to work with the Laplacian in a variety of different coordinate systems. Given a function f, in cylindrical coordinates, one has:

<math> \Delta f

= {1 \over r} {\partial \over \partial r}

 \left( r {\partial f \over \partial r} \right) 

+ {1 \over r^2} {\partial^2 f \over \partial \phi^2} + {\partial^2 f \over \partial z^2 }. <math>

In spherical coordinates:

<math> \Delta f

= {1 \over r^2} {\partial \over \partial r}

 \left( r^2 {\partial f \over \partial r} \right) 

+ {1 \over r^2 \sin \theta} {\partial \over \partial \theta}

 \left( \sin \theta {\partial f \over \partial \theta} \right) 

+ {1 \over r^2 \sin^2 \theta} {\partial^2 f \over \partial \phi^2}. <math>

The spherical coordinates Laplacian can also be written in this form:

<math> \Delta f

= {1 \over r} {\partial^2 \over \partial r^2}

 \left( rf \right) 

+ {1 \over r^2 \sin \theta} {\partial \over \partial \theta}

 \left( \sin \theta {\partial f \over \partial \theta} \right) 

+ {1 \over r^2 \sin^2 \theta} {\partial^2 f \over \partial \phi^2}. <math>

See also the article Nabla in cylindrical and spherical coordinates.


If f and g are functions, then the Laplacian of the product is given by

<math>\Delta(fg)=(\Delta f)g+2(\nabla f)\cdot(\nabla g)+f(\Delta g).<math>

Laplace-Beltrami operator

The Laplacian can also be defined on curved surfaces, or more generally, on Riemannian and pseudo-Riemannian manifolds. One defines this operator, as before, as the divergence of the gradient. To be able to find a formula for this operator, one will need to first write the divergence and the gradient on the manifold.

If <math>g<math> denotes the (pseudo)-metric tensor on the manifold, one finds that the volume form in local coordinates is given by

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

where the <math>dx^i<math> are the 1-forms forming the dual basis to the basis vectors

<math>\partial_i := \frac {\partial}{\partial x^i}<math>

for the local coordinate system, and <math>\wedge<math> is the wedge product. Here <math>|g|:=|\det g|<math> is the absolute value of the determinant of the metric tensor. The divergence of a vector field X on the manifold can then be defined as

<math>\mathcal{L}_X \mathrm{vol}_n = (\mbox{div} X) \; \mathrm{vol}_n<math>

where <math>\mathcal{L}_X<math> is the Lie derivative along the vector field X. In local coordinates, one obtains

<math>\mbox{div} X = \frac{1}{\sqrt{|g|}} \partial_i \sqrt {|g|} X^i

<math> Here (and below) we use the Einstein notation, so the above is actually a sum in i.

The gradient of a scalar function f may be defined through the inner product <math>\langle\cdot,\cdot\rangle<math> on the manifold, as

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

for all vectors <math>v_x<math> anchored at point x in the tangent bundle <math>T_xM<math> of the manifold at point x. Here, df is the exterior derivative of the function f; it is a 1-form taking argument <math>v_x<math>. In local coordinates, one has

<math> \left(\mbox{grad} f\right)^i =

\partial^i f = g^{ij} \partial_j f<math>

Combining these, one can express the Laplacian of a scalar function f in local coordinates as

<math>\Delta f = \mbox{div grad} \; f =

\frac{1}{\sqrt {|g|}} \partial_i \sqrt{|g|} \partial^i f<math>.

Here, <math>g^{ij}<math> are the components of the inverse of the metric tensor <math>g<math>, so that <math>g^{ij}g_{jk}=\delta^i_k<math> with <math>\delta^i_k<math> the Kronecker delta.

When defined in this way, the Laplacian is more commonly called the Laplace-Beltrami operator. Note that the above definition is, by construction, valid only for scalar functions <math>f:M\rightarrow \mathbb{R}<math>. One may want a more general definition of a Laplacian, valid for k-forms as well as scalar functions; for this, one must turn to the Laplace-deRham operator, defined in the next section.

One may show that the Laplace-Beltrami operator reduces to the ordinary Laplacian in Euclidean space by noting that it can be re-written using the chain rule as

<math>\Delta f = \partial_i \partial^i f + (\partial^i f) \partial_i \ln \sqrt{|g|}.<math>

When <math>|g| = 1<math>, such as in the case of Euclidean space, one then easily obtains

<math>\Delta f = \partial_i \partial^i f<math>

which is the ordinary Laplacian. Using the Minkowski metric with signature (+++-), one regains the D'Alembertian given previously. Note also that by using the metric tensor for spherical and cylindrical coordinates, one can similarly regain the expressions for the Laplacian in spherical and cylindrical coordinates. The Laplace-Beltrami operator is handy not just in curved space, but also in ordinary flat space endowed with a non-linear coordinate system.

Note that the exterior derivative d and -div are adjoint:

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

where the last equality is an application of Stokes theorem. Note also, the Laplace-Beltrami operator is symmetric:

<math>\int_M f\Delta h \;\mathrm{vol}_n =

\int_M \langle \mbox{grad} f, \mbox{grad} h \rangle \;\mathrm{vol}_n = \int_M h\Delta f \;\mathrm{vol}_n<math>

for functions f and h.

Laplace-de Rham operator

In the general case of differential geometry, one defines the Laplace-de Rham operator as the generalization of the Laplacian. It is a differential operator on the exterior algebra of a differentiable manifold. On a Riemannian manifold it is an elliptic operator, while on a pseudo-Riemannian manifold it is hyperbolic. The Laplace-de Rham operator is defined by

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

where d is the exterior derivative or differential and δ is the codifferential. When acting on scalar functions, the codifferential may be defined as δ = −*d*, where * is the Hodge star; more generally, the codifferential may include a sign that depends on the order of the k-form being acted on.

One may prove that the Laplace-de Rahm operator is equivalent to the previous definition of the Laplace-Beltrami operator when acting on a scalar function f; see the Laplace operator article proofs for details. Notice that the Laplace-de Rham operator is actually minus the Laplace-Beltrami operator; this minus sign follows from the conventional definition of the properties of the codifferential. Unfortuanatly, Δ is used to denote both; which can sometimes be a source of confusion.


Given scalar functions f and h, and a real number a, the Laplace-de Rham operator has the following properties:

  1. <math>\Delta(af + h) = a\Delta f + \Delta h\!<math>
  2. <math>\Delta(fh) = f \Delta h + 2 \partial_i f \partial^i h + h \Delta f<math>    (proof)

See also

External links


  • Charles W. Misner, Kip S. Thorne, John Archibald Wheeler, Gravitation, (1970) W.H. Freeman, New York; ISBN 0-7167-0344-0. (Provides a basic review of differential geometry in the special case of four-dimensional space-time.)
  • Jurgen Jost, Riemannian Geometry and Geometric Analysis, (2002) Springer-Verlag, Berlin ISBN 3-540-4267-2 . (Provides a general introduction to curved surfaces).de:Laplace-Operator

fr:Opérateur laplacien it:Operatore di Laplace nl:Laplaceoperator pl:Laplasjan sl:Laplaceov operator sv:Laplaceoperatorn tr:Laplasyen


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