Calculus/Vectors

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Vectors

Two-Dimensional VectorsEdit

IntroductionEdit

In most mathematics courses up until this point, we deal with scalars. These are quantities which only need one number to express. For instance, the amount of gasoline used to drive to the grocery store is a scalar quantity because it only needs one number: 2 gallons.

In this unit, we deal with vectors. A vector is a directed line segment -- that is, a line segment that points one direction or the other. As such, it has an initial point and a terminal point. The vector starts at the initial point and ends at the terminal point, and the vector points towards the terminal point. A vector is drawn as a line segment with an arrow at the terminal point:

A single vector without coordinate axes.


The same vector can be placed anywhere on the coordinate plane and still be the same vector -- the only two bits of information a vector represents are the magnitude and the direction. The magnitude is simply the length of the vector, and the direction is the angle at which it points. Since neither of these specify a starting or ending location, the same vector can be placed anywhere. To illustrate, all of the line segments below can be defined as the vector with magnitude 4\sqrt{2} and angle 45 degrees:

Multiple locations for the same vector.

It is customary, however, to place the vector with the initial point at the origin as indicated by the black vector. This is called the standard position.

Component FormEdit

In standard practice, we don't express vectors by listing the length and the direction. We instead use component form, which lists the height (rise) and width (run) of the vectors. It is written as follows:

\begin{pmatrix} \mathrm{run} \\ \mathrm{rise}\end{pmatrix}

Vector with rise and run measurements.

Other ways of denoting a vector in component form include:

\mathbf{(u_x,u_y)} and \mathbf{\left\langle u_x,u_y\right\rangle}

From the diagram we can now see the benefits of the standard position: the two numbers for the terminal point's coordinates are the same numbers for the vector's rise and run. Note that we named this vector u. Just as you can assign numbers to variables in algebra (usually x, y, and z), you can assign vectors to variables in calculus. The letters u, v, and w are usually used, and either boldface or an arrow over the letter is used to identify it as a vector.

When expressing a vector in component form, it is no longer obvious what the magnitude and direction are. Therefore, we have to perform some calculations to find the magnitude and direction.

MagnitudeEdit

|\mathbf{u}| = \sqrt{u_x^2+u_y^2}

where u_x is the width, or run, of the vector; u_y is the height, or rise, of the vector. You should recognize this formula as the Pythagorean theorem. It is -- the magnitude is the distance between the initial point and the terminal point.

The magnitude of a vector can also be called the norm.

DirectionEdit

\tan \theta = \frac{u_y}{u_x}

Vector triangle with ux and uy labeled.


where \theta is the direction of the vector. This formula is simply the tangent formula for right triangles.

Vector OperationsEdit

For these definitions, assume:


\mathbf{u} = \begin{pmatrix} u_x \\ u_y \end{pmatrix}

\mathbf{v} = \begin{pmatrix} v_x \\ v_y \end{pmatrix}


Vector AdditionEdit

Vector Addition is often called tip-to-tail addition, because this makes it easier to remember.

The sum of the vectors you are adding is called the resultant vector, and is the vector drawn from the initial point (tip) of the first vector to the terminal point (tail) of the second vector. Although they look like the arrows, the pointy bit is the tail, not the tip. (Imagine you were walking the direction the vector was pointing... you would start at the flat end (tip) and walk toward the pointy end.)

It looks like this:

Tip-to-tail addition

(Notice, the black lined vector is the sum of the two dotted line vectors!)


Numerically:


\begin{pmatrix} 4 \\ 6 \end{pmatrix} + \begin{pmatrix} 1 \\ -3 \end{pmatrix} = \begin{pmatrix} 5 \\ 3 \end{pmatrix}

Or more generally:


\mathbf{u} + \mathbf{v} = \begin{pmatrix} u_x + v_x \\ u_y + v_y \end{pmatrix}

Scalar MultiplicationEdit

Graphically, multiplying a vector by a scalar changes only the magnitude of the vector by that same scalar. That is, multiplying a vector by 2 will "stretch" the vector to twice its original magnitude, keeping the direction the same.

