In the constant-density incompressible equations, the normalized pressure p(t,x)p(t,x) is the physical pressure divided by the constant density. Its contribution to acceleration is

xp.-\nabla_xp.

Pressure is a scalar field; its is a vector field. In the evolution problem, pressure is an unknown enforcing compatibility with the incompressibility constraint.

Additive freedom

Replacing p(t,x)p(t,x) by p(t,x)+c(t)p(t,x)+c(t) leaves its spatial gradient unchanged. A normalization, such as zero spatial mean on a periodic domain, fixes this freedom. On a disconnected domain there can be one additive function of time on each component.

Regularity and reconstruction

To speak of a classical pressure gradient, the necessary spatial derivatives must exist. Pressure can instead be interpreted distributionally in weaker formulations. Taking the divergence of the momentum equation leads to a pressure Poisson equation, developed with the harmonic-analysis prerequisites.

References