Lower 6 Cameroon A-Level Physics: Mechanics (Detailed Notes)

1. Introduction to Mechanics

Mechanics is the branch of physics concerned with the study of motion, forces, energy, and momentum. It forms a core part of the Lower 6 Cameroon syllabus.

Main topics include:

2. Kinematics

Kinematics describes motion without considering the forces causing it.

2.1 Scalars and Vectors

2.2 Displacement, Velocity, and Acceleration

Displacement: s = x_final - x_initial
Velocity: v = ds/dt (instantaneous),
Average: v_avg = Δs/Δt
Acceleration: a = dv/dt (instantaneous),
Average: a_avg = Δv/Δt

2.3 Equations of Motion (Constant Acceleration)

v = u + at
s = ut + 1/2 at²
v² = u² + 2as
s = ((u+v)/2) × t

Where: u = initial velocity, v = final velocity, a = acceleration, t = time, s = displacement

2.4 Motion in Two Dimensions

Break motion into x and y components:

v_x = v cos θ, v_y = v sin θ
x = u_x t, y = u_y t - 1/2 g t²

Projectile motion: horizontal velocity constant, vertical motion under gravity.

Projectile Motion Diagram

3. Dynamics

Dynamics deals with forces and their effects on motion.

3.1 Newton’s Laws of Motion

3.2 Types of Forces

3.3 Friction

f = μ × N
where μ = coefficient of friction, N = normal reaction

3.4 Circular Motion

For uniform circular motion:

Centripetal acceleration: a_c = v² / r
Centripetal force: F_c = m × v² / r

Where r = radius, v = speed, m = mass

4. Work, Energy, and Power

4.1 Work Done

W = F × d × cos θ

Work is positive when force and displacement are in same direction; negative if opposite.

4.2 Kinetic and Potential Energy

KE = 1/2 m v²
PE = m g h

Law of conservation of energy: Total energy remains constant in an isolated system.

4.3 Power

P = W / t = F × v (if force and velocity are in same direction)

5. Linear Momentum and Impulse

5.1 Linear Momentum

p = m × v

Where p = momentum, m = mass, v = velocity

5.2 Impulse

J = F × Δt = Δp

Impulse = change in momentum. Useful in collision problems.

5.3 Conservation of Momentum

In absence of external forces, total momentum before collision = total momentum after collision.

6. Gravitation

Newton’s law of universal gravitation:

F = G × (m₁ m₂) / r²

Where G = 6.674 × 10⁻¹¹ N·m²/kg², r = distance between centers

6.1 Acceleration Due to Gravity

g = G × M / R²

Where M = mass of planet, R = radius of planet

6.2 Orbital Motion

Centripetal force = gravitational force: m v² / r = G m M / r² → v = √(G M / r)

Orbital period: T = 2π r / v

7. Oscillations (Simple Harmonic Motion)

7.1 SHM Basics

Displacement varies sinusoidally with time:

x = A cos(ω t + φ)

Velocity: v = dx/dt = -A ω sin(ω t + φ)
Acceleration: a = dv/dt = -ω² x

7.2 Period and Frequency

T = 2π / ω
f = 1 / T

7.3 Energy in SHM

Total energy: E = 1/2 k A² (constant)
KE = 1/2 m v², PE = 1/2 k x²

8. Example Problems

Example 1: A car accelerates from 0 to 20 m/s in 10 s. Find acceleration and distance traveled.

Solution: a = Δv / t = 20 / 10 = 2 m/s²
s = ut + 1/2 at² = 0 + 0.5 × 2 × 10² = 100 m

Example 2: A 2 kg mass moves in a circle of radius 0.5 m at 4 m/s. Find centripetal force.

Solution: F_c = m v² / r = 2 × 16 / 0.5 = 64 N

9. Diagram Placeholders

10. Tips for Exams