Multiplication of a vector with a scalar 2 \cdot \begin{pmatrix} 3 \\ 3 \end{pmatrix} = \begin{pmatrix} 6 \\ 6 \end{pmatrix}

Numerically, you calculate the resultant vector with this formula:

c \mathbf{u} = \begin{pmatrix} c u_x \\ c u_y \end{pmatrix}, where c is a constant scalar.

As previously stated, the magnitude is changed by the same constant:

|c \mathbf{u}| = c |\mathbf{u}|

Since multiplying a vector by a constant results in a vector in the same direction, we can reason that two vectors are parallel if one is a constant multiple of the other -- that is, that \mathbf{u} || \mathbf{v} if \mathbf{u} = c \mathbf{v} for some constant c.

We can also divide by a non-zero scalar by instead multiplying by the reciprocal, as with dividing regular numbers:

\frac{\mathbf{u}}{c} = \frac{1}{c} \mathbf{u}, {c}\ne 0


Dot ProductEdit

The dot product is a way of multiplying two vectors to produce a scalar value. Because it combines the components of two vectors to form a /scalar/, it is sometimes called a scalar product. If you were asked to take the 'dot product of two rectangular vectors' you would do the following:

\mathbf{u} \cdot \mathbf{v} = u_x v_x + u_y v_y

http://en.wikibooks.org/w/index.php?title=Calculus/Vectors&action=edit&section=9

It is very important to note that the dot product of two vectors does not result in another vector, it gives you a scalar, just a numerical value.

Another common pitfall may arise if your vectors are not in rectangular ('cartesian') format. Sometimes, vectors are instead expressed in polar coordinates, where the first component is the vector's magnitude (length) and the second is the angle from the x-axis at which the vector should be oriented. Dot products cannot be performed using the conventional method on these sorts of vectors; vectors in polar format must be converted to their equivalent rectangular form before you can work with them using the formula given above. A common way to convert to rectangular coordinates is to imagine that the vector was projected horizontally and vertically to form a right triangle. You could then use properties of sin and cos to find the length of the two legs the right triangle. The horizontal length would then be the x-component of the rectangular expression of the vector and the vertical length would be the y-component. Remember that if the vector is pointing down or to the left, the corresponding components would have to be negative to indicate that.

With some rearrangement and trigonometric manipulation, we can see that the number that results from the dot product of two vectors is a surprising and useful identity:

\mathbf{u} \cdot \mathbf{v} = |\mathbf{u}| |\mathbf{v}| \cos \theta

where \theta is the angle between the two vectors. This provides a convenient way of finding the angle between two vectors:

 \cos \theta = \frac{\mathbf{u} \cdot \mathbf{v}}{
|\mathbf{u}| |\mathbf{v}|}

Notice that the dot product is 'commutative', that is:

\mathbf{u} \cdot \mathbf{v} = \mathbf{v} \cdot \mathbf{u}

Also, the dot product of two vectors will be the length of the vector squared:

\mathbf{u} \cdot \mathbf{u} = u_x u_x + u_y u_y = (u_x)^2+(u_y)^2

and by the Pythagorean theorem,

(u_x)^2+(u_y)^2=||u||^2

The dot product can be visualized as the length of a projection of one vector on to the other. In other words, the dot product asks 'how much magnitude of this vector is going in the direction of that vector?'

Applications of Scalar Multiplication and Dot ProductEdit

Unit VectorsEdit

A unit vector is a vector with a magnitude of 1. The unit vector of u is a vector in the same direction as \mathbf{u}, but with a magnitude of 1:

Unit vector


The process of finding the unit vector of u is called normalization. As mentioned in scalar multiplication, multiplying a vector by constant C will result in the magnitude being multiplied by C. We know how to calculate the magnitude of \mathbf{u}. We know that dividing a vector by a constant will divide the magnitude by that constant. Therefore, if that constant is the magnitude, dividing the vector by the magnitude will result in a unit vector in the same direction as \mathbf{u}:

\mathbf{w}=\frac{\mathbf{u}}{|\mathbf{u}|}, where \mathbf{w} is the unit vector of \mathbf{u}

Standard Unit VectorsEdit

A special case of Unit Vectors are the Standard Unit Vectors i and j: i points one unit directly right in the x direction, and j points one unit directly up in the y direction:

\mathbf{i} = \begin{pmatrix} 1 \\ 0 \end{pmatrix}

\mathbf{j} = \begin{pmatrix} 0 \\ 1 \end{pmatrix}

Using the scalar multiplication and vector addition rules, we can then express vectors in a different way:

\begin{pmatrix} x \\ y \end{pmatrix} = x \mathbf{i} + y \mathbf{j}

If we work that equation out, it makes sense. Multiplying x by i will result in the vector \begin{pmatrix} x \\ 0 \end{pmatrix}. Multiplying y by j will result in the vector \begin{pmatrix} 0 \\ y \end{pmatrix}. Adding these two together will give us our original vector, \begin{pmatrix} x \\ y \end{pmatrix}. Expressing vectors using i and j is called standard form.

Projection and Decomposition of VectorsEdit

Sometimes it is necessary to decompose a vector  \mathbf{u} into two components: one component parallel to a vector  \mathbf{v}
, which we will call  \mathbf{u}_ \parallel ; and one component perpendicular to it,  \mathbf{u}_ \bot .

Projection of a vector

Since the length of  \mathbf{u}_ \parallel is (|\mathbf{u}| \cdot \cos \theta ), it is straightforward to write down the formulas for  \mathbf{u}_ \bot and 
\mathbf{u}_ \parallel  :

\mathbf{u_ \parallel} = |\mathbf{u}| * \frac{(\mathbf{u} \cdot
\mathbf{v})}{(|\mathbf{u}| |\mathbf{v}|)} * \frac{\mathbf{v}}{|\mathbf{v}|}= 
(\mathbf{u} \cdot \mathbf{v})/(|\mathbf{v}|^2)  \mathbf{v}

and

 \mathbf{u}_ \bot = \mathbf{u} - \mathbf{u}_ \parallel

Length of a vectorEdit

The length of a vector is given by the dot product of a vector with itself, and  \theta = 0 deg :

\mathbf{u} \cdot \mathbf{u} = |\mathbf{u}||\mathbf{u}| \cos \theta = |\mathbf{u}|^2

Perpendicular vectorsEdit

If the angle  \theta between two vectors is 90 degrees or  {\pi \over 2} (if the two vectors are orthogonal to each other), that is the vectors are perpendicular, then the dot product is 0. This provides us with an easy way to find a perpendicular vector: if you have a vector  \mathbf{u} = \begin{pmatrix} u_x \\ u_y \end{pmatrix}, a perpendicular vector can easily be found by either

 \mathbf{v} = \begin{pmatrix} -u_y \\ u_x \end{pmatrix} = - \begin{pmatrix} u_y \\ -u_x \end{pmatrix}


Polar coordinatesEdit

Polar coordinates are an alternative two-dimensional coordinate system, which is often useful when rotations are important. Instead of specifying the position along the x and y axes, we specify the distance from the origin, r, and the direction, an angle θ.

Polar coordinates

Looking at this diagram, we can see that the values of x and y are related to those of r and θ by the equations

\begin{matrix} 
x=r \cos \theta & r = \sqrt{x^2+y^2} \\
y=r \sin \theta & \tan \theta = \frac{y}{x} \end{matrix}

Because tan-1 is multivalued, care must be taken to select the right value.

Just as for Cartesian coordinates the unit vectors that point in the x and y directions are special, so in polar coordinates the unit vectors that point in the r and θ directions are also special.

We will call these vectors \hat{\mathbf{r}} and \hat{\boldsymbol{\theta}}, pronounced r-hat and theta-hat. Putting a circumflex over a vector this way is often used to mean the unit vector in that direction.

