A Reynolds defect system, with the right-hand-side sign convention, is

∂tv+div⁡(v⊗v)+∇p=νΔv+f+div⁡R,div⁡v=0.\partial_t v+\operatorname{div}(v\otimes v)+\nabla p =\nu\Delta v+f+\operatorname{div}R,\qquad \operatorname{div}v=0.

Here R(x,t)R(x,t) is a , its is (div⁡R)i=∑j∂jRij(\operatorname{div}R)_i=\sum_j\partial_jR_{ij}, and v⊗vv\otimes v is an . For ν>0\nu>0 this is called Navier–Stokes–Reynolds; for ν=0\nu=0, Euler–Reynolds. The is recovered when the defect divergence vanishes.

The pressure term is its and Δ\Delta is the componentwise .

Pressure and trace

Writing R=R∘+rIR=R^\circ+rI with r=tr⁡R/nr=\operatorname{tr}R/n, replace pp by p−rp-r to use the trace-free tensor R∘R^\circ. Thus trace parts can be put into pressure. The sign of a tensor called Reynolds stress must be checked against its displayed equation.