For a , write e=∣u∣2/2e=|u|^2/2. Assume ∇u∈Lloc2\nabla u\in L^2_{\rm loc} and e,eu,pu,f⋅ue,eu,pu,f\cdot u are . The local energy inequality is

∂te+div⁡((e+p)u)−νΔe+ν∣∇u∣2≤f⋅u\partial_t e+\operatorname{div}((e+p)u)-\nu\Delta e +\nu|\nabla u|^2\leq f\cdot u

in distributions. Explicitly, every nonnegative ϕ∈Cc∞(Q)\phi\in C_c^\infty(Q) satisfies

ν∫Q∣∇u∣2ϕ≤∫Qe(∂tϕ+νΔϕ)+(e+p)u⋅∇ϕ+f⋅u ϕ.\nu\int_Q|\nabla u|^2\phi\leq\int_Q e(\partial_t\phi+\nu\Delta\phi)+(e+p)u\cdot\nabla\phi+f\cdot u\,\phi.

It permits extra energy loss relative to the .

Local and global statements

Tests have compact support inside space-time. Obtaining a global energy inequality requires cutoff limits and endpoint information; the two definitions are not interchangeable without those arguments.