Again, on looking at the diagram we see,
\begin{matrix} 
\mathbf{i}= \hat{\mathbf{r}} \cos \theta  
-\hat{\boldsymbol{\theta}} \sin \theta  &
\hat{\mathbf{r}} = \frac{x}{r}\mathbf{i}+ \frac{y}{r}\mathbf{j} \\
\mathbf{j}= \hat{\mathbf{r}} \sin \theta  
+\hat{\boldsymbol{\theta}} \cos \theta & 
\hat{\boldsymbol{\theta}} =  -\frac{y}{r}\mathbf{i} + \frac{x}{r}\mathbf{j}
\end{matrix}

Three-Dimensional Coordinates and VectorsEdit

Basic definitionEdit

Two-dimensional Cartesian coordinates as we've discussed so far can be easily extended to three-dimensions by adding one more value: 'z'. If the standard (x,y) coordinate axes are drawn on a sheet of paper, the 'z' axis would extend upwards off of the paper.

3D coordinate axes.

Similar to the two coordinate axes in two-dimensional coordinates, there are three coordinate planes in space. These are the xy-plane, the yz-plane, and the xz-plane. Each plane is the "sheet of paper" that contains both axes the name mentions. For instance, the yz-plane contains both the y and z axes and is perpendicular to the x axis.

center|Coordinate planes in space.

Therefore, vectors can be extended to three dimensions by simply adding the 'z' value.

\mathbf{u} = \begin{pmatrix} x \\ y \\ z \end{pmatrix}

To facilitate standard form notation, we add another standard unit vector:

\mathbf{k} = \begin{pmatrix} 0 \\ 0 \\ 1 \end{pmatrix}

Again, both forms (component and standard) are equivalent.

\begin{pmatrix} 1 \\ 2 \\ 3 \end{pmatrix} = 1 \mathbf{i} + 2 \mathbf{j} + 3 \mathbf{k}

Magnitude: Magnitude in three dimensions is the same as in two dimensions, with the addition of a 'z' term in the radicand.

| \mathbf{u} | = \sqrt{u_x^2 + u_y^2 + u_z^2}

Three dimensionsEdit

The polar coordinate system is extended into three dimensions with two different coordinate systems, the cylindrical and spherical coordinate systems, both of which include two-dimensional or planar polar coordinates as a subset. In essence, the cylindrical coordinate system extends polar coordinates by adding an additional distance coordinate, while the spherical system instead adds an additional angular coordinate.

Cylindrical coordinatesEdit

a point plotted with cylindrical coordinates

The cylindrical coordinate system is a coordinate system that essentially extends the two-dimensional polar coordinate system by adding a third coordinate measuring the height of a point above the plane, similar to the way in which the Cartesian coordinate system is extended into three dimensions. The third coordinate is usually denoted h, making the three cylindrical coordinates (r, θ, h).

The three cylindrical coordinates can be converted to Cartesian coordinates by

 \begin{align}
x &= r \, \cos\theta \\
y &= r \, \sin\theta \\
z &= h.
\end{align}

Spherical coordinatesEdit

A point plotted using spherical coordinates

Polar coordinates can also be extended into three dimensions using the coordinates (ρ, φ, θ), where ρ is the distance from the origin, φ is the angle from the z-axis (called the colatitude or zenith and measured from 0 to 180°) and θ is the angle from the x-axis (as in the polar coordinates). This coordinate system, called the spherical coordinate system, is similar to the latitude and longitude system used for Earth, with the origin in the centre of Earth, the latitude δ being the complement of φ, determined by δ = 90° − φ, and the longitude l being measured by l = θ − 180°.

The three spherical coordinates are converted to Cartesian coordinates by

 \begin{align}
x &= \rho \, \sin\phi \, \cos\theta \\
y &= \rho \, \sin\phi \, \sin\theta \\
z &= \rho \, \cos\phi.
\end{align}


r = \sqrt{x^2 + y^2 + z^2},
\theta\ = \arctan{\frac{y}{x}},
\phi\ = \arccos{\frac{z}{r}},

Cross ProductEdit

The cross product of two vectors is a determinant:

 \mathbf{u} \times \mathbf{v} = \begin{vmatrix} \mathbf{i} & \mathbf{j} & \mathbf{k} \\ u_x & u_y & u_z \\ v_x & v_y & v_z \end{vmatrix}

and is also a pseudovector.

