In Riemannian geometry, the curl or rotation of a vector field over an oriented -dimensional Riemannian manifold is the vector field (or ) defined by
where is the Hodge star operator of ,
Alternatively, the curl/rotation of a vector field in some point is calculated (or alternatively defined) by the integral formula
where runs over the domains with smooth boundary containing point and is the unit vector of outer normal to the surface . The formula does not depend on the shape of boundaries taken in limiting process, so one can typically take a coordinate chart and balls with decreasing radius in this particular coordinate chart.
More generally, if is a Riemannian manifold whose cotangent spaces (equivalently, tangent spaces) are smoothly equipped with a binary cross product , then the curl of any vector field is
However, this is not as general as it may appear:
There are also cross products of other arity? in other dimensions; using essentially the same formula, we can take the curl of a -vector field? if we have a smooth -ary cross product.
If is endowed with the canonical Euclidean metric, then the curl of a vector field is
This is the classical curl from vector analysis?.
In many classical applications of the curl in vector analysis?, the Riemannian structure is actually irrelevant, and the gradient can be replaced with the deRham differential . That is, is treated as the -form , its curl is treated as the -form , and once these identifications are made there is no need to involve at all.