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)LVdr=LVLds=L[Pdu+Qdv]

Then, it can be shown that

CL(V){Q(c)Q(a)}δv{P(d)P(b)}δu(uQvP)δA

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

curl(V)=uQvP

which is the traditional definition.

In the 3D space R3

Mnemonic rule

×F=|ı^ȷ^k^xyzFxFyFz|

which expands as

×F=(FzyFyz)i^+(FxzFzx)j^+(FyxFxy)k^=[FzyFyzFxzFzxFyxFxy]

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

(×F)i=ϵkijjFk,

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=ϵkijj(AmkVm).

Using the product rule:

(×W)i=ϵkijj(Amk)Vm+ϵkijAmkj(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=ϵkijAmkj(Vm),

or simply

×(AV)=A(×V).