Bremen Abitur Physik study materials
Bremen Abitur Physik study resources

Bremen Abitur Physik cheat sheet

Bremen Abitur Physik · 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

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

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