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Torsion of curves |
In the elementary differential geometry of curves in three dimensions, the torsion of a curve measures how sharply it is twisting. Taken together, the curvature and the torsion of a space curve are analogous to the curvature of a plane curve. For example, they are coefficients in the system of differential equations for the Frenet frame given by the Frenet-Serret formulas.
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Let C be a space curve in a unit-length (or natural) parametrization and with the unit tangent vector t. If the curvature κ of C at a certain point is not zero then the principal normal vector and the binormal vector at that point are the unit vectors

The torsion τ measures the speed of rotation of the binormal vector at the given point. It is found from the equation

which means

Remark: The derivative of the binormal vector is perpendicular to both the binormal and the tangent, hence it has to be proportional to the principal normal vector. The negative sign is simply a matter of convention: it is a by-product of the historical development of the subject.
The radius of torsion, often denoted by σ, is defined as

Let r = r(t) be the parametric equation of a space curve. Assume that this is a regular parametrization and that the curvature of the curve does not vanish. Analytically, r(t) is a three times differentiable function of t with values in R3 and the vectors

are linearly independent.
Then the torsion can be computed from the following formula:

Here the primes denote the derivatives with respect to t and the cross denotes the cross product. For r = (x, y, z), the formula in components is

Andrew Pressley, Elementary Differential Geometry, Springer Undergraduate Mathematics Series, Springer-Verlag, 2001 ISBN 1-85233-152-6
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