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Reparameterization 📂Geometry

Reparameterization

Definition 1

Reparameterization

Let kNk \in \mathbb{N} and a curve α:(a,b)R3\alpha : (a,b) \to \mathbb{R}^{3} be given. If a bijection g:(c,d)(a,b)g: (c,d) \to (a,b) satisfies g,g1Ckg , g^{-1} \in C^{k}, then gg is referred to as the Reparameterization of α\alpha.


Explanation

Pronouncing it is hard, so even in English, it’s read as [Reparameterization]; it’s just that the word itself is long.

In fact, the concept may sound grandiose, but thinking of curve α\alpha represented by parameters like α(t)\alpha (t) as if β(t)=α(g(t))\beta (t) = \alpha \left( g (t) \right) is essentially reparameterization. The clear part mathematically is not just leaving it as a thought or concept but defining it as a function and objectifying it.

Conservation of Regularity

The purpose of reparameterization can be easily imagined from the fact that gg is a bijection. It’s about changing a curve that is hard to handle into one that is easy to write and manage, using various tricks, and g1g^{-1} to revert it back. In other words, it’s a variable substitution.

According to the chain rule of differentiation, one obtains the following for parameters g(r)=t(a,b)g(r) = t \in (a,b), r(c,d)r \in (c,d). dβdr=(dαdt)(dgdr) {{ d \beta } \over { d r }} = \left( {{ d \alpha } \over { d t }} \right) \left( {{ d g } \over { d r }} \right) Similarly, by applying the chain rule and differentiating both sides of g(g1(t))=tg \left( g^{-1} (t) \right) = t by tt, (dgdr)(dg1dt)=1 \left( {{ d g } \over { d r }} \right) \left( {{ d g^{-1} } \over { d t }} \right) = 1 it is understood that dgdr0\dfrac{dg}{dr} \ne 0. Here, if α\alpha is a regular curve, then since dαdt0\dfrac{d\alpha}{dt} \ne \mathbf{0}, it is guaranteed that dβdr0\dfrac{d\beta}{dr} \ne \mathbf{0} and thus, reparameterization conserves the curve’s Regularity.

Lemma

Let’s say for reparameterization g:(c,d)(a,b)g: (c,d) \to (a,b) that β=αg\beta = \alpha \circ g. If t0=g(r0)t_{0} = g \left( r_{0} \right), in t0t_{0}, the tangent vector field TT of α\alpha and in r0r_{0}, the tangent vector field SS of β\beta satisfy the following. S=±T S = \pm T Especially if gg is an increasing function, then S=TS=T; if it’s a decreasing function, then S=TS = -T.


Proof

S=dβdrdβdr=dαdtdαdtdgdrdgdr=T(±1)=±T \begin{align*} S =& {{ {{ d \beta } \over { dr }} } \over { \left| {{ d \beta } \over { dr }} \right| }} \\ =& {{ {{ d \alpha } \over { dt }} } \over { \left| {{ d \alpha } \over { dt }} \right| }} {{ {{ d g } \over { dr }} } \over { \left| {{ d g } \over { dr }} \right| }} \\ =& T \cdot ( \pm 1) \\ =& \pm T \end{align*}


  1. Millman. (1977). Elements of Differential Geometry: p17~18. ↩︎