On the Dynamical System of Principal Curves in $\mathbb R^d$
Robert Beinert, Arian Bërdëllima, Manuel Gräf, Gabriele Steidl
TL;DR
This work generalizes principal curves from the plane to $\mathbb{R}^d$ with $d\ge3$, formulating a differential-equation description that characterizes self-consistent curves as critical points of the energy $D_{\bm X}^2(\Gamma)$. Building on stochastic and variational viewpoints, it introduces a moving-frame construction and transverse moments to express self-consistency as an explicit ODE system for $\Gamma(s)$ and its tangent directions. The authors then compute principal curves for uniformly distributed data on several 3D domains, showing symmetry-induced planar reductions, and derive concrete examples including rectangular triangles, triangular prisms, and helices on cylinders; these illustrate the method's versatility in higher dimensions. The results open avenues for extending principal-curve computations to other measures and manifolds, with potential applications in nonlinear dimensionality reduction and geometric data analysis, while also suggesting directions for robustness and generalizations.
Abstract
Principal curves are natural generalizations of principal lines arising as first principal components in the Principal Component Analysis. They can be characterized from a stochastic point of view as so-called self-consistent curves based on the conditional expectation and from the variational-calculus point of view as saddle points of the expected difference of a random variable and its projection onto some curve, where the current curve acts as argument of the energy functional. Beyond that, Duchamp and Stützle (1993,1996) showed that planar curves can by computed as solutions of a system of ordinary differential equations. The aim of this paper is to generalize this characterization of principal curves to $\mathbb R^d$ with $d \ge 3$. Having derived such a dynamical system, we provide several examples for principal curves related to uniform distribution on certain domains in $\mathbb R^3$.
