Newtonian Fluids

A Newtonian fluid is described by an explicit constitutive equation that relates the viscous stress tensor T to the velocity field through a constant viscosity. The relation between the shear stress and the shear rate is linear.

The viscous stress tensor in Eqn. (656) is not constant, but a variable function of the velocity field for a particular fluid. Typically, in a constitutive relation, the velocity field is expressed in the form of the rate of deformation tensor:
Figure 1. EQUATION_DISPLAY
D = 1 2 ( v + ( v ) T )
(695)

Newtonian fluid is the simplest mathematical model to describe the viscous behavior of many liquids and gases such as water and air.

The stress tensor is given by:

Figure 2. EQUATION_DISPLAY
T=2μD-23μ(v)I
(696)

where μ is the constant dynamic viscosity of the fluid and D is the rate of deformation (strain) tensor given by Eqn. (695). For incompressible flows, the second term in Eqn. (696) is zero due to the continuity equation.

Temperature-Dependent Newtonian Viscosity

For gases, the viscosity can be a function of temperature.

Sutherland's Law
The Sutherland equation is a widely used approximation for modeling the dependence of gas viscosity on temperature:
Figure 3. EQUATION_DISPLAY
μ μ 0 = ( T T 0 ) 3 2 ( T 0 + S T + S )
(697)

Here, S is an effective temperature, called the Sutherland constant, and μ 0 is the reference viscosity at the reference temperature T 0 = 273 K

Power Law

For dilute gases, the temperature-dependent viscosity can be approximated by a power-law:

Figure 4. EQUATION_DISPLAY
μ μ 0 = ( T T 0 ) n
(698)

where T 0 is the reference temperature, μ 0 is the reference viscosity and n is the Power law exponent.