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]
Vorticity Created 2026-09-24 Updated 2026-10-13
Use vorticity to distinguish the local spin of a fluid element from the motion of its center along a pathline. Circular streamlines can occur both with and without vorticity: the two velocity fields below even have the same circulation around the unit circle.
Figure 1.
Solid-body rotation and a potential line vortex: equal unit-circle circulation, different local vorticity
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For a continuously differentiable velocity field , vorticity is the curl vector
Each partial derivative divides velocity by distance, so vorticity has units . In a planar velocity field independent of , only survives. Positive points along : the right-hand rule associates it with counterclockwise spin viewed from positive toward the plane. [ref]
The local rotational angular velocity is half the vorticity, . To see the factor, split the velocity gradient into its symmetric rate-of-strain tensor and antisymmetric spin tensor . A nearby displacement has relative velocity ; its rotational part satisfies . This is a proof outline of the local spin interpretation. The rate-of-strain tensor can also change the angle of a particular material line, so that line's angular velocity need not equal .
For solid-body rotation, gives and . Taking , the vorticity is , although the angular velocity is only . For the potential line vortex, , the planar curl is wherever . Its circular pathlines therefore coexist with zero local spin.
This distinction makes vorticity useful for recognizing shear flow as well as swirling motion; taking the curl of the Euler equations also removes a pressure gradient and leads to the vorticity equation. A historical landmark is Hermann von Helmholtz's 1858 paper on fluid vortex motion, an early study devoted to vortex dynamics. [ref]
For differentiable vector fields, the displayed identity relates vorticity to the antisymmetric part of the velocity gradient. Together with the curl of a cross product, it converts the adjoint linearized Navier-Stokes evolution between component and rotational forms.
Use a linear shear flow to see why straight pathlines can still carry local spin. Faster layers pull past slower ones, and a small symmetric paddle can turn clockwise while its center travels straight ahead.
Figure 1.
Straight particle paths in linear shear coexist with clockwise local spin and material-line deformation
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For the planar simple shear flow with constant signed shear rate , direct differentiation gives
With , these are and : both signs indicate clockwise orientation under the right-hand rule. Yet a particle initially at follows the straight pathline , . The curl measures differences of velocity between neighboring particles, rather than bending of one particle's pathline.
The velocity gradient has as its only nonzero entry. Its spin tensor supplies clockwise rotation, while its rate-of-strain tensor supplies simultaneous deformation. For a material line making angle to the horizontal, the equation gives . Initially horizontal and vertical material lines therefore have angular velocities and ; their mean is . At with , an initially vertical displacement becomes times its original length and has angle , a clockwise change of . The plotted cross deforms; an actual paddle's response also depends on its shape and interaction with the fluid. The exact local spin statement concerns the spin tensor, rather than every tracer's orientation.