Reynolds transport theorem


Introduction

Reynolds transport theoremMathworldPlanetmath [1] is a fundamental theorem used in formulating the basic laws of fluid mechanics. We will enunciate and demonstrate in this entry the referred theorem. For our purpose, let us consider a fluid flow, characterized by its streamlines, in the Euclidean vector space (ℝ3,∥⋅∥) and embedded on it we consider, a continuum body ℬ occupying a volume 𝒱 whose particles are fixed by their material (Lagrangian) coordinatesPlanetmathPlanetmath 𝐗, and a region ℜ where a control volume 𝔳 is defined whose points are fixed by it spatial (Eulerian) coordinates 𝐱 and bounded by the control surface ∂⁡𝔳. An arbitrary tensor field of any rank is defined over the fluid flow according to the following definition.

Definition 1.

We call an extensive tensor property to the expression

Ψ⁢(𝐱,t):=∫𝔳ψ⁢(𝐱,t)⁢ρ⁢(𝐱,t)⁢𝑑v, (1)

where ψ⁢(x,t) is the respective intensive tensor property.

Theorem’s hypothesis

The kinematics of the continuum can be described by a diffeomorphism χ which, at any given instant t∈[0,∞)⊂ℝ, gives the spatial coordinates 𝐱 of the material particle 𝐗,

𝒱×[0,∞)→𝔳×[0,∞),t↦t,𝐗↦𝐱=χ⁢(𝐗,t).

Indeed the above sentence corresponds to a change of coordinates which must verify

J=|∂⁡xi∂⁡Xj|≡|Fi⁢j|≠0,Fi⁢j:=∂⁡xi∂⁡Xj,

J being the JacobianMathworldPlanetmathPlanetmath of transformation and Fi⁢j the Cartesian components of the so-called strain gradientMathworldPlanetmath tensor 𝐅.

Reynolds transport theorem 1.

The material rate of an extensive tensor property associate to a continuum body B is equal to the local rate of such property in a control volume v plus the efflux of the respective intensive property across its control surface ∂⁡v.

Proof.

By taking on Eq.(1) the material time derivative,

D⁢ΨD⁢t=Ψ˙=∫𝔳ψ⁢ρ⁢𝑑v¯˙=∫𝒱ψ⁢ρ⁢J⁢𝑑V¯˙=∫𝒱ψ⁢ρ⁢J¯˙⁢𝑑V=∫𝒱(ψ⁢ρ¯˙⁢J+ψ⁢ρ⁢J˙)⁢𝑑V=
∫𝒱{J⁢[∂∂⁡t⁢(ψ⁢ρ)+𝐯⋅∇x⁡(ψ⁢ρ)]+ψ⁢ρ⁢(J⁢∇x⋅𝐯)}⁢𝑑V=∫𝒱{[∂∂⁡t⁢(ψ⁢ρ)]+[𝐯⋅∇x⁡(ψ⁢ρ)+(ψ⁢ρ)⁢∇x⋅𝐯]}⁢(J⁢d⁢V)
=∫𝔳∂∂⁡t⁢(ψ⁢ρ)⁢𝑑v+∫𝔳∇x⋅(ψ⁢ρ⁢𝐯)⁢𝑑v=∂∂⁡t⁢∫𝔳ψ⁢ρ⁢𝑑v+∫∂⁡𝔳ψ⁢ρ⁢𝐯⋅𝐧⁢𝑑a,

since ∂t⁡(d⁢v)=0 (𝐱 fixed) on the first integral and by applying the Gauss-Green divergence theoremMathworldPlanetmathPlanetmath on the second integral at the left-hand side. Finally, by substituting Eq.(1) on the first integral at the right-hand side, we obtain

Ψ˙=∂⁡Ψ∂⁡t+∫∂⁡𝔳ψ⁢ρ⁢𝐯⋅𝐧⁢𝑑a, (2)

endorsing the theorem statement. ∎

References

  • 1 O. Reynolds, Papers on mechanical and physical subjects-the sub-mechanics of the Universe, Collected Work, Volume III, Cambridge University Press, 1903.
Title Reynolds transport theorem
Canonical name ReynoldsTransportTheorem
Date of creation 2013-03-22 16:00:48
Last modified on 2013-03-22 16:00:48
Owner perucho (2192)
Last modified by perucho (2192)
Numerical id 7
Author perucho (2192)
Entry type Theorem
Classification msc 53A45