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Mathematical Tools & Measurement

  1. 01Basic Essential Mathematics
  2. 02Vectors
  3. 03Differentiation
  4. 04Applications of Differentiation
  5. 05Integration
  6. 06Applications of Integration
  7. 07Physical Quantities and Units
  8. 08Dimensional Formula
  9. 09Dimensional Analysis and Its Applications
  10. 10Experimental Skills

Kinematics

  1. 01Motion in One Dimension
  2. 02Motion in Multiple Dimensions
  3. 03Relative Velocity
  4. 04Circular Motion Kinematics
  5. 05Circular Motion Dynamics

Dynamics

  1. 01Forces and Laws of Motion
  2. 02Laws of Motion
  3. 03Friction
  4. 04Force and Potential Energy
  5. 05Fundamentals of Force
  6. 06Newton's Laws and Free Body Diagrams
  7. 07Applications: Objects in Equilibrium
  8. 08Applications: Objects in Motion
  9. 09Constraint Relations
  10. 10Inertial and Non-Inertial Frames
  11. 11Basics of Friction
  12. 12Applications of Friction

Work, Energy, and Power

  1. 01Conservation of Mechanical Energy
  2. 02Work and the Work-Energy Theorem
  3. 03Work and Kinetic Energy Theorem
  4. 04Energy and its Conservation
Theory/Mathematical Tools & Measurement

Mathematical Tools & Measurement · Chapter 01

Basic Essential Mathematics

Basic Essential Mathematics detailed theory study guide for Physics.

85 min read · 6 topics

01

Introduction to Mathematical Foundations

Why Mathematics in Physics?

Physics describes nature in the language of mathematics. The motion of a planet, the fall of a stone, the current in a wire — each is written as an equation. To read physics, you must first read this language.

This chapter builds that foundation. With it you will be able to:

  • State physical quantities precisely
  • Solve physics problems step by step
  • Predict the outcome of a physical process before it happens

Numbers and the Number Line

Every real number has a place on the number line. In physics the number line is a one-dimensional coordinate system: the position of a car on a straight road is a single number.

A number line used as a one-dimensional coordinate system, with the origin marked and the two directions labelled
A number line used as a one-dimensional coordinate system, with the origin marked and the two directions labelled

Negative numbers and absolute value. In physics a negative sign carries direction. A position of −15 m-15 \text{ m}−15 m lies on the opposite side of the origin from +15 m+15 \text{ m}+15 m. The absolute value drops the sign and keeps the size. It answers how much, not which way.

Example. A car moves from position xA=+10 mx_A = +10 \text{ m}xA​=+10 m to position xB=−15 mx_B = -15 \text{ m}xB​=−15 m. Its displacement is Δx=xB−xA=−15−10=−25 m\Delta x = x_B - x_A = -15 - 10 = -25 \text{ m}Δx=xB​−xA​=−15−10=−25 m. The minus sign gives the direction of the change. The distance travelled is the magnitude: ∣Δx∣=∣−25∣=25 m|\Delta x| = |-25| = 25 \text{ m}∣Δx∣=∣−25∣=25 m.

Order of operations (BODMAS/PEMDAS). Every calculation follows one fixed order:

  1. Brackets / Parentheses
  2. Orders / Exponents (powers and roots)
  3. Division and Multiplication (left to right)
  4. Addition and Subtraction (left to right)

Example. Take the kinematic formula s=ut+12at2s = u t + \frac{1}{2} a t^2s=ut+21​at2 with initial velocity u=5 m/su = 5 \text{ m/s}u=5 m/s, time t=4 st = 4 \text{ s}t=4 s, and acceleration a=10 m/s2a = 10 \text{ m/s}^2a=10 m/s2:

s=5×4+12×10×42s = 5 \times 4 + \frac{1}{2} \times 10 \times 4^2s=5×4+21​×10×42

Work through it in order:

  • Exponents: 42=164^2 = 1642=16. The expression becomes 5×4+12×10×165 \times 4 + \frac{1}{2} \times 10 \times 165×4+21​×10×16.
  • Multiplication, left to right: 5×4=205 \times 4 = 205×4=20, and 12×10×16=80\frac{1}{2} \times 10 \times 16 = 8021​×10×16=80. The expression becomes 20+8020 + 8020+80.
  • Addition: 20+80=100 m20 + 80 = 100 \text{ m}20+80=100 m.

If a particle is at position x1=−5 mx_1 = -5 \text{ m}x1​=−5 m and another is at x2=3 mx_2 = 3 \text{ m}x2​=3 m, the distance between them is the absolute value of their difference. What is the distance in meters?

Evaluate: 3+4×23 + 4 \times 23+4×2

02

Algebraic Operations and Equations

Variables, Constants, and Expressions

Algebra states a physical rule once, for every case. Instead of saying that a car moving at 10 m/s10 \text{ m/s}10 m/s for 5 s5 \text{ s}5 s travels 50 m50 \text{ m}50 m, we write d=vtd = vtd=vt. The letters stand for the quantities.

Constants and variables. Take Newton's second law, F=maF = maF=ma. For one object of fixed mass, mmm is a constant, while the applied force FFF and the resulting acceleration aaa are variables.

Examples of expressions:

  • 3x+53x + 53x+5 (linear expression)
  • ut+12at2ut + \frac{1}{2}at^2ut+21​at2 (quadratic expression; the displacement formula)

Simplifying Expressions

Like terms carry the same variable to the same power, and only like terms can be combined.

Example: 3x+5x−2x=6x3x + 5x - 2x = 6x3x+5x−2x=6x

Equations and Isolating Variables

In physics you often know the formula and need one particular variable out of it. Rearranging a formula is therefore a basic skill.

The golden rule. An equation is a balance. Whatever is done to one side — adding, subtracting, multiplying, dividing, squaring, taking a root — must be done to the other. The equality then survives every step.

To take the acceleration out of Newton's second law, F=maF = maF=ma, undo the multiplication by dividing both sides by mmm:

Fm=mam  ⟹  a=Fm\frac{F}{m} = \frac{ma}{m} \implies a = \frac{F}{m}mF​=mma​⟹a=mF​

Linear equations. A linear equation has highest power 1. Its general form is ax+b=cax + b = cax+b=c.

Example. Solve 5x+3=185x + 3 = 185x+3=18.

  • Subtract 3 from both sides: 5x=18−3=155x = 18 - 3 = 155x=18−3=15
  • Divide both sides by 5: x=155=3x = \frac{15}{5} = 3x=515​=3

Rearranging a physics formula. From the kinematics equation v=u+atv = u + atv=u+at, solve for the acceleration aaa:

  • Subtract uuu from both sides: v−u=atv - u = atv−u=at
  • Divide both sides by ttt: a=v−uta = \frac{v - u}{t}a=tv−u​

Solve for xxx: 2x+7=152x + 7 = 152x+7=15

Ratios, Proportions, and Variations

Physical quantities are often tied to one another in fixed proportion. Recognising the form of the tie — direct, inverse, or inverse square — is half the work of a physics problem.

Ratios. A ratio compares two numbers by division. The diameter of a circle is always twice its radius: DR=2\frac{D}{R} = 2RD​=2. Many physical quantities are themselves defined as ratios:

  • Resistance: the ratio of voltage to current, R=VIR = \frac{V}{I}R=IV​ (Ohm's law).
  • Density: the ratio of mass to volume, ρ=mV\rho = \frac{m}{V}ρ=Vm​.

Observe the green curve representing y=1xy = \frac{1}{x}y=x1​ in the graph above. As the variable xxx increases from 1.01.01.0 to 2.02.02.0, what happens to the value of yyy?

  • Direct Variation (y∝xy \propto xy∝x): As one increases, the other increases in the same proportion. Equation: y=kxy = kxy=kx.
  • Inverse Variation (y∝1xy \propto \frac{1}{x}y∝x1​): As one increases, the other decreases. Equation: y=kxy = \frac{k}{x}y=xk​.
  • Inverse Square Variation (y∝1x2y \propto \frac{1}{x^2}y∝x21​): Common throughout physics — gravity and the electric force both follow it.

The gravitational force is inversely proportional to the square of the distance (F∝1r2F \propto \frac{1}{r^2}F∝r21​). If you double the distance, what happens to the force?

Boyle's Law states that for a fixed amount of gas at a constant temperature, pressure PPP is inversely proportional to volume VVV (P∝1VP \propto \frac{1}{V}P∝V1​). If a gas initially at pressure P1P_1P1​ occupies a cylinder, and you compress the gas so that the volume is reduced to one-third of its original size, what happens to the pressure?

Important Algebraic Identities

These identities shorten many derivations in physics. Open each list below:

Square Identities
  • Square of a Sum: (a+b)2=a2+2ab+b2(a + b)^2 = a^2 + 2ab + b^2(a+b)2=a2+2ab+b2
  • Square of a Difference: (a−b)2=a2−2ab+b2(a - b)^2 = a^2 - 2ab + b^2(a−b)2=a2−2ab+b2
  • Difference of Squares: a2−b2=(a+b)(a−b)a^2 - b^2 = (a + b)(a - b)a2−b2=(a+b)(a−b)
  • Square of a Trinomial: (a+b+c)2=a2+b2+c2+2ab+2bc+2ca(a + b + c)^2 = a^2 + b^2 + c^2 + 2ab + 2bc + 2ca(a+b+c)2=a2+b2+c2+2ab+2bc+2ca
Cube Identities
  • Cube of a Sum: (a+b)3=a3+3a2b+3ab2+b3=a3+b3+3ab(a+b)(a + b)^3 = a^3 + 3a^2b + 3ab^2 + b^3 = a^3 + b^3 + 3ab(a + b)(a+b)3=a3+3a2b+3ab2+b3=a3+b3+3ab(a+b)
  • Cube of a Difference: (a−b)3=a3−3a2b+3ab2−b3=a3−b3−3ab(a−b)(a - b)^3 = a^3 - 3a^2b + 3ab^2 - b^3 = a^3 - b^3 - 3ab(a - b)(a−b)3=a3−3a2b+3ab2−b3=a3−b3−3ab(a−b)
  • Sum of Cubes: a3+b3=(a+b)(a2−ab+b2)a^3 + b^3 = (a + b)(a^2 - ab + b^2)a3+b3=(a+b)(a2−ab+b2)
  • Difference of Cubes: a3−b3=(a−b)(a2+ab+b2)a^3 - b^3 = (a - b)(a^2 + ab + b^2)a3−b3=(a−b)(a2+ab+b2)
Product & Advanced Identities
  • Product of Two Binomials: (x+a)(x+b)=x2+(a+b)x+ab(x + a)(x + b) = x^2 + (a + b)x + ab(x+a)(x+b)=x2+(a+b)x+ab
  • Product of Three Binomials: (x+a)(x+b)(x+c)=x3+(a+b+c)x2+(ab+bc+ca)x+abc(x + a)(x + b)(x + c) = x^3 + (a + b + c)x^2 + (ab + bc + ca)x + abc(x+a)(x+b)(x+c)=x3+(a+b+c)x2+(ab+bc+ca)x+abc
  • Sum of Three Cubes Identity: a3+b3+c3−3abc=(a+b+c)(a2+b2+c2−ab−bc−ca)a^3 + b^3 + c^3 - 3abc = (a + b + c)(a^2 + b^2 + c^2 - ab - bc - ca)a3+b3+c3−3abc=(a+b+c)(a2+b2+c2−ab−bc−ca)

Compute 103×97103 \times 97103×97 without long multiplication, using an identity.

If a+b=7a + b = 7a+b=7 and ab=12ab = 12ab=12, what is a2+b2a^2 + b^2a2+b2?

03

Various Functions and Their Graphs

Modeling Relationships

A function is a rule that turns an input into exactly one output. Give the position function a time, and it returns the position at that time. A graph shows the whole rule at once — the entire history of a motion in one picture. The graph below is a first example: the position x=2tx = 2tx=2t of a walker, read off for any time at a glance.

Graphical Analysis in Physics

A graph carries a full table of data in a single figure: the score of a cricket match over by over, the temperature of the Earth year by year, the inflation rate month by month. One glance gives the trend.

Physics uses graphs the same way. The kinetic energy of a car, K=12mv2K = \frac{1}{2}mv^2K=21​mv2, plotted against its speed vvv, rises as a steepening curve: doubling the speed quadruples the destructive energy in a crash.

The slope and the intercepts of such graphs carry physical meaning — an initial velocity, an acceleration.

Understanding the Slope

The slope of a graph is the rate of change of the vertical quantity with respect to the horizontal one. It tells you how fast one quantity changes as the other advances:

  • Constant Slope (Straight Lines): A straight line has one slope along its whole length — a uniform rate of change. In a displacement-time graph, a straight diagonal line means motion at constant velocity.
  • Changing Slope (Curved Lines): On a curve the slope changes from point to point. The slope at any point is the slope of the tangent drawn to the curve there:
    • Increasing Slope: The curve steepens from left to right. In a displacement-time graph this means the velocity is growing — acceleration.
    • Decreasing Slope: The curve flattens. In a displacement-time graph this means the velocity is falling — deceleration.

The three graphs below show the three cases side by side. In the first, equal times bring equal gains in position. In the second, each second brings a larger gain than the one before. In the third, each second brings a smaller gain, and the curve levels off.

1. Linear Functions

A linear function has a constant rate of change. Its graph is a straight line. The general equation is y=mx+cy = mx + cy=mx+c, where mmm is the slope and ccc is the y-intercept.

The Identity Function: y=xy = xy=x

With slope m=1m = 1m=1 and intercept c=0c = 0c=0, the function reduces to y=xy = xy=x, the identity function. Every output equals its input. It describes a one-to-one relationship, such as motion at exactly 1 m/s1\text{ m/s}1 m/s: the displacement in meters equals the time elapsed in seconds.

Changing the Slope: y=2xy = 2xy=2x

Raise the slope to m=2m = 2m=2, keeping c=0c = 0c=0, and the line becomes twice as steep. For every unit change in xxx, the output yyy changes by 2 units. In physics this is motion at a higher constant velocity: at 2 m/s2\text{ m/s}2 m/s, the displacement grows twice as fast as time.

Adding an Offset (y-intercept): y=x+5y = x + 5y=x+5

Keep the slope m=1m = 1m=1 and set the intercept c=5c = 5c=5. The line has the same steepness — it is parallel to y=xy = xy=x — but sits 5 units higher. The intercept is the value of yyy at x=0x = 0x=0. In physics it is the initial value: motion that starts from 5 m5\text{ m}5 m instead of the origin.

Exercise: Match the Line

Adjust the sliders for slope mmm and intercept ccc until your blue line lies on the gold target line.

The temperature at 8:00 am is found to be 36∘C36^\circ\text{C}36∘C. It is increasing linearly by 0.5∘C0.5^\circ\text{C}0.5∘C every hour. At what time will it be 38∘C38^\circ\text{C}38∘C?

2. Quadratic Functions

A quadratic function contains the square of the variable and nothing higher. Its graph is a parabola. The general form is y=ax2+bx+cy = ax^2 + bx + cy=ax2+bx+c. A body in free fall under gravity follows a parabolic trajectory, so parabolas appear throughout mechanics.

Roots of a Quadratic Equation

The roots of a quadratic equation are the values of xxx where the parabola crosses the x-axis (where y=0y = 0y=0). Depending on the discriminant (b2−4acb^2 - 4acb2−4ac), a parabola can have different types of roots:

  • Two distinct real roots: The parabola crosses the x-axis at two different points. For example, y=x2−4y = x^2 - 4y=x2−4 crosses at x=2x = 2x=2 and x=−2x = -2x=−2.
  • One repeated real root: The parabola just touches the x-axis at a single point (its vertex). For example, y=(x−2)2y = (x - 2)^2y=(x−2)2 touches the x-axis exactly at x=2x = 2x=2.
  • No real roots: The parabola never crosses the x-axis; it lies entirely above or below it. For example, y=x2+4y = x^2 + 4y=x2+4 never reaches y=0y = 0y=0.

Transformations of Parabolas

The position of a parabola shifts when its equation is modified:

  • Horizontal Shifts: Replacing xxx with (x+Δx)(x + \Delta x)(x+Δx) shifts the whole graph horizontally. Counter-intuitively, y=(x+2)2y = (x + 2)^2y=(x+2)2 shifts the graph to the left by 2 units, while y=(x−2)2y = (x - 2)^2y=(x−2)2 shifts it to the right by 2 units.
  • Vertical Shifts: Adding a constant to the whole function shifts it along the y-axis. y=x2+3y = x^2 + 3y=x2+3 moves the standard parabola up by 3 units; y=x2−3y = x^2 - 3y=x2−3 moves it down by 3 units.

Exercise: Match the Parabola

Adjust the sliders until your blue curve lies on the gold target parabola.

A ball is thrown upwards. Its height hhh in meters after ttt seconds is given by the quadratic function h(t)=−5t2+20t+2h(t) = -5t^2 + 20t + 2h(t)=−5t2+20t+2. At what time(s) does the ball reach a height of 17 meters17 \text{ meters}17 meters?

The equation of motion of a particle is given by y=3x2+2x+1y = 3x^2 + 2x + 1y=3x2+2x+1. Which type of curve does this represent?

3. Exponential Functions

In an exponential function, the independent variable sits in the exponent. The general mathematical form is:

y=a⋅rx+cy = a \cdot r^x + cy=a⋅rx+c

where each parameter controls one feature of the curve:

  • aaa (Scale Factor): Controls the vertical stretch, compression, or inversion. If a>0a > 0a>0, the curve stays above the asymptote; if a<0a < 0a<0, the curve is flipped upside down.
  • rrr (Base / Growth Rate): Must be a positive number (r>0r > 0r>0). It decides whether the curve grows or decays.
  • ccc (Vertical Shift / Asymptote): Moves the whole graph up or down. The horizontal line y=cy = cy=c is the horizontal asymptote.

Exponential Growth vs. Decay

The behaviour of the function follows from the base rrr:

  • Growth (r>1r > 1r>1): The value climbs faster and faster as xxx increases — the growth of a population, for example.
  • Decay (0<r<10 < r < 10<r<1): The value drops rapidly and levels off towards the asymptote — the cooling of hot tea, or radioactive half-life.

Exercise: Match the Exponential Curve

Adjust the sliders for scale aaa, base rrr, and shift ccc until your blue curve lies on the gold target curve.

A bacterial colony doubles its population every hour. If the initial population at t=0t = 0t=0 is 100100100, which exponential function correctly models the population P(t)P(t)P(t) after ttt hours?

04

Basic Geometry and Graphs

Mapping Space with Geometry

Physics happens in space, and geometry is the tool that maps it. We use it to trace light rays, calculate volumes, and resolve vectors.

Triangles. The Pythagorean theorem and similar triangles do most of the geometric work in this course. Consider a person standing near a street lamp. The lamp, the person, and the light rays form two nested right triangles with the same angles. Comparing the ratios of their sides gives the length of the shadow, or the height of the lamp.

A person standing near a street lamp, showing how the similar triangles are formed between the person, their shadow, and the lamp height.
A person standing near a street lamp, showing how the similar triangles are formed between the person, their shadow, and the lamp height.

Coordinate System and Distance

A coordinate system fixes the position of a point in space by numbers.

The straight-line distance d between P1 and P2, built from a right triangle in the Cartesian plane.
The straight-line distance d between P1P_1P1​ and P2P_2P2​, built from a right triangle in the Cartesian plane.

In a two-dimensional Cartesian plane, the straight-line distance ddd between two points P1(x1,y1)P_1(x_1, y_1)P1​(x1​,y1​) and P2(x2,y2)P_2(x_2, y_2)P2​(x2​,y2​) follows directly from the Pythagorean theorem, as shown above:

d=(x2−x1)2+(y2−y1)2d = \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2}d=(x2​−x1​)2+(y2​−y1​)2​

Three dimensions. Real motion happens in three dimensions. A point then needs three coordinates (x,y,z)(x, y, z)(x,y,z), with the zzz-axis perpendicular to the xyxyxy-plane. The distance formula gains one term:

d=(x2−x1)2+(y2−y1)2+(z2−z1)2d = \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2 + (z_2 - z_1)^2}d=(x2​−x1​)2+(y2​−y1​)2+(z2​−z1​)2​

Slopes and Line Equations

The slope mmm of a line through points P1P_1P1​ and P2P_2P2​ gives the rate of change. On the page, it is the steepness of the line.

The slope of a line as rise over run, read off a right triangle between two points.
The slope of a line as rise over run, read off a right triangle between two points.

m=y2−y1x2−x1=riserunm = \frac{y_2 - y_1}{x_2 - x_1} = \frac{\text{rise}}{\text{run}}m=x2​−x1​y2​−y1​​=runrise​

Equations of Lines:

  • Slope-Intercept Form: y=mx+cy = mx + cy=mx+c, where mmm is the slope and ccc is the yyy-intercept.
  • Point-Slope Form: y−y1=m(x−x1)y - y_1 = m(x - x_1)y−y1​=m(x−x1​), the line through the point (x1,y1)(x_1, y_1)(x1​,y1​) with slope mmm.

Positive Slope: Quantities Rising Together

A positive slope means the vertical variable rises as the horizontal one does. The line climbs from left to right. In physics this is an object moving steadily away from its starting point; the steeper the line, the faster the position changes.

In the graph above, the position rises with time: every second, the object moves 2 meters forward. The graph is a straight line, so the motion is uniform and the velocity constant.

Negative Slope: Quantities Moving Opposite Ways

A negative slope means the vertical variable falls as the horizontal one rises. The line drops from left to right. In physics this is an object returning toward the origin, or moving backward at constant speed.

Here the position falls as time passes. The object starts at 10 m10\text{ m}10 m and moves back toward the origin at a steady 2 m/s2\text{ m/s}2 m/s. The straight line again means constant velocity — now directed the negative way.

Comparing the Two

Both graphs are straight lines, so both show constant velocity. The only difference is the sign of the slope: positive slope, motion in the positive direction; negative slope, motion in the opposite direction. The slope of a position-time graph is the velocity.

Interactive Visualization

Compare the slopes of a linear and a quadratic graph below.

Interactive slope comparison between linear and quadratic functions
Interactive slope comparison between linear and quadratic functions

In a position-time graph (where yyy is position and xxx is time), what physical quantity does the slope of the line represent?

