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Reynolds transport theorem

3D generalization of the Leibniz integral rule

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Through Divergence theorem

Consider integrating f = f(x,t) over the time-dependent region Ω(t) that has boundary ∂Ω(t), then taking the derivative with respect to time: ddt∫Ω(t)fdV. If we wish to move the derivative into the integral, there are two issues: the time dependence of f, and the introduction of and removal of space from Ω due to its dynamic boundary. Reynolds transport theorem provides the necessary framework.

General form

The Reynolds transport theorem can be expressed as follows: ddt∫Ω(t)fdV=∫Ω(t)∂f∂tdV+∫∂Ω(t)(vb⋅n)fdA in which n(x,t) is the outward-pointing unit normal vector, x is a point in the region and is the variable of integration, dV and dA are volume and surface elements at x, and vb(x,t) is the velocity of the area element (not the flow velocity). The function f may be tensor-, vector- or scalar-valued. Note that the integral on the left hand side is a function solely of time, and so the total derivative has been used.

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