Vector Laplacian/Proofs&o=10616

Vector Laplacian

In mathematics and physics, the vector Laplace operator, denoted by scriptstyle nabla^2, named after Pierre-Simon Laplace, is a differential operator defined over a vector field. The vector Laplacian is similar to the scalar Laplacian. Whereas the scalar Laplacian applies to scalar field and returns a scalar quantity, the vector Laplacian applies to the vector fields and returns a vector quantity.

Definition

The vector Laplacian of a vector field mathbf{A} is defined as

nabla^2 mathbf{A} = nabla(nabla cdot mathbf{A}) - nabla times (nabla times mathbf{A})

In Cartesian coordinates, this reduces to the much simpler form (see proof)

nabla^2 mathbf{A} = (nabla^2 A_x, nabla^2 A_y, nabla^2 A_z)

where A_x, A_y, and A_z are the components of mathbf{A}.

For expressions of the vector Laplacian in other coordinate systems see Nabla in cylindrical and spherical coordinates.

Generalization

The Laplacian of any tensor field T ("tensor" includes scalar and vector) is defined as the divergence of the gradient of the tensor:

nabla^2 T = nabla cdot (nabla T)

For the special case where T is a scalar (a tensor of rank zero), the Laplacian takes on the familiar form.

If T is a vector, the gradient is a covariant derivative which results in a tensor of second rank, and the divergence of this is again a vector (a tensor of first rank). The formula for the vector Laplacian above may be used to avoid tensor math and may be shown to be equivalent to the divergence of the gradient of the vector.

Use in physics

An example of the usage of the vector Laplacian is the Navier-Stokes equations for a Newtonian incompressible flow:

rho left(frac{partial mathbf{v}}{partial t}+ (mathbf{v} cdot nabla ) mathbf{v}right)=rho mathbf{f}-nabla p +muleft(nabla ^2 mathbf{v}right)

where the term with the vector Laplacian of the velocity field muleft(nabla ^2 mathbf{v}right) represents the viscous stresses in the fluid.

Another example is the wave equation for the electric field that can be derived from the Maxwell equations in the absence of charges and currents:

nabla^2 mathbf{E} - mu_0 epsilon_0 frac{partial^2 mathbf{E}}{partial t^2} = 0.

Previous equation can be written also as:

Box, mathbf{E} = 0,
where
Box=frac{1}{c^2} frac{partial^2}{partial t^2}-nabla^2,
is the D'Alembertian

See also

References

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