Abitur Physics study materials
Abitur Physics study resources

Abitur Physics cheat sheet

Abitur Physics · Keep the key ideas within reach.

Quick reference

Electricity and Magnetism

  • EMF is per unit charge from the source; terminal p.d. is E − Ir

  • Kirchhoff's laws follow from conservation of charge and energy

  • Capacitor energy is ½CV²; discharge is exponential with time constant RC

  • Magnetic-force magnitude is |q|vB sinθ and its vector is perpendicular to velocity, so magnetic force does no work

  • Lenz's law: induced effects oppose the change that causes them

  • RMS values: I₀/√2 and V₀/√2 for sinusoidal quantities

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

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

Modern Physics

  • hf = φ + KEmax; intensity affects rate, not maximum energy

  • Threshold frequency f₀ = φ/h in the ordinary single-photon model; below it that model predicts no photoemission

  • hf = E₂ − E₁ explains line spectra

  • λ = h/p generally; p = mv for a nonrelativistic massive particle

  • α: A−4, Z−2; β⁻: Z+1; γ: no change in A or Z

  • N = N₀e^(−λt) with t½ = ln2/λ; 1 u c² is approximately 931.5 MeV

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

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