Math 2.0

Fluid mechanics Definition

Newtonian fluid

Builds on ViscosityStrain rate tensorTrace of a matrixIncompressible flowNavier–Stokes equations

Definition

Consider a fluid with pressure pp, velocity field 𝐮\mathbf{u} and strain rate tensor EE. Let II be the 3×33 \times 3 identity matrix, and note that the trace of EE is tr⁡E=∇⋅𝐮\tr E = \nabla \cdot \mathbf{u}. The fluid is Newtonian if its Cauchy stress tensor σ\sigma has the form σ=−pI+2μE+λ (tr⁡E) I.\sigma = -p I + 2 \mu E + \lambda \, (\tr E) \, I. Here μ\mu is the dynamic viscosity and λ\lambda is a second coefficient. Both may depend on the thermodynamic state but not on EE.

Remarks

The form is the general isotropic stress that is linear in EE. For an incompressible flow, tr⁡E=0\tr E = 0 and the law becomes σ=−pI+2μE\sigma = -p I + 2 \mu E. Example: in the simple shear flow 𝐮=(γ˙y,0,0)\mathbf{u} = (\dot\gamma y, 0, 0), E12=γ˙/2E_{12} = \dot\gamma / 2, so the shear stress is σ12=μγ˙\sigma_{12} = \mu \dot\gamma, proportional to the shear rate. Non-example: a power-law fluid with shear stress τ=Kγ˙m\tau = K \dot\gamma^{m} for a constant m≠1m \ne 1 is not Newtonian, since its stress is not linear in the shear rate. Substituting the Newtonian law into the balance of momentum gives the Navier–Stokes equations.

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To understand this page from the ground up, read these 6 pages in order. The foundations come first.

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  1. Incompressible flow concept
  2. Navier–Stokes equations concept
  3. Strain rate tensor concept
  4. Trace of a matrix concept
  5. Viscosity concept
  6. Newtonian fluid definition

Further reading

  1. Web https://en.wikipedia.org/wiki/Newtonian_fluid
About this page
TagKVRVGFMAYJ
URIm2://KVRVGFMAYJ
Kinddefinition
WritingW0 stub
MSC76A02, 76D05
DefinesNewtonian fluid
UsesViscosity, Strain rate tensor, Trace of a matrix, Incompressible flow, Navier–Stokes equations
Changed3 November 2026

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