Fluid Flow

Simcenter STAR-CCM+ can simulate internal and external fluid flow across a wide range of flow regimes, and for a variety of fluid types. It solves the conservation equations for mass, momentum, and energy for general incompressible and compressible fluid flows.

Equations of Fluid Flow

When integrating Eqn. (654), Eqn. (656), and Eqn. (658) over a finite control volume, the governing equations of fluid flow can be written as:
Continuity Equation
Figure 1. EQUATION_DISPLAY
tVρdV+Aρvda=VSudV
(664)
where:
  • t is time.
  • V is volume.
  • a is the area vector.
  • ρ is the density.
  • v is the velocity.
  • Su is a user-specified source term.
Momentum Equation
Figure 2. EQUATION_TITILE
tVρvdV+Aρvvd= ApIda+ATda+VfbdV+VsudV
(665)
where:
  • p is pressure.
  • T is the viscous stress tensor.
  • fb is the resultant of body forces.
  • su is a user-specified source term.
Energy Equation
Figure 3. EQUATION_TITLE
t V ρ E d V + A ρ H v d a = - A q d a + A T v d a + V f b v d V + V S u d V
(666)
where:
  • E is the total energy.
  • H is the total enthalpy.
  • q is the heat flux.

Constitutive Relations

In order to solve the momentum equations for the velocity field, closure must be provided between the stress tensor and the velocity field of the fluid. A large number of constitutive equations exist that incorporate different material properties of the fluid such as viscosity, first and second normal stress coefficient. In addition, the equations of state, which are also constitutive relations, are required for the closure of the system of equations that is described above.