Abitur Physics cheat sheet
Abitur Physics · Keep the key ideas within reach.
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
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
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
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
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
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