PlanetPhysics/Curl

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To the [[../VectorProduct/|cross product]] of the [[../Gradient/|gradient operator]] × Maxwell gave the name 𝐜url.

×𝐕=curl𝐕

The curl of a [[../VectorFunctions/|vector function]] 𝐕 is itself a vector function of [[../Position/|position]] in space. As the name indicates, it is closely connected with the angular [[../Velocity/|velocity]] or [[../QuarkAntiquarkPair/|spin]] of the [[../AbsoluteMagnitude/|flux]] at each point. But the interpretation of the curl is neither so easily obtained nor so simple as that of the [[../DivergenceOfAVectorField/|divergence]].

Consider as before that 𝐕 represents the flux of a fluid. Take at a definite instant an infinitesimal sphere about any point (x,y,z). At the next instant what has become of the sphere? In the first place it may have moved off as a whole in a certain direction by an amount d𝐫. In other words it may have a translational velocity of d𝐫/dt. In other words it may have undergone such a [[../CohomologicalProperties/|deformation]] that it is no longer a sphere. It may have been subjected to a strain by virtue of which it becomes slightly ellipsoidal in shape. Finally it may have been rotated as a whole about some axis through an angle dw. That is to say, it may have an angular velocity the [[../AbsoluteMagnitude/|magnitude]] of which is dw/dt. An infinitesimal sphere therefore may have any one of these distinct [[../Bijective/|types]] of [[../CosmologicalConstant/|motion]] or all of them combined. First, a translation with definite velocity. Second, a strain with three definite rates of elongation along the axes of an ellipsoid. Third, an angular velocity about a difinite axis. It is this third type of motion which is given by the curl. In fact, the curl of the flux V is a [[../Vectors/|vector]] which has at each point of space the direction of the instantaneous axis of rotation at that point and a magnitude equal to twice the instantaneous angular velocity about that axis.

The analytic discussion of the motion of a fluid presents more difficulties than it is necessary to introduce in treating the curl. The motion of a [[../CenterOfGravity/|rigid body]] is sufficiently complex to give an adequate idea of the [[../Cod/|operation]]. It was seen that the velocity of the [[../Particle/|particles]] of a rigid body at any instant is given by the [[../Formula/|formula]] 𝐯=𝐯0+𝐚×𝐫

curl𝐯=×𝐯=×𝐯0+×(𝐚×𝐫)

Let

𝐚=a1𝐒^+a2𝐣^+a3𝐀^

𝐫=r1𝐒^+r2𝐣^+r3𝐀^=x𝐒^+y𝐣^+z𝐀^

expand ×(𝐚×𝐫) formally as if it were the [[../BACKCAB/|Vector Triple Product]] of , 𝐚, and 𝐫. Then

×𝐯=×𝐯0+(𝐫)𝐚(𝐚)𝐫

𝐯0 is a constant vector. Hence the term ×𝐯0 vanishes.

𝐫=xx+yy+zz=3

Since 𝐚 is a constant vector, it may be placed upon the other side of the differential [[../QuantumSpinNetworkFunctor2/|operator]], 𝐚=𝐚

𝐚𝐫=(a1x+a2y+a3z)𝐫=a1𝐒^+a2𝐣^+a3𝐀^=𝐚

Hence

×𝐯=3𝐚𝐚=2𝐚

Therefore in the case of the motion of a rigid body the curl of the linear velocity at any point is equal to twice the angular velocity in magnitude and in direction.

×𝐯=curl𝐯=2𝐚 𝐚=12×𝐯=12curl𝐯 𝐯=𝐯0+12(×𝐯)×𝐫=𝐯0+12(curl𝐯)×𝐫

The expansion of ×(𝐚×𝐫) formally may be avoided by multiplying 𝐚×𝐫 out and then applying the operator × to the result.

References

[1] Wilson, E. "Vector Analysis." Yale University Press, New Haven, 1913.

This entry is a derivative of the Public [[../Bijective/|domain]] [[../Work/|work]] [1].

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