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=πœ΅Ο†+Οˆπœ΅Ο‡,

where the scalar fields Ο†(𝒙),ψ(𝒙) and Ο‡(𝒙) are known as Clebsch potentials[3] or Monge potentials,[4] named after Alfred Clebsch (1833–1872) and Gaspard Monge (1746–1818), and 𝜡 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 Οˆπœ΅Ο‡ 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=πœ΅Γ—π’—=πœ΅Γ—(πœ΅Ο†+Οˆπœ΅Ο‡)=πœ΅ΟˆΓ—πœ΅Ο‡,

with the last step due to the vector calculus identity πœ΅Γ—(Οˆπ‘¨)=ψ(πœ΅Γ—π‘¨)+πœ΅ΟˆΓ—π‘¨. So the vorticity 𝝎 is perpendicular to both 𝜡ψ and πœ΅Ο‡, while further the vorticity does not depend on Ο†.

Notes

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References

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