Definitions

# Differential geometry of curves

This article only considers curves in Euclidean space. Most of the notions presented here have analogues for curves in Riemannian and pseudo-Riemannian manifolds. For a discussion of curves in an arbitrary topological space, see the main article on curves.

Differential geometry of curves is the branch of geometry that deals with smooth curves in the plane and in the Euclidean space by methods of differential and integral calculus.

Starting in antiquity, many concrete curves have been thoroughly investigated using synthetic approach. Differential geometry takes another path: curves are represented in a parametrized form, and their geometric properties and various quantities associated with them, such as the curvature and the arc length, are expressed via derivatives and integrals using vector calculus. One of the most important tools used to analyze a curve is the Frenet frame, a moving frame that provides a coordinate system at each point of the curve that is "best adapted" to the curve near that point.

The theory of curves is much simpler and narrower in scope than the theory of surfaces and its higher-dimensional generalizations, because a regular curve in an Euclidean space has no intrinsic geometry. Any regular curve may be parametrized by the arc length (the natural parametrization) and from the point of view of a bug on the curve that does not know anything about the ambient space, all curves would appear the same. Different space curves are only distinguished by the way in which they bend and twist. Quantitatively, this is measured by the differential-geometric invariants called the curvature and the torsion of a curve. The fundamental theorem of curves asserts that the knowledge of these invariants completely determines the curve.

## Definitions

Let n be a natural number, r a natural number or ∞, I be a non-empty interval of real numbers and t in I. A vector-valued function

$mathbf\left\{gamma\right\}:I to \left\{mathbb R\right\}^n$

of class Cr (i.e. γ is r times continuously differentiable) is called a parametric curve of class Cr or a Cr parametrization of the curve γ. t is called the parameter of the curve γ. γ(I) is called the image of the curve. It is important to distinguish between a curve γ and the image of a curve γ(I) because a given image can be described by several different Cr curves.

One may think of the parameter t as representing time and the curve γ(t) as the trajectory of a moving particle in space.

If I is a closed interval [a, b], we call γ(a) the starting point and γ(b) the endpoint of the curve γ.

If γ(a) = γ(b), we say γ is closed or a loop. Furthermore, we call γ a closed Cr-curve if γ(k)(a) = γ(k)(b) for all kr.

If γ:(a,b) → Rn is injective, we call the curve simple.

If γ is a parametric curve which can be locally described as a power series, we call the curve analytic or of class $C^omega$.

We write -γ to say the curve is traversed in opposite direction.

A Ck-curve

$gamma:\left[a,b\right] rightarrow mathbb\left\{R\right\}^n$

is called regular of order m if for any t in interval I

$lbrace gamma\text{'}\left(t\right), gamma\left(t\right), ...,gamma^\left\{\left(m\right)\right\}\left(t\right) rbrace mbox \left\{, \right\} m leq k$

are linearly independent in Rn.

In particular, a C1-curve γ is regular if

$gamma\text{'}\left(t\right) neq 0$ for any $t in I$.

## Reparametrization and equivalence relation

Given the image of a curve one can define several different parameterizations of the curve. Differential geometry aims to describe properties of curves invariant under certain reparametrizations. So we have to define a suitable equivalence relation on the set of all parametric curves. The differential geometric properties of a curve (length, frenet frame and generalized curvature) are invariant under reparametrization and therefore properties of the equivalence class.The equivalence classes are called Cr curves and are central objects studied in the differential geometry of curves.

Two parametric curves of class Cr

$mathbf\left\{gamma_1\right\}:I_1 to R^n$

and

$mathbf\left\{gamma_2\right\}:I_2 to R^n$

are said to be equivalent if there exists a bijective Cr map

$phi :I_1 to I_2$

such that

$phi\text{'}\left(t\right) neq 0 qquad \left(t in I_1\right)$

and

$mathbf\left\{gamma_2\right\}\left(phi\left(t\right)\right) = mathbf\left\{gamma_1\right\}\left(t\right) qquad \left(t in I_1\right)$

γ2 is said to be a reparametrisation of γ1. This reparametrisation of γ1 defines the equivalence relation on the set of all parametric Cr curves. The equivalence class is called a Cr curve.

