Clebsch representation

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In physics and mathematics, the Clebsch representation of an arbitrary three-dimensional vector field v(x) is:[1][2] v=∇φ+ψ∇χ,

where the scalar fields φ(x),ψ(x) and χ(x) are known as Clebsch potentials[3] or Monge potentials,[4] named after Alfred Clebsch (1833–1872) and Gaspard Monge (1746–1818), and ∇ is the gradient operator.

Background

In fluid dynamics and plasma physics, the Clebsch representation provides a means to overcome the difficulties to describe an inviscid flow with non-zero vorticity – in the Eulerian reference frame – using Lagrangian mechanics and Hamiltonian mechanics.[5][6][7] At the critical point of such functionals the result is the Euler equations, a set of equations describing the fluid flow. Note that the mentioned difficulties do not arise when describing the flow through a variational principle in the Lagrangian reference frame. In case of surface gravity waves, the Clebsch representation leads to a rotational-flow form of Luke's variational principle.[8]

For the Clebsch representation to be possible, the vector field v has (locally) to be bounded, continuous and sufficiently smooth. For global applicability v has to decay fast enough towards infinity.[9] The Clebsch decomposition is not unique, and (two) additional constraints are necessary to uniquely define the Clebsch potentials.[1] Since ψ∇χ is in general not solenoidal, the Clebsch representation does not in general satisfy the Helmholtz decomposition.[10]

Vorticity

The vorticity ω(x) is equal to[2]

ω=∇×v=∇×(∇φ+ψ∇χ)=∇ψ×∇χ,

with the last step due to the vector calculus identity ∇×(ψA)=ψ(∇×A)+∇ψ×A. So the vorticity ω is perpendicular to both ∇ψ and ∇χ, while further the vorticity does not depend on φ.

Notes

  1. ↑ 1.0 1.1 (Lamb 1993)
  2. ↑ 2.0 2.1 (Serrin 1959)
  3. ↑ (Benjamin 1984)
  4. ↑ (Aris 1962)
  5. ↑ (Clebsch 1859)
  6. ↑ (Bateman 1929)
  7. ↑ (Seliger Whitham)
  8. ↑ (Luke 1967)
  9. ↑ (Wesseling 2001)
  10. ↑ (Wu Ma)

References