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 :
C L ( V ) ≡ ∮ L V ⋅ d r = ∮ L V L d s = ∮ L [ P d u + Q d v ] Then, it can be shown that
C L ( V ) ≍ { Q ( c ) − Q ( a ) } δ v − { P ( d ) − P ( b ) } δ u ≍ ≍ ( ∂ u Q − ∂ v P ) δ A where ≍ means "ultimately equal".
Now, the curl is defined as the "local circulation per unit area", so
c u r l ( V ) = ∂ u Q − ∂ v P which is the traditional definition.
Mnemonic rule
∇ × F = | ı ^ ȷ ^ k ^ ∂ ∂ x ∂ ∂ y ∂ ∂ z F x F y F z | which expands as
∇ × F = ( ∂ F z ∂ y − ∂ F y ∂ z ) i ^ + ( ∂ F x ∂ z − ∂ F z ∂ x ) j ^ + ( ∂ F y ∂ x − ∂ F x ∂ y ) k ^ = [ ∂ F z ∂ y − ∂ F y ∂ z ∂ F x ∂ z − ∂ F z ∂ x ∂ F y ∂ x − ∂ F x ∂ y ] In R 3 , for vector fields F = ( F 1 , F 2 , F 3 ) , the curl is alternatively given by:
( ∇ × F ) i = ϵ k i j ∂ j F k , where ϵ k i j 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
( ∗ ( d F ♭ ) ) ♯ , where we are using the musical isomorphism ♭ , ♯ and the Hodge star operator ∗ .
Given a vector field V ( p ) and a linear map A ( p ) applied in every tangent space T p M , 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 = A V , we can expand:
W k = A m k V m . Let's compute ( ∇ × W ) i :
( ∇ × W ) i = ϵ k i j ∂ j ( A m k V m ) . Using the product rule:
( ∇ × W ) i = ϵ k i j ∂ j ( A m k ) V m + ϵ k i j A m k ∂ j ( V m ) . 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 ( A m k ) = 0 , and the expression simplifies to:
( ∇ × W ) i = ϵ k i j A m k ∂ j ( V m ) , or simply
∇ × ( A V ) = A ( ∇ × V ) .