We can define an even finer equivalence relation of oriented Cr curves by requiring φ to be φ‘(t) > 0.

Equivalent Cr curves have the same image. And equivalent oriented Cr curves even traverse the image in the same direction.

## Length and natural parametrization

The length l of a curve γ : [a, b] → Rn of class C1 can be defined as

$l = int_a^b vert mathbf\left\{gamma\right\}\text{'}\left(t\right) vert dt.$

The length of a curve is invariant under reparametrization and therefore a differential geometric property of the curve.

For each regular Cr-curve (r at least 1) γ: [a, b] → Rn we can define a function

$s\left(t\right) = int_\left\{t_0\right\}^t vert mathbf\left\{gamma\right\}\text{'}\left(x\right) vert dx.$

Writing

$barmathbf\left\{gamma\right\}\left(s\right) = gamma\left(t\left(s\right)\right)$

where t(s) is the inverse of s(t), we get a reparametrization $bar gamma$of γ which is called natural, arc-length or unit speed parametrization. The parameter s(t) is called the natural parameter of γ.

We prefer this parametrization because the natural parameter s(t) traverses the image of γ at unit speed so that

$vert barmathbf\left\{gamma\right\}\text{'}\left(s\left(t\right)\right) vert = 1 qquad \left(t in I\right).$

In practice it is often very difficult to calculate the natural parametrization of a curve, but it is useful for theoretical arguments.

For a given parametrized curve γ(t) the natural parametrization is unique up to shift of parameter.

The quantity

$E\left(gamma\right) = frac\left\{1\right\}\left\{2\right\}int_a^b vert mathbf\left\{gamma\right\}\text{'}\left(t\right) vert^2 dt$

is sometimes called the energy or action of the curve; this name is justified because the geodesic equations are the Euler–Lagrange equations of motion for this action.

## Frenet frame

A Frenet frame is a moving reference frame of n orthonormal vectors ei(t) which are used to describe a curve locally at each point γ(t). It is the main tool in the differential geometric treatment of curves as it is far easier and more natural to describe local properties (e.g. curvature, torsion) in terms of a local reference system than using a global one like the Euclidean coordinates.

Given a Cn+1-curve γ in Rn which is regular of order n the Frenet Frame for the curve is the set of orthonormal vectors

$mathbf\left\{e\right\}_1\left(t\right), ldots, mathbf\left\{e\right\}_n\left(t\right)$

called Frenet vectors. They are constructed from the derivatives of γ(t) using the Gram-Schmidt orthogonalization algorithm with

$mathbf\left\{e\right\}_1\left(t\right) = frac\left\{mathbf\left\{gamma\right\}\text{'}\left(t\right)\right\}\left\{| mathbf\left\{gamma\right\}\text{'}\left(t\right) |\right\}$


mathbf{e}_{j}(t) = frac{overline{mathbf{e}_{j}}(t)}{|overline{mathbf{e}_{j}}(t) |} mbox{, } overline{mathbf{e}_{j}}(t) = mathbf{gamma}^{(j)}(t) - sum _{i=1}^{j-1} langle mathbf{gamma}^{(j)}(t), mathbf{e}_i(t) rangle , mathbf{e}_i(t)

The real valued functions χi(t) are called generalized curvatures and are defined as

$chi_i\left(t\right) = frac\left\{langle mathbf\left\{e\right\}_i\text{'}\left(t\right), mathbf\left\{e\right\}_\left\{i+1\right\}\left(t\right) rangle\right\}\left\{| mathbf\left\{gamma\right\}^\text{'}\left(t\right) |\right\}$

The Frenet frame and the generalized curvatures are invariant under reparametrization and therefore differential geometric properties of the curve.

