Navier-Stokes Equations

Interactive Lecture

Understanding Fluid Flow Through Conservation Laws

by Dr Arnaldo Delli Carri

Understanding the Navier-Stokes Equations

What are the Navier-Stokes Equations?

The Navier-Stokes equations are the fundamental governing equations of fluid mechanics, describing the motion of viscous fluids. They express Newton's second law for fluid elements, accounting for pressure gradients, viscous forces, and body forces.

The Navier-Stokes equations represent conservation of momentum for a fluid continuum. Combined with mass conservation (continuity equation) and energy conservation, they form a complete system for predicting fluid behaviour — from aircraft aerodynamics to blood flow.

Conservation of Mass (Continuity Equation)

For an incompressible fluid, the continuity equation simplifies to:

\[\nabla \cdot \vec{u} = \frac{\partial u}{\partial x} + \frac{\partial v}{\partial y} + \frac{\partial w}{\partial z} = 0\]

This states that the divergence of the velocity field must be zero for incompressible flow.

Conservation of Momentum (Navier-Stokes)

The momentum equation for an incompressible Newtonian fluid is:

Vector Form:

\[\rho\left(\frac{\partial \vec{u}}{\partial t} + \vec{u} \cdot \nabla \vec{u}\right) = -\nabla p + \mu \nabla^2 \vec{u} + \rho \vec{g}\]

where:

Component Form (2D):

\[\rho\left(\frac{\partial u}{\partial t} + u\frac{\partial u}{\partial x} + v\frac{\partial u}{\partial y}\right) = -\frac{\partial p}{\partial x} + \mu\left(\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}\right)\]

\[\rho\left(\frac{\partial v}{\partial t} + u\frac{\partial v}{\partial x} + v\frac{\partial v}{\partial y}\right) = -\frac{\partial p}{\partial y} + \mu\left(\frac{\partial^2 v}{\partial x^2} + \frac{\partial^2 v}{\partial y^2}\right)\]

Reynolds Number

The Reynolds number characterises the flow regime and indicates the relative importance of inertial forces to viscous forces:

\[Re = \frac{\rho U L}{\mu} = \frac{UL}{\nu}\]

where:

Flow Regimes:

Vorticity

Vorticity measures the local rotation of fluid elements and is defined as the curl of the velocity field:

\[\vec{\omega} = \nabla \times \vec{u}\]

In 2D: \(\omega_z = \frac{\partial v}{\partial x} - \frac{\partial u}{\partial y}\)

The vorticity transport equation is:

\[\frac{\partial \omega}{\partial t} + \vec{u} \cdot \nabla \omega = \nu \nabla^2 \omega\]

Simplified Solutions

For certain flow conditions, the Navier-Stokes equations can be simplified:

Common Simplifications:

Interactive Simulation: Vortex Shedding Behind a Cylinder

What This Simulation Shows:

This simulation demonstrates vortex shedding (von Kármán vortex street) — a fundamental phenomenon predicted by the Navier-Stokes equations. When fluid flows past an obstacle at moderate Reynolds numbers, vortices alternately form and detach from either side, creating an oscillating wake pattern.

The coloured particles are passive tracers that move with the fluid, visualising the velocity field. Red particles show clockwise rotation, blue shows counterclockwise rotation.

1.5
0.01
0.4
800

Engineering Applications

The Navier-Stokes equations underpin whole branches of engineering:

Summary of Key Equations

Concept Equation Description
Continuity (Incompressible) \(\nabla \cdot \vec{u} = 0\) Mass conservation
Navier-Stokes (Vector) \(\rho\left(\frac{\partial \vec{u}}{\partial t} + \vec{u} \cdot \nabla \vec{u}\right) = -\nabla p + \mu \nabla^2 \vec{u} + \rho \vec{g}\) Momentum conservation
Reynolds Number \(Re = \frac{\rho U L}{\mu} = \frac{UL}{\nu}\) Ratio of inertial to viscous forces
Vorticity \(\vec{\omega} = \nabla \times \vec{u}\) Local rotation of fluid elements
Vorticity Transport \(\frac{\partial \omega}{\partial t} + \vec{u} \cdot \nabla \omega = \nu \nabla^2 \omega\) Evolution of vorticity
Strouhal Number \(St = \frac{fD}{U}\) Vortex shedding frequency (≈0.2 for cylinders)

Practice Problems

Problem 1: Reynolds Number Calculation

Water (ν = 1.0 × 10⁻⁶ m²/s) flows through a pipe of diameter D = 0.05 m at a velocity of U = 2 m/s. Calculate the Reynolds number and determine if the flow is laminar or turbulent. If the pipe diameter is doubled while maintaining the same flow rate, how does the Reynolds number change?

Show Solution

Problem 2: Pressure Drop in Pipe Flow

For laminar flow in a circular pipe, the Hagen-Poiseuille equation gives the pressure drop: \(\Delta p = \frac{32 \mu L U}{D^2}\). Calculate the pressure drop for oil (μ = 0.1 Pa·s) flowing at U = 0.5 m/s through a 10 m long pipe with D = 0.02 m. Verify that the flow is indeed laminar (assume ρ = 900 kg/m³).

Show Solution

Problem 3: Vortex Shedding Frequency

A chimney with diameter D = 2 m is exposed to wind at U = 15 m/s. Using the Strouhal number relationship \(St = fD/U \approx 0.2\) for cylinders, calculate the vortex shedding frequency. If the chimney has a natural frequency of 0.8 Hz, is there a risk of resonance?

Show Solution

Knowledge Check Quiz

Question 1: What does the Reynolds number represent?

Question 2: For incompressible flow, the continuity equation states:

Question 3: What is vorticity?

Question 4: Vortex shedding behind a cylinder typically begins when:

Question 5: In the Navier-Stokes equations, the term μ∇²u represents: