Comprehensive Guide to Parametrics, Vectors, and Matrices

4.1 Parametric Functions

Definitions & Concepts

Parametric functions allow us to define curves that are not necessarily functions of xx (i.e., they can fail the vertical line test). Instead of relating yy directly to xx, we define both variables in terms of a third independent variable called the parameter, usually denoted by tt.

  • Notation: A parametric function is written as a set of equations: x=f(t)x = f(t) and y=g(t)y = g(t).
  • Coordinate Points: At any specific value tt, the coordinate is (f(t),g(t))(f(t), g(t)).
  • Orientation: The direction the graph is traced as tt increases is called the orientation of the curve.
Graphing Parametric Functions

To graph a parametric equation:

  1. Create a table with columns for tt, x(t)x(t), and y(t)y(t).
  2. Select values for tt within the given domain.
  3. Calculate the resulting (x,y)(x, y) coordinate pairs.
  4. Plot points and connect them in order of increasing tt.

f(t)={x(t)=t2−1 y(t)=2tf(t) = \begin{cases} x(t) = t^2 - 1 \ y(t) = 2t \end{cases}

Graph of a parametric parabola showing orientation arrows

Eliminating the Parameter

To convert a parametric equation to a Cartesian (rectangular) equation (y=f(x)y=f(x)):

  1. Solve one equation for tt (e.g., t=x/2t = x/2).
  2. Substitute this expression into the other equation.

Example:
Given x=2tx = 2t and y=t2+1y = t^2 + 1:

  1. Solve for tt: t=x2t = \frac{x}{2}.
  2. Substitute into yy: y=(x2)2+1⇒y=x24+1y = (\frac{x}{2})^2 + 1 \Rightarrow y = \frac{x^2}{4} + 1.

4.2 Parametric Functions Modeling Planar Motion

Analyzing Particle Motion

In physics and applied mathematics, parametric equations often model the position of a particle at time tt.

  • x(t)x(t): The horizontal position of the particle.
  • y(t)y(t): The vertical position of the particle.
  • Domain: Usually t≥0t \geq 0 (time cannot be negative), but context determines the domain.
Extrema (Maximums and Minimums)

To find the boundaries of motion:

  • Horizontal Extrema: Find the maximum and minimum values of x(t)x(t). These represent the usually "rightmost" and "leftmost" points.
  • Vertical Extrema: Find the maximum and minimum values of y(t)y(t). These represent the "highest" and "lowest" points.

Example:
If x(t)=sin⁡(t)x(t) = \sin(t) and y(t)=t2y(t) = t^2 on [0,π][0, \pi]:

  • Max horizontal Position: x=1x=1 at t=π/2t=\pi/2.
  • Max vertical Position: y=π2y=\pi^2 at t=πt=\pi.

4.3 Parametric Functions and Rates of Change

Direction of Motion

To understand how a particle moves, we analyze the rate of change of xx and yy independently.

ConditionInterpretation
xx is increasingParticle moves to the right
xx is decreasingParticle moves to the left
yy is increasingParticle moves up
yy is decreasingParticle moves down
Average Rate of Change (AROC)

The average rate of change describes how the position changes over an interval [a,b][a, b]. Unlike standard functions, we calculate AROC for each component separately:

  • AROC of x: x(b)−x(a)b−a\frac{x(b) - x(a)}{b - a} (Average horizontal velocity)
  • AROC of y: y(b)−y(a)b−a\frac{y(b) - y(a)}{b - a} (Average vertical velocity)

4.4 Parametrically Defined Functions

Parametrizing Circles

The Unit Circle is the foundation for parametrizing circular motion. Based on the Pythagorean identity cos⁡2θ+sin⁡2θ=1\cos^2 \theta + \sin^2 \theta = 1:

General Standard Form for a Circle:
{x(t)=rcos⁡(b(t−h))+x<em>c y(t)=rsin⁡(b(t−h))+y</em>c\begin{cases} x(t) = r \cos(b(t-h)) + x<em>c \ y(t) = r \sin(b(t-h)) + y</em>c \end{cases}

  • (x<em>c,y</em>c)(x<em>c, y</em>c): Center of the circle.
  • rr: Radius.
  • tt: Angle parameter (often θ\theta).
  • Period: Standard circle completes in 2π2\pi. If the argument is btbt, the period changes to 2π/b2\pi/b.

Unit circle with coordinates labeled as (cos t, sin t)

Parametrizing Line Segments

To describe linear motion from Point A (x<em>1,y</em>1)(x<em>1, y</em>1) to Point B (x<em>2,y</em>2)(x<em>2, y</em>2):

{x(t)=x<em>1+t(x</em>2−x<em>1) y(t)=y</em>1+t(y<em>2−y</em>1)\begin{cases} x(t) = x<em>1 + t(x</em>2 - x<em>1) \ y(t) = y</em>1 + t(y<em>2 - y</em>1) \end{cases}

  • For 0≤t≤10 \leq t \leq 1, the particle starts at A and ends at B.

4.5 Implicitly Defined Functions

Concepts

An implicitly defined function relates xx and yy in a single equation where one variable is not isolated (e.g., x2+y2=25x^2 + y^2 = 25 or x3+y3=9xyx^3 + y^3 = 9xy).

  • Verifying Points: To check if a point (a,b)(a, b) is on the graph, substitute x=ax=a and y=by=b. If the equation yields a true statement (e.g., 25=2525=25), the point lies on the curve.
  • Graphing: These often define non-functions (like circles, ellipses, or hyperbolas) which may require solving for yy (often resulting in ±\pm square roots) to graph on a standard calculator.

4.6 Conic Sections

We can represent conic sections using parametric equations to easily graph and analyze them.

Ellipses

For an ellipse centered at (h,k)(h, k) with horizontal radius aa and vertical radius bb:

  • Implicit: (x−h)2a2+(y−k)2b2=1\frac{(x-h)^2}{a^2} + \frac{(y-k)^2}{b^2} = 1
  • Parametric:
    x(t)=acos⁡(t)+hx(t) = a \cos(t) + h
    y(t)=bsin⁡(t)+ky(t) = b \sin(t) + k
    for 0≤t≤2π0 \leq t \leq 2\pi.
Hyperbolas

For a hyperbola opening horizontally:

  • Implicit: (x−h)2a2−(y−k)2b2=1\frac{(x-h)^2}{a^2} - \frac{(y-k)^2}{b^2} = 1
  • Parametric:
    x(t)=h+asec⁡(t)x(t) = h + a \sec(t)
    y(t)=k+btan⁡(t)y(t) = k + b \tan(t)

4.8 Vectors

Vector Fundamentals

A Vector is a quantity defined by both magnitude (length) and direction. It is represented geometrically as a directed line segment (arrow).

  • Component Form: v=⟨a,b⟩\mathbf{v} = \langle a, b \rangle. This represents the change in xx (aa) and the change in yy (bb) from the tail to the head.
  • Zero Vector: 0=⟨0,0⟩\mathbf{0} = \langle 0, 0 \rangle.
Magnitude and Direction

Given vector v=⟨a,b⟩\mathbf{v} = \langle a, b \rangle:

  1. Magnitude (∣∣v∣∣||\mathbf{v}||): Pythagorean theorem.
    ∣∣v∣∣=a2+b2||\mathbf{v}|| = \sqrt{a^2 + b^2}
  2. Direction Angle (θ\theta): Using trigonometry.
    tan⁡θ=ba  ⟹  θ=tan⁡−1(ba)\tan \theta = \frac{b}{a} \implies \theta = \tan^{-1}\left(\frac{b}{a}\right)
    Note: You must adjust θ\theta based on the quadrant where (a,b)(a,b) is located.
Vector Operations

Given u=⟨u<em>1,u</em>2⟩\mathbf{u} = \langle u<em>1, u</em>2 \rangle, v=⟨v<em>1,v</em>2⟩\mathbf{v} = \langle v<em>1, v</em>2 \rangle, and scalar kk:

  • Addition: u+v=⟨u<em>1+v</em>1,u<em>2+v</em>2⟩\mathbf{u} + \mathbf{v} = \langle u<em>1+v</em>1, u<em>2+v</em>2 \rangle
  • Scalar Multiplication: ku=⟨ku<em>1,ku</em>2⟩k\mathbf{u} = \langle k u<em>1, k u</em>2 \rangle

Visual diagram of Vector Addition (Head-to-Tail method)


4.9 Vector-Valued Functions

Position Vectors

A vector-valued function p(t)\mathbf{p}(t) describes the position of a particle at time tt as a vector from the origin (0,0)(0,0) to the point (x(t),y(t))(x(t), y(t)).

p(t)=⟨x(t),y(t)⟩=x(t)i+y(t)j\mathbf{p}(t) = \langle x(t), y(t) \rangle = x(t)\mathbf{i} + y(t)\mathbf{j}

  • Radius: The magnitude ∣∣p(t)∣∣||\mathbf{p}(t)|| represents the distance of the particle from the origin.
Velocity Vectors

The velocity vector v(t)\mathbf{v}(t) represents the instantaneous speed and direction of motion.

  • If position is linear, velocity is constant.
  • Speed: The magnitude of the velocity vector is the speed of the particle.

4.10 Matrices

Concepts & Notation

A Matrix is a rectangular array of numbers. Dimensions are given as Rows×ColumnsRows \times Columns (R×CR \times C).

A=[123 456]A = \begin{bmatrix} 1 & 2 & 3 \ 4 & 5 & 6 \end{bmatrix}

  • This is a 2×32 \times 3 matrix (2 rows, 3 columns).
  • Element a2,3a_{2,3} is the entry in Row 2, Column 3 (value is 6).
Matrix Multiplication

To multiply Matrix AA (m×nm \times n) by Matrix BB (n×pn \times p), the inner dimensions (nn) must match. The result will be size m×pm \times p.

The Rule: Row by Column
To find the entry in, say, row 1 column 1 for the result, you take the Dot Product of Row 1 from Matrix A and Column 1 from Matrix B.

[ab cd]⋅[x y]=[(a)(x)+(b)(y) (c)(x)+(d)(y)]\begin{bmatrix} a & b \ c & d \end{bmatrix} \cdot \begin{bmatrix} x \ y \end{bmatrix} = \begin{bmatrix} (a)(x) + (b)(y) \ (c)(x) + (d)(y) \end{bmatrix}

Mnemonics:

RC Cola: Always multiply Rows by Columns.


4.11 The Inverse and Determinant of a Matrix

The Determinant

For a 2×22 \times 2 square matrix A=[ab cd]A = \begin{bmatrix} a & b \ c & d \end{bmatrix}:

det⁡(A)=ad−bc\det(A) = ad - bc

  • Geometric Meaning: The absolute value ∣det⁡(A)∣|\det(A)| is the area of the parallelogram formed by the vectors ⟨a,c⟩\langle a, c \rangle and ⟨b,d⟩\langle b, d \rangle.
  • If det⁡(A)=0\det(A) = 0, the matrix is singular (non-invertible).
The Inverse Matrix

The inverse A−1A^{-1} "undoes" matrix A. When multiplied, A⋅A−1=IA \cdot A^{-1} = I (Identity Matrix).

A−1=1ad−bc[d−b −ca]A^{-1} = \frac{1}{ad-bc} \begin{bmatrix} d & -b \ -c & a \end{bmatrix}

  • Note: We swap the main diagonal elements (aa and dd) and negate the other diagonal (bb and cc).

4.12 Linear Transformations and Matrices

Defining Linear Transformations

A transformation LL is linear if it preserves vector addition and scalar multiplication. Essentially, it keeps grid lines parallel and the origin fixed.

Any linear transformation from R2\mathbb{R}^2 to R2\mathbb{R}^2 can be defined by a 2×22 \times 2 matrix MM.

Output Vector=Matrix M×Input Vector v\text{Output Vector} = \text{Matrix } M \times \text{Input Vector } \mathbf{v}

Mapping Basis Vectors

To construct a transformation matrix, figure out where the unit vectors i=⟨1,0⟩\mathbf{i} = \langle 1, 0 \rangle and j=⟨0,1⟩\mathbf{j} = \langle 0, 1 \rangle go.

  • Column 1 of matrix MM is the new position of i\mathbf{i}.
  • Column 2 of matrix MM is the new position of j\mathbf{j}.

Grid transformation showing basis vectors i and j moving to new positions


4.13 Matrices as Functions

Composition of Functions

If Matrix AA represents transformation ff, and Matrix BB represents transformation gg:

  • The transformation f(g(v))f(g(\mathbf{v})) (applying gg first, then ff) is represented by the matrix product A⋅BA \cdot B.
  • Order Matters: Since matrix multiplication is not commutative (AB≠BAAB \neq BA), the order of transformations matters. The transformation applied first is the matrix on the right.
Inverse Transformations

If a transformation scales and rotates a vector, the inverse matrix reverses that process, returning the vector to its original state.


4.14 Matrices Modeling Contexts

Transition Matrices (Markov Chains)

Matrices are powerful tools for modeling states changing over time (e.g., population migration, customer retention).

  • State Vector (S0S_0): A column matrix representing the initial populations or proportions.
  • Transition Matrix (TT): Contains the probabilities or rates of moving from state jj (columns) to state ii (rows).

Equation for Next State:
S<em>n+1=T⋅S</em>nS<em>{n+1} = T \cdot S</em>n

To find the state after kk steps:
S<em>k=Tk⋅S</em>0S<em>k = T^k \cdot S</em>0

Common Mistakes & Pitfalls
  1. Order of Matrix Multiplication: Students often multiply S<em>n×TS<em>n \times T. This is usually dimensionally impossible. It must be T×S</em>nT \times S</em>n (Matrix ×\times Vector).
  2. Calculator Mode: When working with parametric equations involving trig (Circles/Ellipses), ensure your calculator is in Radian mode unless specified otherwise.
  3. Vector Brackets: Do not use parentheses (a,b)(a, b) for vectors; use chevrons ⟨a,b⟩\langle a, b \rangle to distinguish them from points.
  4. Inverse Elements: In the inverse formula, students often forget to negate bb and cc, or they swap them instead of swapping aa and dd.
  5. Determinant Calculation: A common error is calculating ad+bcad + bc instead of ad−bcad - bc.