## Special Frenet vectors and generalized curvatures

The first three Frenet vectors and generalized curvatures can be visualized in three-dimensional space. They have additional names and more semantic information attached to them.

### Tangent vector

If a curve γ represents the path of a particle then the instanteneous velocity of the particle at a given point P is expressed by a vector, called the tangent vector to the curve at P. Mathematically, given a parametrized C1 curve γ = γ(t), for every value t = t0 of the parameter, the vector

$gamma\text{'}\left(t_0\right) = frac\left\{d\right\}\left\{d,t\right\}mathbf\left\{gamma\right\}\left(t\right)$ at $\left\{t=t_0\right\}$

is the tangent vector at the point P = γ(t0). Generally speaking, the tangent vector may be zero. The magnitude of the tangent vector,

$|mathbf\left\{gamma\right\}\text{'}\left(t_0\right)|,$

is the speed at the time t0.

The first Frenet vector e1(t) is the unit tangent vector in the same direction, defined at each regular point of γ:

$mathbf\left\{e\right\}_\left\{1\right\}\left(t\right) = frac\left\{ mathbf\left\{gamma\right\}\text{'}\left(t\right) \right\}\left\{ | mathbf\left\{gamma\right\}\text{'}\left(t\right) |\right\}.$

If t = s is the natural parameter then the tangent vector has unit length, so that the formula simplifies:

$mathbf\left\{e\right\}_\left\{1\right\}\left(s\right) = mathbf\left\{gamma\right\}\text{'}\left(s\right).$

The unit tangent vector determines the orientation of the curve, or the forward direction, corresponding to the increasing values of the parameter.

### Normal or curvature vector

The normal vector, sometimes called the curvature vector, indicates the deviance of the curve from being a straight line.

It is defined as

$overline\left\{mathbf\left\{e\right\}_2\right\}\left(t\right) = mathbf\left\{gamma\right\}$(t) - langle mathbf{gamma}(t), mathbf{e}_1(t) rangle , mathbf{e}_1(t).

Its normalized form, the unit normal vector, is the second Frenet vector e2(t) and defined as

$mathbf\left\{e\right\}_2\left(t\right) = frac\left\{overline\left\{mathbf\left\{e\right\}_2\right\}\left(t\right)\right\} \left\{| overline\left\{mathbf\left\{e\right\}_2\right\}\left(t\right) |\right\}.$

The tangent and the normal vector at point t define the osculating plane at point t.

### Curvature

The first generalized curvature χ1(t) is called curvature and measures the deviance of γ from being a straight line relative to the osculating plane. It is defined as

$kappa\left(t\right) = chi_1\left(t\right) = frac\left\{langle mathbf\left\{e\right\}_1\text{'}\left(t\right), mathbf\left\{e\right\}_2\left(t\right) rangle\right\}\left\{| mathbf\left\{gamma\right\}^\text{'}\left(t\right) |\right\}$

and is called the curvature of γ at point t.

The reciprocal of the curvature

$frac\left\{1\right\}\left\{kappa\left(t\right)\right\}$

is called the radius of curvature.

A circle with radius r has a constant curvature of

$kappa\left(t\right) = frac\left\{1\right\}\left\{r\right\}$

whereas a line has a curvature of 0.

### Binormal vector

The binormal vector is the third Frenet vector e3(t) It is always orthogonal to the unit tangent and normal vectors at t, and is defined as

$mathbf\left\{e\right\}_3\left(t\right) = frac\left\{overline\left\{mathbf\left\{e\right\}_3\right\}\left(t\right)\right\} \left\{| overline\left\{mathbf\left\{e\right\}_3\right\}\left(t\right) |\right\}$
mbox{, } overline{mathbf{e}_3}(t) = mathbf{gamma}(t) - langle mathbf{gamma}(t), mathbf{e}_1(t) rangle , mathbf{e}_1(t) - langle mathbf{gamma}'(t), mathbf{e}_2(t) rangle ,mathbf{e}_2(t)

In 3-dimensional space the equation simplifies to

$mathbf\left\{e\right\}_3\left(t\right) = mathbf\left\{e\right\}_2\left(t\right) times mathbf\left\{e\right\}_1\left(t\right)$

### Torsion

The second generalized curvature χ2(t) is called torsion and measures the deviance of γ from being a plane curve. Or, in other words, if the torsion is zero the curve lies completely in a same osculating plane (there is an only osculating plane for every point t).

