Vector field Created 2026-09-24 Updated 2026-10-03
A vector field assigns a vector to every point of its domain.
Velocity potential Created 2026-09-24 Updated 2026-10-13
Use a velocity potential to reconstruct an irrotational flow from one scalar field. A velocity potential satisfies
It has units and is unchanged as a description of the velocity field when any function of time alone is added. For twice continuously differentiable , the identity curl of a gradient proves zero vorticity. In incompressible flow, taking the divergence also gives , the Laplace equation. This turns a three-component velocity field into a single harmonic function with appropriate boundary conditions. [ref]
For uniform flow , take . With , the change from to is . By the fundamental theorem for line integrals, the line integral of velocity between these points equals that change along any path in the domain; a closed curve gives zero circulation.
For the potential line vortex, choose a local angle branch in polar coordinates and set . Then and . One counterclockwise turn changes the continued velocity potential by , although the velocity field returns to its original value. With , this change is , exactly the circulation. A full annulus therefore admits local angle branches and a multivalued velocity potential, but no global single-valued velocity potential when . Cutting the annulus along a radial line allows a single-valued angle branch on the remaining domain. The obstruction is path independence, not a failure of the local gradient formula.
Let be bounded, connected and simply connected, and let be a smooth divergence-free field. Suppose a sufficiently smooth vector field satisfies the displayed Poisson and boundary conditions. Divergence gives with zero boundary value, so harmonic uniqueness gives . The vector Laplacian identity then implies .
On a simply connected domain, define a scalar potential by integrating this curl-free difference along a path from a fixed point. Vanishing circulation around contractible loops proves path independence. Thus the difference is ; its divergence and boundary normal component give and . Green's identity yields , proving the reconstruction. Additional conditions on can specify its own boundary problem; the argument assumes its existence and proves that its curl is exactly . Simple connectivity is essential for eliminating possible non-gradient harmonic circulation fields.
Velocity-space divergence 2026-10-25
The divergence with respect to velocity coordinates, with position held fixed. In dimensions, has . A kinetic conservation law must retain this term for velocity-dependent forces.
Viscous stress tensor Created 2026-09-28 Updated 2026-10-14
The viscous stress tensor is the part of the Cauchy stress tensor associated with deformation rates. For an isotropic Newtonian fluid in incompressible flow,
Here is pressure, is the identity matrix, is dynamic viscosity, and is the strain-rate tensor. The convention is ; denotes transpose and denotes trace. Across a plane with unit normal vector , the viscous traction is . The tensor makes this rule work for any plane orientation. [ref]
In the worked Couette flow, , so
In particular, while the shear rate is ; the factor in recovers . On the upper face of a fluid slice, gives viscous traction ; on the lower face it is . Constant stress can therefore transmit a force between the plates even though its divergence, and the net viscous force on each slice, vanish.
Compare planar extension with solid-body rotation :
Extension changes lengths and produces viscous normal stresses . Rotation preserves distances and gives zero viscous stress, despite its nonzero velocity gradient and vorticity . For and , extension gives and ; rotation gives zero. A rotating fluid may still have a pressure gradient supplying its centripetal acceleration.
Figure 1.
Deformation produces Newtonian viscous stress; rigid rotation does not
. Blue arrows show instantaneous velocity. The dashed square is a material patch at ; its orange outline at is obtained from the exact trajectories of planar extension and solid-body rotation, with . The marked corner makes rotation visible. Both motions preserve area, but only extension changes the patch's shape. Details.
For an isotropic Newtonian fluid in three-dimensional compressible flow, separate shape change from volume change:
The first term is deviatoric stress, with zero trace; is volume viscosity, also called bulk viscosity. For uniform expansion , and , so the shear contribution vanishes and the viscous stress is . Thus dynamic viscosity and volume viscosity describe distinct responses, and incompressible flow removes only the volume-change term. [ref]
Volume integral 2026-10-14
A volume integral integrates a scalar or componentwise vector field over a three-dimensional region with its volume form. In spherical polar coordinates the Euclidean volume form is . The divergence theorem relates a volume integral of a divergence to a boundary flux integral.
Weak divergence 2026-10-25
The divergence defined through weak derivatives: pair a locally integrable vector field with a smooth compactly supported test function using the displayed integration-by-parts identity. A piecewise smooth field can have a surface contribution where its normal component jumps. Thus zero classical divergence on each side does not imply zero weak divergence across the interface.