Categories: Fluid dynamics, Fluid mechanics, Physics.

# Vorticity

In fluid mechanics, the **vorticity** $\va{\omega}$
is a measure of the local circulation in a fluid.
It is defined as the curl of the flow velocity field $\va{v}$:

Just as curves tangent to $\va{v}$ are called *streamlines*,
curves tangent to $\va{\omega}$ are **vortex lines**,
which are to be interpreted as the “axes” that $\va{v}$ is circulating around.

The vorticity is a local quantity,
and the corresponding global quantity is the **circulation** $\Gamma$,
which is defined as the projection of $\va{v}$ onto a close curve $C$.
Then, by Stokes’ theorem:

## Ideal fluids

For an inviscid, incompressible fluid,
consider the *Bernoulli field* $H$, which is defined as:

Where $\Phi$ is the gravitational potential, $p$ is the pressure, and $\rho$ is the (constant) density. We then take the gradient of this scalar field:

$\begin{aligned} \nabla H &= \frac{1}{2} \nabla \va{v}^2 + \nabla \Phi + \frac{\nabla p}{\rho} \\ &= \va{v} \cdot (\nabla \va{v}) - \Big( \!-\! \nabla \Phi - \frac{\nabla p}{\rho} \Big) \end{aligned}$Since $-\nabla \Phi = \va{g}$, the rightmost term is the right-hand side of the Euler equation. We substitute the other side of said equation, yielding:

$\begin{aligned} \nabla H &= \va{v} \cdot (\nabla \va{v}) - \frac{\mathrm{D} \va{v}}{\mathrm{D} t} = \va{v} \cdot (\nabla \va{v}) - \pdv{\va{v}}{t} - (\va{v} \cdot \nabla) \va{v} \end{aligned}$We isolate this equation for $\ipdv{\va{v}}{t}$, and apply a vector identity to reduce it to the following:

$\begin{aligned} \pdv{\va{v}}{t} = \va{v} \cdot (\nabla \va{v}) - (\va{v} \cdot \nabla) \va{v} - \nabla H = \va{v} \cross (\nabla \cross \va{v}) - \nabla H \end{aligned}$Here, the definition of the vorticity $\va{\omega}$ is clear to see, leading us to an equation of motion for $\va{v}$:

$\begin{aligned} \boxed{ \pdv{\va{v}}{t} = \va{v} \cross \va{\omega} - \nabla H } \end{aligned}$More about this later. Now, we take the curl of both sides of this equation, giving us:

$\begin{aligned} \nabla \cross \pdv{\va{v}}{t} = \nabla \cross (\va{v} \cross \va{\omega}) - \nabla \cross (\nabla H) \end{aligned}$On the left, we swap $\nabla$ with $\ipdv{}{t}$, and on the right, the curl of a gradient is always zero. We are thus left with the equation of motion of the vorticity $\va{\omega}$:

$\begin{aligned} \boxed{ \pdv{\va{\omega}}{t} = \nabla \cross (\va{v} \cross \va{\omega}) } \end{aligned}$Let us now return to the equation of motion for $\va{v}$.
For *steady* flows where $\ipdv{\va{v}}{t} = 0$, in which case
Bernoulli’s theorem applies,
it reduces to:

If a fluid has $\va{\omega} = 0$ in some regions, it is known as **irrotational**.
From this equation, we see that, in that case, $\nabla H = 0$,
meaning that $H$ is a constant in those regions,
a fact sometimes referred to as **Bernoulli’s stronger theorem**.

Furthermore, irrotationality $\va{\omega} = 0$ implies that $\va{v}$ is the gradient of a potential $\Psi$:

$\begin{aligned} \va{v} = \nabla \Psi \end{aligned}$This fact allows us to rewrite the Euler equations in a particularly simple way. Firstly, the condition of incompressibility becomes the well-known Laplace equation:

$\begin{aligned} 0 = \nabla \cdot \va{v} = \nabla^2 \Psi \end{aligned}$And second, the main equation of motion for $\va{v}$ states that the quantity $H + \ipdv{\Psi}{t}$ is spatially constant in the irrotational region:

$\begin{aligned} \pdv{\va{v}}{t} = \nabla \pdv{\Psi}{t} = - \nabla H \quad \implies \quad \nabla \Big( H + \pdv{\Psi}{t} \Big) = 0 \end{aligned}$## References

- B. Lautrup,
*Physics of continuous matter: exotic and everyday phenomena in the macroscopic world*, 2nd edition, CRC Press.