05

Trigonometric Ratios and Identities

Breaking Down Diagonal Forces

A force is rarely applied along a single axis. A rope pulling a crate makes an angle with the floor, and the pull acts partly forward and partly upward. Trigonometry splits such a force into independent horizontal and vertical components. Without it, angled forces cannot be analysed.

Trigonometry is the study of the relations between the angles and sides of triangles. In a right-angled triangle:

A diagonal force pulling a crate on a flat floor, resolved into horizontal and vertical components with the angle marked.
A diagonal force pulling a crate on a flat floor, resolved into horizontal and vertical components with the angle marked.

Six Trigonometric Ratios:

  • sin⁡θ=oppositehypotenuse\sin\theta = \frac{\text{opposite}}{\text{hypotenuse}}sinθ=hypotenuseopposite​
  • cos⁡θ=adjacenthypotenuse\cos\theta = \frac{\text{adjacent}}{\text{hypotenuse}}cosθ=hypotenuseadjacent​
  • tan⁡θ=oppositeadjacent=sin⁡θcos⁡θ\tan\theta = \frac{\text{opposite}}{\text{adjacent}} = \frac{\sin\theta}{\cos\theta}tanθ=adjacentopposite​=cosθsinθ​
  • csc⁡θ=1sin⁡θ\csc\theta = \frac{1}{\sin\theta}cscθ=sinθ1​ (cosecant)
  • sec⁡θ=1cos⁡θ\sec\theta = \frac{1}{\cos\theta}secθ=cosθ1​ (secant)
  • cot⁡θ=1tan⁡θ\cot\theta = \frac{1}{\tan\theta}cotθ=tanθ1​ (cotangent)
A right triangle with the six trigonometric ratios labeled relative to angle theta.
A right triangle with the six trigonometric ratios labeled relative to angle θ\thetaθ.

The Pythagorean Identities

The opposite, adjacent, and hypotenuse of a right triangle always obey the Pythagorean theorem. Dividing that relation through by each side in turn produces three identities that hold for every angle θ\thetaθ. They are among the most used relations in physics, letting you pass between sin⁡\sinsin, cos⁡\coscos, and tan⁡\tantan at will.

sin⁡2θ+cos⁡2θ=1\sin^2\theta + \cos^2\theta = 1sin2θ+cos2θ=1

1+tan⁡2θ=sec⁡2θ1 + \tan^2\theta = \sec^2\theta1+tan2θ=sec2θ

1+cot⁡2θ=csc⁡2θ1 + \cot^2\theta = \csc^2\theta1+cot2θ=csc2θ

The first identity is the Pythagorean theorem applied to the unit circle. Dividing it through by cos⁡2θ\cos^2\thetacos2θ gives the second; dividing it through by sin⁡2θ\sin^2\thetasin2θ gives the third.

Standard Trigonometric Values

Certain angles recur so often in physics that their exact sine, cosine, and tangent values are worth committing to memory:

θ\thetaθ0∘0^\circ0∘30∘30^\circ30∘45∘45^\circ45∘60∘60^\circ60∘90∘90^\circ90∘120∘120^\circ120∘135∘135^\circ135∘150∘150^\circ150∘180∘180^\circ180∘
radians000π/6\pi/6π/6π/4\pi/4π/4π/3\pi/3π/3π/2\pi/2π/22π/32\pi/32π/33π/43\pi/43π/45π/65\pi/65π/6π\piπ
sin⁡θ\sin\thetasinθ00012\frac{1}{2}21​12\frac{1}{\sqrt{2}}2​1​32\frac{\sqrt{3}}{2}23​​11132\frac{\sqrt{3}}{2}23​​12\frac{1}{\sqrt{2}}2​1​12\frac{1}{2}21​000
cos⁡θ\cos\thetacosθ11132\frac{\sqrt{3}}{2}23​​12\frac{1}{\sqrt{2}}2​1​12\frac{1}{2}21​000−12-\frac{1}{2}−21​−12-\frac{1}{\sqrt{2}}−2​1​−32-\frac{\sqrt{3}}{2}−23​​−1-1−1
tan⁡θ\tan\thetatanθ00013\frac{1}{\sqrt{3}}3​1​1113\sqrt{3}3​Not Defined−3-\sqrt{3}−3​−1-1−1−13-\frac{1}{\sqrt{3}}−3​1​000

A force of 10 N10 \text{ N}10 N is applied to a block at an angle of 60∘60^\circ60∘ above the horizontal. What is the magnitude of the horizontal component of this force pulling the block forward? (Given cos⁡(60∘)=0.5\cos(60^\circ) = 0.5cos(60∘)=0.5)

Angles: Degrees and Radians

Angles greater than 90∘90^\circ90∘ matter constantly in physics — a wheel turns through full rotations, not fractions of a right angle. Angles are measured in:

  • Degrees (°): A full circle = 360∘360^\circ360∘
  • Radians (rad): A full circle = 2π rad2\pi \text{ rad}2π rad
The radian defined from a circle: the angle theta subtended at the centre equals the arc length s divided by the radius r.
The radian defined from a circle: the angle θ\thetaθ subtended at the centre equals the arc length sss divided by the radius rrr.

To see what a radian is, take a circle of radius rrr. The angle θ\thetaθ (in radians) subtended at the centre by an arc of length sss is defined as the ratio of arc length to radius:

θ=sr\theta = \frac{s}{r}θ=rs​

On a unit circle (r=1r = 1r=1), the arc length itself is the angle.

A particle moves along a circular path of radius r=2 mr = 2 \text{ m}r=2 m. If it travels an arc length of s=3 ms = 3 \text{ m}s=3 m, what is the angle subtended at the center of the circle?

