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Helmholtz decomposition

The Helmholtz decomposition of a vector field which is twice continuously differentiable, with rapid enough decay at infinity, splits the vector field into a sum of gradient and curl as follows:

\mathbf{F} = - \nabla\,\mathcal{G} (\nabla \cdot \mathbf{F}) + \nabla \times \mathcal{G}(\nabla \times \mathbf{F})

where \mathcal{G} represents the Newtonian potential.

If ∇·F=0, we say F is solenoidal or divergence-free and thus the Helmholtz decomposition of F collapses to

\mathbf{F} = \nabla \times \mathcal{G}(\nabla \times \mathbf{F}) = \nabla \times \mathbf{P}

In this case, P is known as the vector potential for F.

Likewise, if ∇×F=0 then F is said to be curl-free or irrotational and thus the Helmholtz decomposition of F collapses then to

\mathbf{F} =  - \nabla\,\mathcal{G} (\nabla \cdot \mathbf{F}) = - \nabla \phi

In this case, φ is known as the scalar potential for F.

01-04-2007 01:16:19
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