The Navier-Stokes equations describe the motion of fluid substances such as liquids and gases. They are a set of nonlinear partial differential equations that arise from applying Newton's second law to fluid motion, incorporating the effects of viscosity. Below, we will derive the Navier-Stokes equation and solve it for a simple case.
The Navier-Stokes equations can be derived from the principles of conservation of momentum and mass. The general form for an incompressible fluid is given by:
ρ(∂u/∂t + u · ∇u) = -∇p + μ∇²u + f
Where:
The equation can be broken down into the following components:
u · ∇u
∂u/∂t
-∇p
μ∇²u
f
For illustrative purposes, let's simplify the Navier-Stokes equations by considering a two-dimensional, incompressible, steady flow in a rectangular channel with no external forces. We can express the Navier-Stokes equations as follows:
ρ(∂u/∂t + u ∂u/∂x + v ∂u/∂y) = -∂p/∂x + μ(∂²u/∂x² + ∂²u/∂y²)
Assuming steady state (∂u/∂t = 0) and uniform density, we can simplify this to:
0 = -∂p/∂x + μ(∂²u/∂x² + ∂²u/∂y²)
Rearranging gives us:
∂p/∂x = μ(∂²u/∂x² + ∂²u/∂y²)
To solve this equation, we can apply boundary conditions. For instance, if we consider a flow in a channel where:
Let’s take a simple case where the velocity profile is parabolic, typical of laminar flow in a channel:
u(y) = Umax(1 - (y/h)²)
where Umax is the maximum velocity at the center of the channel.
Using the parabolic velocity profile, we can substitute into our equation:
∂²u/∂y² = -2Umax/h²
Now substituting this back into our rearranged Navier-Stokes equation:
∂p/∂x = μ(-2Umax/h²)
This implies that the pressure gradient is constant along the channel:
p(x) = -2μUmax/h² * x + C
where C is a constant determined by boundary conditions.
The Navier-Stokes equations are fundamental to fluid mechanics and can be quite complex depending on the flow regime and boundary conditions. The example provided illustrates a basic scenario of laminar flow in a channel, leading to a parabolic velocity profile and a linear pressure gradient.
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