The Small Angle Approximation

Interactive unit circle demonstrating the small angle approximation where the arc length and vertical height converge.
Interactive unit circle demonstrating the small angle approximation where the arc length and vertical height converge.

For very small angles (typically under 10∘10^\circ10∘), the sine of the angle and the angle itself, measured in radians, are nearly equal: sin⁡θ≈θ\sin\theta \approx \thetasinθ≈θ. Physics uses this constantly — most famously in deriving the time period of a simple pendulum.

In physics, we frequently use the small angle approximation (sin⁡θ≈θ\sin \theta \approx \thetasinθ≈θ) to simplify complex equations. For this approximation to be mathematically valid, how MUST the angle θ\thetaθ be measured?

Angles in All Four Quadrants

In physics, angles greater than 90∘90^\circ90∘ describe rotations and orientations across the Cartesian plane. By convention, positive angles are measured anti-clockwise from the positive x-axis.

The four quadrants of the unit circle with the ASTC rule: which ratios are positive in each quadrant.
The four quadrants of the unit circle with the ASTC rule: which ratios are positive in each quadrant.

Trigonometric Ratios as Coordinates

Instead of opposite and adjacent sides, the ratios can be defined from the coordinates (x,y)(x, y)(x,y) of a point on a circle of radius rrr:

  • sin⁡θ=yr\sin\theta = \frac{y}{r}sinθ=ry​
  • cos⁡θ=xr\cos\theta = \frac{x}{r}cosθ=rx​
  • tan⁡θ=yx\tan\theta = \frac{y}{x}tanθ=xy​
A point P at distance r from the origin, at angle theta. Its coordinates x and y define the trigonometric ratios of theta.
A point PPP at distance rrr from the origin, at angle θ\thetaθ. Its coordinates xxx and yyy define the trigonometric ratios of θ\thetaθ.

The ASTC Rule (All, Sin, Tan, Cos): The coordinates xxx and yyy change sign from quadrant to quadrant, and the ratios change sign with them:

  • Quadrant I (0∘0^\circ0∘ to 90∘90^\circ90∘): Both x and y are positive. All ratios are positive.
  • Quadrant II (90∘90^\circ90∘ to 180∘180^\circ180∘): x is negative, y is positive. Only Sine (and cosecant) are positive.
  • Quadrant III (180∘180^\circ180∘ to 270∘270^\circ270∘): Both x and y are negative. Only Tangent (and cotangent) are positive.
  • Quadrant IV (270∘270^\circ270∘ to 360∘360^\circ360∘): x is positive, y is negative. Only Cosine (and secant) are positive.

Standard Trigonometric Formulas

The analysis of waves and rotations constantly shifts and combines angles. These are the formulas it runs on.

Phase Shifts and Quadrant Reductions

  • sin⁡(π−θ)=sin⁡θ\sin(\pi - \theta) = \sin\thetasin(π−θ)=sinθ and cos⁡(π−θ)=−cos⁡θ\cos(\pi - \theta) = -\cos\thetacos(π−θ)=−cosθ (Quadrant II)
  • sin⁡(π+θ)=−sin⁡θ\sin(\pi + \theta) = -\sin\thetasin(π+θ)=−sinθ and cos⁡(π+θ)=−cos⁡θ\cos(\pi + \theta) = -\cos\thetacos(π+θ)=−cosθ (Quadrant III)
  • sin⁡(2π−θ)=−sin⁡θ\sin(2\pi - \theta) = -\sin\thetasin(2π−θ)=−sinθ and cos⁡(2π−θ)=cos⁡θ\cos(2\pi - \theta) = \cos\thetacos(2π−θ)=cosθ (Quadrant IV)
  • sin⁡(−θ)=−sin⁡θ\sin(-\theta) = -\sin\thetasin(−θ)=−sinθ and cos⁡(−θ)=cos⁡θ\cos(-\theta) = \cos\thetacos(−θ)=cosθ (Even/Odd functions)

Sum, Difference, and Double Angle Formulas

  • sin⁡(A±B)=sin⁡Acos⁡B±cos⁡Asin⁡B\sin(A \pm B) = \sin A \cos B \pm \cos A \sin Bsin(A±B)=sinAcosB±cosAsinB
  • cos⁡(A±B)=cos⁡Acos⁡B∓sin⁡Asin⁡B\cos(A \pm B) = \cos A \cos B \mp \sin A \sin Bcos(A±B)=cosAcosB∓sinAsinB
  • sin⁡(2θ)=2sin⁡θcos⁡θ\sin(2\theta) = 2\sin\theta\cos\thetasin(2θ)=2sinθcosθ
  • cos⁡(2θ)=cos⁡2θ−sin⁡2θ=1−2sin⁡2θ=2cos⁡2θ−1\cos(2\theta) = \cos^2\theta - \sin^2\theta = 1 - 2\sin^2\theta = 2\cos^2\theta - 1cos(2θ)=cos2θ−sin2θ=1−2sin2θ=2cos2θ−1
Worked Example 1: Converting Degrees to Radians

Problem: Convert 270∘270^\circ270∘ into radians.

Solution: Since π rad=180∘\pi \text{ rad} = 180^\circπ rad=180∘, every degree measure converts on multiplication by π180∘\frac{\pi}{180^\circ}180∘π​:

270∘=270∘180∘×π=1.5π rad270^\circ = \frac{270^\circ}{180^\circ} \times \pi = 1.5\pi \text{ rad}270∘=180∘270∘​×π=1.5π rad

Now Solve: Convert 150∘150^\circ150∘ into radians. (Answer: 5π6 rad\frac{5\pi}{6} \text{ rad}65π​ rad)

Worked Example 2: Identifying the Quadrant

Problem: If sin⁡θ<0\sin\theta < 0sinθ<0, tan⁡θ<0\tan\theta < 0tanθ<0, and cos⁡θ>0\cos\theta > 0cosθ>0, in which quadrant does θ\thetaθ lie?

