Sachsen-Anhalt Abitur Physics cheat sheet
Sachsen-Anhalt Abitur Physics · Keep the key ideas within reach.
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
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
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
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).
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
Relatividad: tiempo, longitud y energía
γ = 1/√(1 − v²/c²) ≥ 1.
Dilatación temporal: Δt = γ·Δt₀; contracción: L = L₀/γ.
p = γmv y E = γmc²; E_k = (γ − 1)mc².
E² = p²c² + m²c⁴; para el fotón E = pc.
El tiempo propio se mide en el sistema donde los sucesos ocurren en el mismo lugar.
Campo gravitatorio: campo, potencial y órbitas
F = G·M·m/r² y g = G·M/r²; el campo apunta hacia la masa que lo crea.
V = −G·M/r y E_p = −G·M·m/r, con referencia cero en el infinito.
Órbita circular: v = √(G·M/r) y T² = 4π²·r³/(G·M).
Energía mecánica de una órbita circular: E = −G·M·m/(2r).
La velocidad de escape cumple v_e = √(2G·M/R).
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
Climate physics: radiation, energy balance and feedback
Define whether the boundary is the surface or top of the atmosphere.
Absorbed solar flux equals (1 - albedo) times mean incident solar flux.
A spherical planet introduces a disk-to-surface geometric factor of four.
Positive net incoming flux means energy accumulates in the system.
Blackbody emission scales as absolute temperature to the fourth power.
Greenhouse absorption, albedo and heat transport affect different parts of the budget.