The cross product of two vectors is orthogonal to both vectors. The magnitude of the cross product is the product of the magnitude of the vectors and the sin of the angle between them.

 |\mathbf{u} \times \mathbf{v}|=|\mathbf{u}||\mathbf{v}| \sin \theta

This magnitude is the area of the parallelogram defined by the two vectors.

The cross product is linear and anticommutative. For any numbers a and b,

\mathbf{u} \times \left( a\mathbf{v} +b\mathbf{w} \right) =
a \mathbf{u} \times  \mathbf{v} +b\mathbf{u} \times \mathbf{w} 
\quad \mathbf{u} \times  \mathbf{v} = - \mathbf{v} \times  \mathbf{u}

If both vectors point in the same direction, their cross product is zero.

Triple ProductsEdit

If we have three vectors we can combine them in two ways, a triple scalar product,

 \mathbf{u} \cdot (\mathbf{v} \times \mathbf{w})

and a triple vector product

 \mathbf{u} \times (\mathbf{v} \times \mathbf{w})

The triple scalar product is a determinant

 \mathbf{u} \cdot(\mathbf{v} \times \mathbf{w}) = \begin{vmatrix} 
u_x & u_y & u_z \\ v_x & v_y & v_z \\ w_x & w_y & w_z \end{vmatrix}

If the three vectors are listed clockwise, looking from the origin, the sign of this product is positive. If they are listed anticlockwise the sign is negative.

The order of the cross and dot products doesn't matter.

 
\mathbf{u} \cdot (\mathbf{v} \times \mathbf{w}) = 
(\mathbf{u} \times \mathbf{v}) \cdot \mathbf{w}

Either way, the absolute value of this product is the volume of the parallelepiped defined by the three vectors, u, v, and w

The triple vector product can be simplified

 \mathbf{u} \times (\mathbf{v} \times \mathbf{w})
=(\mathbf{u} \cdot \mathbf{w}) \mathbf{v} 
-(\mathbf{u} \cdot \mathbf{v}) \mathbf{w}

This form is easier to do calculations with.

The triple vector product is not associative.

 \mathbf{u} \times (\mathbf{v} \times \mathbf{w})
\ne (\mathbf{u} \times \mathbf{v}) \times \mathbf{w}

There are special cases where the two sides are equal, but in general the brackets matter. They must not be omitted.

Three-Dimensional Lines and PlanesEdit

We will use r to denote the position of a point.

The multiples of a vector, a all lie on a line through the origin. Adding a constant vector b will shift the line, but leave it straight, so the equation of a line is,

\mathbf{r}=\mathbf{a}s+\mathbf{b}

This is a parametric equation. The position is specified in terms of the parameter s.

Any linear combination of two vectors, a and b lies on a single plane through the origin, provided the two vectors are not colinear. We can shift this plane by a constant vector again and write

\mathbf{r}=\mathbf{a}s+\mathbf{b}t+\mathbf{c}

If we choose a and b to be orthonormal vectors in the plane (i.e. unit vectors at right angles) then s and t are Cartesian coordinates for points in the plane.

These parametric equations can be extended to higher dimensions.

Instead of giving parametric equations for the line and plane, we could use constraints. E.g., for any point in the xy plane z=0

For a plane through the origin, the single vector normal to the plane, n, is at right angle with every vector in the plane, by definition, so

\mathbf{r} \cdot \mathbf{n}=0

is a plane through the origin, normal to n.

For planes not through the origin we get

(\mathbf{r}- \mathbf{a}) \cdot \mathbf{n}=0
\quad \mathbf{r} \cdot \mathbf{n}=\mathbf{a} \cdot \mathbf{n}

A line lies on the intersection of two planes, so it must obey the constraint for both planes, i.e.