Solution: Check each condition against the ASTC rule separately, then find the quadrant common to all three:

  • sin⁡θ<0\sin\theta < 0sinθ<0 ⇒\Rightarrow⇒ 3rd or 4th quadrant
  • tan⁡θ<0\tan\theta < 0tanθ<0 ⇒\Rightarrow⇒ 2nd or 4th quadrant
  • cos⁡θ>0\cos\theta > 0cosθ>0 ⇒\Rightarrow⇒ 1st or 4th quadrant

All three conditions are satisfied only in the 4th quadrant.

Now Solve: If sin⁡θ×cos⁡θ>0\sin\theta \times \cos\theta > 0sinθ×cosθ>0, in which quadrant(s) does θ\thetaθ lie? (Answer: 1st or 3rd quadrant)

Worked Example 3: Simplifying a Trigonometric Expression

Problem: Find the value of sin⁡28∘cos⁡17∘+sin⁡62∘cos⁡73∘\sin 28^\circ \cos 17^\circ + \sin 62^\circ \cos 73^\circsin28∘cos17∘+sin62∘cos73∘.

Solution: Rewrite 62∘62^\circ62∘ and 73∘73^\circ73∘ using the co-function identities sin⁡(90∘−θ)=cos⁡θ\sin(90^\circ - \theta) = \cos\thetasin(90∘−θ)=cosθ and cos⁡(90∘−θ)=sin⁡θ\cos(90^\circ - \theta) = \sin\thetacos(90∘−θ)=sinθ, so that both terms share the same angle sum:

sin⁡28∘cos⁡17∘+sin⁡62∘cos⁡73∘=sin⁡28∘cos⁡17∘+sin⁡(90∘−28∘)cos⁡(90∘−17∘)\sin 28^\circ \cos 17^\circ + \sin 62^\circ \cos 73^\circ = \sin 28^\circ \cos 17^\circ + \sin(90^\circ - 28^\circ)\cos(90^\circ - 17^\circ)sin28∘cos17∘+sin62∘cos73∘=sin28∘cos17∘+sin(90∘−28∘)cos(90∘−17∘)

=sin⁡28∘cos⁡17∘+cos⁡28∘sin⁡17∘=sin⁡(28∘+17∘)=sin⁡45∘=12= \sin 28^\circ \cos 17^\circ + \cos 28^\circ \sin 17^\circ = \sin(28^\circ + 17^\circ) = \sin 45^\circ = \frac{1}{\sqrt{2}}=sin28∘cos17∘+cos28∘sin17∘=sin(28∘+17∘)=sin45∘=2​1​

Now Solve: Find cos⁡8∘cos⁡52∘−cos⁡82∘cos⁡38∘\cos 8^\circ \cos 52^\circ - \cos 82^\circ \cos 38^\circcos8∘cos52∘−cos82∘cos38∘. (Answer: 0.50.50.5)

Worked Example 4: Sum of Two Angles from Their Tangents

Problem: If tan⁡A=12\tan A = \frac{1}{2}tanA=21​ and tan⁡B=13\tan B = \frac{1}{3}tanB=31​, find (A+B)(A+B)(A+B).

Solution: Apply the tangent sum formula directly:

tan⁡(A+B)=tan⁡A+tan⁡B1−tan⁡Atan⁡B=12+131−12⋅13=5/65/6=1\tan(A+B) = \frac{\tan A + \tan B}{1 - \tan A \tan B} = \frac{\frac{1}{2} + \frac{1}{3}}{1 - \frac{1}{2}\cdot\frac{1}{3}} = \frac{5/6}{5/6} = 1tan(A+B)=1−tanAtanBtanA+tanB​=1−21​⋅31​21​+31​​=5/65/6​=1

Since tan⁡(A+B)=1\tan(A+B) = 1tan(A+B)=1, it follows that A+B=45∘=π4A + B = 45^\circ = \frac{\pi}{4}A+B=45∘=4π​.

Now Solve: Using the same AAA and BBB, find tan⁡(A−B)\tan(A-B)tan(A−B). (Answer: 17\frac{1}{7}71​)

06

Key Concepts

Numbers, Algebra, and Equations

  • The number line is a coordinate system. A position is a single real number; the sign carries direction, and the absolute value ∣x∣|x|∣x∣ keeps the size and drops the sign. Displacement is Δx=xB−xA\Delta x = x_B - x_AΔx=xB​−xA​; distance is its magnitude ∣Δx∣|\Delta x|∣Δx∣.
  • Order of operations (BODMAS). Brackets, then exponents, then division and multiplication left to right, then addition and subtraction left to right.
  • An equation is a balance. Whatever is done to one side — adding, subtracting, multiplying, dividing, squaring, taking a root — must be done to the other. This is the whole method of rearranging formulas: from F=maF = maF=ma, dividing both sides by mmm gives a=Fma = \frac{F}{m}a=mF​; from v=u+atv = u + atv=u+at, a=v−uta = \frac{v - u}{t}a=tv−u​.
  • Only like terms combine: 3x+5x−2x=6x3x + 5x - 2x = 6x3x+5x−2x=6x.
  • The three variations. Direct: y=kxy = kxy=kx — doubling xxx doubles yyy. Inverse: y=kxy = \frac{k}{x}y=xk​ — doubling xxx halves yyy (Boyle's law). Inverse square: y=kx2y = \frac{k}{x^2}y=x2k​ — doubling xxx cuts yyy to one fourth (gravity, the electric force).

