Extremadura PAU Physics study materials
Extremadura PAU Physics study resources

Extremadura PAU Physics cheat sheet

Extremadura PAU Physics · Keep the key ideas within reach.

Quick reference

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).

Quick reference

Campo electromagnético: electrostática, magnetismo e inducción

  • F = k·q₁·q₂/r²; E = F/q y V = k·q/r.

  • E_p = q·V; las líneas de campo son perpendiculares a las equipotenciales.

  • F = q·v×B no realiza trabajo; con v perpendicular a B y modelo no relativista, r = m·v/(|q|B) y T = 2πm/(|q|B).

  • Φ = B·S·cos θ y ε = −N·dΦ/dt (Ley de Faraday-Lenz).

  • 1 T = 1 Wb/m² = 1 N/(A·m).

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

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.

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