\mathbf{r} \cdot \mathbf{n}=a \quad \mathbf{r} \cdot \mathbf{m}=b

These constraint equations con also be extended to higher dimensions.

Vector-Valued FunctionsEdit

Vector-Valued Functions are functions that instead of giving a resultant scalar value, give a resultant vector value. These aid in the creation of direction and vector fields, and are therefore used in physics to aid with visualizations of electric, magnetic, and many other types of fields. They are of the following form:

\mathbf{F(t)} = \begin{pmatrix} \mathbf{a_1(t)} \\ \mathbf{a_2(t)} \\ \mathbf{a_3(t)} \\ \mathbf{.} \\ \mathbf{.} \\ \mathbf{a_n(t)} \end{pmatrix}

IntroductionEdit

Limits, Derivatives, and IntegralsEdit

Put simply, the limit of a vector-valued function is the limit of its parts.

Proof:

Suppose \lim_{t \rightarrow c} \mathbf{F}(t) = \mathbf{L} = \begin{pmatrix} \mathbf{a_1} \\ \mathbf{a_2} \\ \mathbf{a_3} \\ \mathbf{.} \\ \mathbf{.} \\ \mathbf{a_n} \end{pmatrix}

Therefore for any \epsilon > 0 there is a \phi > 0 such that

0 <  |t-c| <  \phi \implies |\mathbf{F}(t) - \mathbf{L}| <  \epsilon

But by the triangle inequality |a_1| \le |\mathbf{F}| \le |a_1| + |a_2| + |a_3| + ... + |a_n| |a_1(t) - a_1| \le |\mathbf{F}(t) - \mathbf{L}|

So

0 < |t-c| < \phi  \implies  |a_1(t) - a_1| < \epsilon

Therefore \lim_{t \rightarrow c} a_1(t) = a_1 A similar argument can be used through parts a_n(t)

Now let \lim_{t \rightarrow c} \mathbf{F}(t) = \mathbf{L} = \begin{pmatrix} \mathbf{a_1} \\ \mathbf{a_2} \\ \mathbf{a_3} \\ \mathbf{.} \\ \mathbf{.} \\ \mathbf{a_n} \end{pmatrix} again, and that for any ε>0 there is a corresponding φ>0 such 0<|t-c|<φ implies

|a_n(t) - a_n| < {\epsilon \over n}

Then

0 < |t-c| < \phi  \implies  |\mathbf{F}(t) - \mathbf{L}| \le {\epsilon_1 \over n} + ... + {\epsilon_n \over n} = \epsilon

therefore!:

 \lim_{t \rightarrow c} \mathbf{F}(t) = \mathbf{L} = \begin{pmatrix} \mathbf{a_1} \\ \mathbf{a_2} \\ \mathbf{a_3} \\ \mathbf{.} \\ \mathbf{.} \\ \mathbf{a_n} \end{pmatrix} = \begin{pmatrix} \lim_{t \rightarrow c} \mathbf{a_1(t)} \\ \lim_{t \rightarrow c} \mathbf{a_2(t)} \\ \lim_{t \rightarrow c} \mathbf{a_3(t)} \\ \mathbf{.} \\ \mathbf{.} \\ \lim_{t \rightarrow c} \mathbf{a_n(t)} \end{pmatrix}

From this we can then create an accurate definition of a derivative of a vector-valued function:


\mathbf{F}'(t)=\lim_{h \rightarrow 0} {\mathbf{F}(t+h) - \mathbf{F}(t) \over h}
= \begin{pmatrix} \mathbf{a_1(t)} \\ \mathbf{a_2(t)} \\ \mathbf{a_3(t)} \\ \mathbf{.} \\ \mathbf{.} \\ \mathbf{a_n(t)} \end{pmatrix}

