CAPE Physics Unit 1 study materials
CAPE Physics Unit 1 study resources

CAPE Physics Unit 1 cheat sheet

CAPE Physics Unit 1 · Keep the key ideas within reach.

Quick reference

Mechanics

  • Resolve vectors before applying F = ma or the SUVAT equations

  • Momentum is a vector: conserve each component only when the corresponding net external impulse is zero

  • Equilibrium requires both zero resultant force and zero resultant moment

  • The centripetal component points to the centre; uniform circular motion has constant speed but changing velocity

  • SHM signature: a = −ω²x, giving T = 2π/ω

  • State g and sign conventions explicitly at the start of a solution

Quick reference

Waves and Optics

  • Phase difference = 2π × path difference/λ

  • Stationary waves: node spacing λ/2, node–antinode λ/4, no energy transfer

  • Grating equation d sinθ = nλ with d = 1/N in metres

  • Young's slits: x = λD/a for small angles

  • Snell: n₁ sinθ₁ = n₂ sinθ₂; critical angle sinθc = n₂/n₁ requires n₁ > n₂

  • Keep one lens sign convention throughout and state it

Quick reference

Thermal Physics

  • Use kelvin in all gas-law and kinetic-theory calculations

  • Q = mcΔθ for temperature change; Q = mL for change of state

  • Mixtures: heat lost by hot bodies = heat gained by cold bodies plus calorimeter

  • pV = nRT and pV = ⅓Nm⟨c²⟩; mean KE = (3/2)kT

  • For a fixed amount of an ideal gas, internal energy depends only on temperature

  • First law: ΔU = Q − W with W defined as work done by the gas

Quick reference

Elasticity and mechanical properties of materials

  • Stress = force/original area; strain = extension/original length.

  • Young modulus = stress/strain within the specified linear elastic range.

  • Specimen stiffness depends on length, area and material properties.

  • One square millimetre equals 10^-6 square metres.

  • Elastic spring energy is one half kx squared in the linear model.

  • Elastic recovery, proportional response, yielding and fracture are distinct ideas.

Quick reference

Oscillations, resonance and energy exchange

  • SHM requires a restoring acceleration proportional to minus displacement.

  • For an ideal mass-spring model, omega = sqrt(k/m) and T = 2pi sqrt(m/k).

  • Maximum speed is omega A and total energy is kA squared divided by two.

  • Pendulum period formula requires the small-angle approximation.

  • Damping removes oscillator energy; a periodic drive can supply energy.

  • An ideal LC circuit has omega = 1/sqrt(LC).

Quick reference

Practical and Experimental Skills

  • State resolution and uncertainty convention for each instrument

  • Random errors → repeats and means; systematic errors → correction

  • For first-order worst-case bounds, add relative contributions; independent standard uncertainties use quadrature

  • Gradient from two points on the best-fit line, with units

  • Average repeated timings and time many oscillations to cut reaction error

  • Never quote more significant figures than the data justify