Statement

For two smooth periodic incompressible Navier–Stokes solutions with common force and viscosity, or smooth whole-space solutions u,vC([0,T];H3(R3))u,v\in C([0,T];H^3(\mathbb R^3)) with common fC([0,T];L2)f\in C([0,T];L^2), let w=vuw=v-u. Then

w(t)22w(0)22exp ⁣(20tu(s)ds).\|w(t)\|_2^2\le\|w(0)\|_2^2 \exp\!\left(2\int_0^t\|\nabla u(s)\|_\infty\,ds\right).

In particular, the same initial velocity gives the same velocity on [0,T][0,T]. This is the classical difference-energy uniqueness estimate obtained from .

Energy calculation

The difference equation and integration cancellations give

12ddtw22+νw22=(w)uwuw22.\frac12\frac d{dt}\|w\|_2^2+\nu\|\nabla w\|_2^2 =-\int(w\cdot\nabla)u\cdot w \le\|\nabla u\|_\infty\|w\|_2^2.

On the torus, smoothness and periodicity justify the integration. In the whole-space case, H3H^3 controls u,u,v,vu,\nabla u,v,\nabla v in LL^\infty; the quadratic tensor lies in L2L^2, and the identified canonical pressure lies in L2L^2. Smooth approximation and expanding cutoffs justify the pairing and cancellation. The reference gradient is bounded on the compact time interval, so Gronwall applies. Equality of velocities determines pressure only up to a function of time.