= \lim_{h \rightarrow 0} {\begin{pmatrix} \mathbf{a_1(t + h)} \\ \mathbf{a_2(t + h)} \\ \mathbf{a_3(t + h)} \\ \mathbf{.} \\ \mathbf{.} \\ \mathbf{a_n(t + h)} \end{pmatrix} - \begin{pmatrix} \mathbf{a_1(t)} \\ \mathbf{a_2(t)} \\ \mathbf{a_3(t)} \\ \mathbf{.} \\ \mathbf{.} \\ \mathbf{a_n(t)} \end{pmatrix} \over h}
= \begin{pmatrix} \lim_{h \rightarrow 0} {a_1(t+h) - a_1(t) \over h} \\ \lim_{h \rightarrow 0} {a_2(t+h) - a_2(t) \over h} \\ \lim_{h \rightarrow 0} {a_3(t+h) - a_3(t) \over h} \\ \mathbf{.} \\ \mathbf{.} \\ \lim_{h \rightarrow 0} {a_n(t+h) - a_n(t) \over h} \end{pmatrix}

The final step was accomplished by taking what we just did with limits.

By the Fundamental Theorem of Calculus integrals can be applied to the vector's components.

In other words: the limit of a vector function is the limit of its parts, the derivative of a vector function is the derivative of its parts, and the integration of a vector function is the integration of it parts.

Velocity, Acceleration, Curvature, and a brief mention of the BinormalEdit

Assume we have a vector-valued function which starts at the origin and as its independent variables changes the points that the vectors point at trace a path.

We will call this vector \mathbf{r}(t), which is commonly known as the position vector.

If \mathbf{r} then represents a position and t represents time, then in model with Physics we know the following:

\mathbf{r}(t+h) - \mathbf{r}(t) is displacement. \mathbf{r}'(t) = \mathbf{v}(t) where \mathbf{v}(t) is the velocity vector. |\mathbf{v}(t)| is the speed. \mathbf{r}''(t) = \mathbf{v}'(t) = \mathbf{a}(t) where \mathbf{a}(t) is the acceleration vector.

The only other vector that comes in use at times is known as the curvature vector.

The vector \mathbf{T}(t) used to find it is known as the unit tangent vector, which is defined as \frac{\mathbf{v}(t)}{|\mathbf{v}(t)|} or shorthand \mathbf{\hat v}.

The vector normal \mathbf{N} to this then is \frac{\mathbf{T}'(t)}{|\mathbf{v}(t)|}.

We can verify this by taking the dot product

\mathbf{T} \cdot \mathbf{N} = 0

Also note that |\mathbf{v}(t)| = {ds \over dt}

and

\mathbf{T}(t) = \frac{v}{|v|} = \frac{\frac{dr}{dt}}{\frac{ds}{dt}} = {dr \over ds}

and

\mathbf{N} = \frac{\mathbf{T}'(t)}{|\mathbf{v}(t)|} = \frac{\frac{dT}{dt}}{\frac{ds}{dt}} = {dT \over ds}

Then we can actually verify:

{d \over ds} ( \mathbf{T} \cdot \mathbf{T} )= {d \over ds} (1)

 {dT \over ds} \cdot \mathbf{T} + \mathbf{T} \cdot {dT \over ds} = 0

2 * \mathbf{T} \cdot {dT \over ds} = 0

 \mathbf{T} \cdot {dT \over ds} = 0

 \mathbf{T} \cdot \mathbf{N} = 0

Therefore \mathbf{N} is perpendicular to \mathbf{T}

What this gives rise to is the Unit Normal Vector  \frac{\frac{dT}{ds}}{|\frac{dT}{ds}|} of which the top-most vector is the Normal vector, but the bottom half (|\frac{dT}{ds}|)^{-1} is known as the curvature. Since the Normal vector points toward the inside of a curve, the sharper a turn, the Normal vector has a large magnitude, therefore the curvature has a small value, and is used as an index in civil engineering to reflect the sharpness of a curve (clover-leaf highways, for instance).

The only other thing not mentioned is the Binormal that occurs in 3-d curves \mathbf{T} \times \mathbf{N} = \mathbf{B}, which is useful in creating planes parallel to the curve.

Last modified on 28 January 2014, at 18:10