$tau\left(t\right) = chi_2\left(t\right) = frac\left\{langle mathbf\left\{e\right\}_2\text{'}\left(t\right), mathbf\left\{e\right\}_3\left(t\right) rangle\right\}\left\{| mathbf\left\{gamma\right\}\text{'}\left(t\right) |\right\}$

and is called the torsion of γ at point t.

## Main theorem of curve theory

Given n functions

$chi_i in C^\left\{n-i\right\}\left(\left[a,b\right]\right) mbox\left\{, \right\} 1 leq i leq n$

with

$chi_i\left(t\right) > 0 mbox\left\{, \right\} 1 leq i leq n-1$

then there exists a unique (up to transformations using the Euclidean group) Cn+1-curve γ which is regular of order n and has the following properties

$|gamma\text{'}\left(t\right)| = 1 mbox\left\{ \right\} \left(t in \left[a,b\right]\right)$
$chi_i\left(t\right) = frac\left\{ langle mathbf\left\{e\right\}_i\text{'}\left(t\right), mathbf\left\{e\right\}_\left\{i+1\right\}\left(t\right) rangle\right\}\left\{| mathbf\left\{gamma\right\}\text{'}\left(t\right) |\right\}$

where the set

$mathbf\left\{e\right\}_1\left(t\right), ldots, mathbf\left\{e\right\}_n\left(t\right)$

is the Frenet frame for the curve.

By additionally providing a start t0 in I, a starting point p0 in Rn and an initial positive orthonormal Frenet frame {e1, ..., en-1} with

$mathbf\left\{gamma\right\}\left(t_0\right) = mathbf\left\{p\right\}_0$
$mathbf\left\{e\right\}_i\left(t_0\right) = mathbf\left\{e\right\}_i mbox\left\{, \right\} 1 leq i leq n-1$

we can eliminate the Euclidean transformations and get unique curve γ.

## Frenet-Serret formulas

The Frenet-Serret formulas are a set of ordinary differential equations of first order. The solution is the set of Frenet vectors describing the curve specified by the generalized curvature functions χi

### 2-dimensions


begin{bmatrix} mathbf{e}_1'(t) mathbf{e}_2'(t) end{bmatrix}

=

begin{bmatrix}

`         0 & kappa(t) `
`-kappa(t) &        0  `
end{bmatrix}

begin{bmatrix} mathbf{e}_1(t) mathbf{e}_2(t) end{bmatrix}

### 3-dimensions


begin{bmatrix} mathbf{e}_1'(t) mathbf{e}_2'(t) mathbf{e}_3'(t) end{bmatrix}

=

begin{bmatrix}

`         0 &  kappa(t) &       0 `
`-kappa(t) &          0 & tau(t) `
`         0 &   -tau(t) &       0 `
end{bmatrix}

begin{bmatrix} mathbf{e}_1(t) mathbf{e}_2(t) mathbf{e}_3(t) end{bmatrix}

### n dimensions (general formula)


begin{bmatrix} mathbf{e}_1'(t)
`          vdots `
mathbf{e}_n'(t) end{bmatrix}

=

begin{bmatrix}

`         0 & chi_1(t) &                &             0 `
`-chi_1(t) &    ddots &         ddots &               `
& ddots & 0 & chi_{n-1}(t) 0 & & -chi_{n-1}(t) & 0 end{bmatrix}

begin{bmatrix} mathbf{e}_1(t)

`         vdots `
mathbf{e}_n(t) end{bmatrix}