Curl of a vector field

In the plane

Following @needham2021visual page 262, we define first the circulation of a vector field V along a closed simple loop L:

CL(V)≡∮LV⋅dr=∮LVLds=∮L[Pdu+Qdv]

Then, it can be shown that

CL(V)≍{Q(c)−Q(a)}δv−{P(d)−P(b)}δu≍≍(∂uQ−∂vP)δA

where ≍ means "ultimately equal".
Now, the curl is defined as the "local circulation per unit area", so

curl(V)=∂uQ−∂vP

which is the traditional definition.

In the 3D space R3

Mnemonic rule

∇×F=|ı^ȷ^k^∂∂x∂∂y∂∂zFxFyFz|

which expands as

∇×F=(∂Fz∂y−∂Fy∂z)i^+(∂Fx∂z−∂Fz∂x)j^+(∂Fy∂x−∂Fx∂y)k^=[∂Fz∂y−∂Fy∂z∂Fx∂z−∂Fz∂x∂Fy∂x−∂Fx∂y]

In R3, for vector fields F=(F1,F2,F3), the curl is alternatively given by:

(∇×F)i=ϵkij∂jFk,

where ϵkij is the Levi-Civita symbol, and the Einstein summation convention is used.

In a coordinate free manner (provided that we have a metric, like the standard one), the curl can be defined as

(∗(dF♭))♯,

where we are using the musical isomorphism ♭,♯ and the Hodge star operator ∗.

Transformation of the curl

Given a vector field V(p) and a linear map A(p) applied in every tangent space TpM, we can find an expression for the curl of the vector field A(p)V(p). Define the vector field W(p)=A(p)V(p).

Given W=AV, we can expand:

Wk=AmkVm.

Let's compute (∇×W)i:

(∇×W)i=ϵkij∂j(AmkVm).

Using the product rule:

(∇×W)i=ϵkij∂j(Amk)Vm+ϵkijAmk∂j(Vm).

Special Case: A is Independent of p
If A does not depend on p (i.e., A(p)=A is a constant linear map across M), then ∂j(Amk)=0, and the expression simplifies to:

(∇×W)i=ϵkijAmk∂j(Vm),

or simply

∇×(AV)=A(∇×V).