Suitable curvature functions determine a regular Frenet curve up to a Euclidean rigid motion. In the plane one signed curvature suffices; in three dimensions positive curvature and torsion determine a unit-speed curve, as in the fundamental theorem of regular space curves. The result is local on the parameter interval and assumes the regularity needed by the frame equations.
For a regular parameter , the curvature and torsion of a space curve are
The torsion of a space curve requires . Reparameterize by arc length and set , , . Differentiating the pairwise inner products of this orthonormal Frenet frame shows that its derivative matrix is skew symmetric. Since , defining gives the Frenet-Serret formulas
The fundamental theorem of regular space curves says that prescribed smooth and smooth on an interval determine a unit-speed curve uniquely up to an orientation-preserving Euclidean rigid motion. Solve this frame's linear differential equation with an initial oriented orthonormal frame, then integrate ; uniqueness proves the assertion.
Under the intended convention that the shared parameter is arc length, equality on an open interval gives equal position and equal Frenet frames at one point. Equal give identical differential equations, so uniqueness gives . The printed “regular smooth” hypothesis alone does not establish this convention. Without common arc length, an orientation-preserving smooth change of speed that is the identity on but not elsewhere reparameterizes a circle into a counterexample: both curves have , and agree on , but differ elsewhere as parameterized curves.
For an oriented surface with unit normal , define normal curvature and geodesic curvature . Thus
A unit-speed curve is a geodesic exactly when . If also , then , so it is a straight line. A vertical ruling of a circular cylinder is such a geodesic, although the cylinder contains no open piece of a plane. A nonconstant regular straight line cannot be a simple closed curve. Hence no planar patch is required, and such a geodesic cannot be simple and closed.
Finally let the principal curvatures be . If the Gaussian curvature , they have the same sign or one vanishes. Euler formula for normal curvature makes a weighted average of them. For a geodesic, , so
A horizontal circle on a cylinder of radius is a geodesic with , , , attaining equality.
The fundamental theorem of regular space curves states that smooth functions and on an interval determine a smooth arc-length-parametrized curve in , unique up to a proper Euclidean motion. Consequently two such curves and are related parameterwise by a proper Euclidean motion if and only if
for every .
Let
This is another unit-speed embedded curve. The assumed identities say that and have the same positive curvature and the same torsion. By the uniqueness part of the fundamental theorem of regular space curves, there is a proper Euclidean motion such that
Since is a bijection of , this motion preserves .
It is nontrivial. For the plus sign, and would imply , contradicting embeddedness. For the minus sign, the identity would imply for every , and injectivity would force for every , which is impossible. Thus the required nontrivial proper Euclidean motion exists.