Algebraic Identities Worth Keeping at Hand

  • (a+b)2=a2+2ab+b2(a + b)^2 = a^2 + 2ab + b^2(a+b)2=a2+2ab+b2 and (a−b)2=a2−2ab+b2(a - b)^2 = a^2 - 2ab + b^2(a−b)2=a2−2ab+b2 — note the cross term 2ab2ab2ab; the common error is to drop it.
  • a2−b2=(a+b)(a−b)a^2 - b^2 = (a + b)(a - b)a2−b2=(a+b)(a−b) — the difference of squares, the fastest factoring tool in the kit.
  • (a±b)3=a3±b3±3ab(a±b)(a \pm b)^3 = a^3 \pm b^3 \pm 3ab(a \pm b)(a±b)3=a3±b3±3ab(a±b)
  • a3±b3=(a±b)(a2∓ab+b2)a^3 \pm b^3 = (a \pm b)(a^2 \mp ab + b^2)a3±b3=(a±b)(a2∓ab+b2)
  • (x+a)(x+b)=x2+(a+b)x+ab(x + a)(x + b) = x^2 + (a + b)x + ab(x+a)(x+b)=x2+(a+b)x+ab

Geometry, Graphs, and Functions

  • Distance between two points. In a plane, d=(x2−x1)2+(y2−y1)2d = \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2}d=(x2​−x1​)2+(y2​−y1​)2​; in three dimensions the formula gains the term (z2−z1)2(z_2 - z_1)^2(z2​−z1​)2. Both are the Pythagorean theorem in coordinates.
  • Slope is rate of change: m=y2−y1x2−x1=riserunm = \frac{y_2 - y_1}{x_2 - x_1} = \frac{\text{rise}}{\text{run}}m=x2​−x1​y2​−y1​​=runrise​. On a position-time graph the slope is the velocity; its sign gives the direction of motion. On a curve, the slope at a point is the slope of the tangent there.
  • Lines: y=mx+cy = mx + cy=mx+c (slope-intercept) and y−y1=m(x−x1)y - y_1 = m(x - x_1)y−y1​=m(x−x1​) (point-slope). The intercept ccc is the initial value.
  • Quadratics: y=ax2+bx+cy = ax^2 + bx + cy=ax2+bx+c graphs as a parabola, opening up for a>0a > 0a>0 and down for a<0a < 0a<0. The discriminant b2−4acb^2 - 4acb2−4ac decides the roots: positive gives two crossings of the x-axis, zero a single touch, negative none. Replacing xxx by x−hx - hx−h shifts the graph right by hhh; adding a constant shifts it up.
  • Exponentials: y=a⋅rx+cy = a \cdot r^x + cy=a⋅rx+c. Growth for r>1r > 1r>1, decay towards the asymptote y=cy = cy=c for 0<r<10 < r < 10<r<1. Doubling and half-life are the physical faces of the two cases.

Trigonometry

  • The ratios. sin⁡θ=opphyp\sin\theta = \frac{\text{opp}}{\text{hyp}}sinθ=hypopp​, cos⁡θ=adjhyp\cos\theta = \frac{\text{adj}}{\text{hyp}}cosθ=hypadj​, tan⁡θ=sin⁡θcos⁡θ\tan\theta = \frac{\sin\theta}{\cos\theta}tanθ=cosθsinθ​, with csc⁡\csccsc, sec⁡\secsec, cot⁡\cotcot their reciprocals. On a circle of radius rrr: sin⁡θ=yr\sin\theta = \frac{y}{r}sinθ=ry​, cos⁡θ=xr\cos\theta = \frac{x}{r}cosθ=rx​, tan⁡θ=yx\tan\theta = \frac{y}{x}tanθ=xy​.
  • Component resolution. A force FFF at angle θ\thetaθ to the horizontal acts as Fcos⁡θF\cos\thetaFcosθ horizontally and Fsin⁡θF\sin\thetaFsinθ vertically. On an incline, gravity splits into mgsin⁡θmg\sin\thetamgsinθ along the slope and mgcos⁡θmg\cos\thetamgcosθ into it.
  • Pythagorean identities: sin⁡2θ+cos⁡2θ=1\sin^2\theta + \cos^2\theta = 1sin2θ+cos2θ=1, 1+tan⁡2θ=sec⁡2θ1 + \tan^2\theta = \sec^2\theta1+tan2θ=sec2θ, 1+cot⁡2θ=csc⁡2θ1 + \cot^2\theta = \csc^2\theta1+cot2θ=csc2θ.
  • Radians. θ=sr\theta = \frac{s}{r}θ=rs​; a full circle is 2π2\pi2π rad and π\piπ rad =180∘= 180^\circ=180∘. The radian is dimensionless.
  • Small angles (in radians, under about 10∘10^\circ10∘): sin⁡θ≈θ\sin\theta \approx \thetasinθ≈θ — the approximation behind the simple pendulum.
  • Signs by quadrant (ASTC): all positive in I; only sine in II; only tangent in III; only cosine in IV.
  • Combining angles: sin⁡(A±B)=sin⁡Acos⁡B±cos⁡Asin⁡B\sin(A \pm B) = \sin A \cos B \pm \cos A \sin Bsin(A±B)=sinAcosB±cosAsinB, cos⁡(A±B)=cos⁡Acos⁡B∓sin⁡Asin⁡B\cos(A \pm B) = \cos A \cos B \mp \sin A \sin Bcos(A±B)=cosAcosB∓sinAsinB, sin⁡2θ=2sin⁡θcos⁡θ\sin 2\theta = 2\sin\theta\cos\thetasin2θ=2sinθcosθ, cos⁡2θ=cos⁡2θ−sin⁡2θ\cos 2\theta = \cos^2\theta - \sin^2\thetacos2θ=cos2θ−sin2θ.
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