Balearic PAU Physics study materials
Balearic PAU Physics study resources

Balearic PAU Physics cheat sheet

Balearic PAU Physics · Keep the key ideas within reach.

Quick reference

Gravitational field

  • Newton's law: F = G·m₁·m₂/r², attractive, G = 6.67×10⁻¹¹ N·m²/kg²; direction along the line joining the masses.

  • Field strength g = F/m = G·M/r², a vector pointing toward the source mass; on Earth's surface g ≈ 9.8 m/s².

  • Uniform-field approximation g ≈ constant is valid only for height differences much smaller than the planet's radius.

  • Gravitational potential V = −G·M/r, always negative with V(∞) = 0; potential energy U = m·V = −G·M·m/r.

  • Work done by the field equals −ΔU; moving a mass along an equipotential surface requires zero work.

  • Escape velocity from a body of mass M and radius R: v_e = √(2GM/R), independent of the escaping mass.

  • Kepler's third law: T² = (4π²/GM)·r³ for circular orbits; orbital speed v = √(GM/r).

  • Satellites in circular orbit: total mechanical energy E = −GMm/(2r), so binding energy is positive and equal to half |U|.

Quick reference

Electromagnetic field

  • Coulomb's law: F = k·q₁·q₂/r², k = 1/(4πε₀) ≈ 9×10⁹ N·m²/C²; force is repulsive for like signs.

  • Electric field E = F/q (N/C or V/m); field lines start on positive and end on negative charge.

  • Potential V = k·q/r with V(∞) = 0; work by external agent to move charge q between points is q·ΔV.

  • Uniform field between parallel plates: E = V/d, directed from the positive to the negative plate.

  • Gauss's law: electric flux through a closed surface equals Q_enclosed/ε₀; use symmetry to choose the surface.

  • Magnetic force on a moving charge: F = q·v×B, magnitude qvB·sinθ; it does no work because F ⊥ v.

  • Force on a straight current wire: F = I·L×B; parallel currents attract, antiparallel currents repel.

  • Field of a long straight wire: B = μ₀·I/(2πr); inside a long solenoid B = μ₀·n·I.

  • Faraday–Lenz law: ε = −dΦ/dt with Φ = B·A·cosθ; the induced current opposes the change in flux.

Quick reference

Waves

  • Wave relation: v = λ·f = λ/T; the medium fixes v, and f is set by the source.

  • Simple harmonic motion: x = A·sin(ωt + φ), with ω = 2π/T = 2πf; maximum speed Aω, maximum acceleration Aω².

  • Mass–spring oscillator: ω = √(k/m), T = 2π√(m/k); simple pendulum: T = 2π√(L/g).

  • Mechanical waves need a material medium; electromagnetic waves propagate in vacuum at c = 3.00×10⁸ m/s.

  • Wave intensity is proportional to the square of the amplitude; for a point source in 3D, I ∝ 1/r².

  • Standing waves on a string fixed at both ends: λ_n = 2L/n, f_n = n·v/(2L), n = 1, 2, 3…

  • Doppler effect for sound: f' = f·(v ± v_o)/(v ∓ v_r), with signs chosen so approach raises the observed frequency.

  • Superposition: constructive interference when path difference = nλ, destructive when path difference = (n + ½)λ.

Quick reference

Optics

  • Snell's law: n₁·sinθ₁ = n₂·sinθ₂; refractive index n = c/v, so light slows in a denser medium.

  • Total internal reflection occurs only going from denser to less dense medium, when θ₁ exceeds θ_c with sinθ_c = n₂/n₁.

  • Thin lens and spherical mirror equation: 1/f = 1/s + 1/s'; magnification m = −s'/s (lens) or m = −s'/s with sign conventions stated.

  • Lens maker's equation: 1/f = (n − 1)·(1/R₁ − 1/R₂); converging lens f > 0, diverging lens f < 0.

  • Young's double slit: fringe spacing Δy = λ·D/d; maxima at d·sinθ = nλ, minima at d·sinθ = (n + ½)λ.

  • Single-slit diffraction minima: a·sinθ = nλ (n = 1, 2, …); central maximum is twice as wide as the secondary ones.

  • Diffraction grating: d·sinθ = nλ; smaller grating spacing d gives larger angular separation of orders.

  • Dispersion: n decreases with increasing wavelength, so violet refracts more than red in glass.

Quick reference

Relativity

  • Postulates: physical laws are identical in all inertial frames, and the speed of light in vacuum is c for every inertial observer.

  • Lorentz factor γ = 1/√(1 − v²/c²) ≥ 1; time dilation Δt = γ·Δτ for the proper time Δτ.

  • Length contraction L = L₀/γ applies only to the dimension parallel to the motion; proper length is measured in the rest frame.

  • Relativistic mass–energy: E = γ·m·c²; rest energy E₀ = m·c²; kinetic energy K = (γ − 1)·m·c².

  • Energy–momentum relation: E² = (p·c)² + (m·c²)²; for photons m = 0 and E = p·c = h·f.

  • Velocity addition: u = (u' + v)/(1 + u'·v/c²); the result never exceeds c.

  • Simultaneity is frame-dependent: events simultaneous in one inertial frame are generally not simultaneous in another.

  • For v ≤ 0.1c, γ ≈ 1 + v²/(2c²), so classical mechanics is a good approximation.

Quick reference

Quantum physics

  • Photon energy E = h·f = h·c/λ, with h = 6.63×10⁻³⁴ J·s; photon momentum p = h/λ.

  • Photoelectric effect: K_max = h·f − W₀, where W₀ is the work function; threshold frequency f₀ = W₀/h.

  • Stopping potential relation: e·V₀ = K_max; no emission occurs below the threshold frequency regardless of intensity.

  • de Broglie wavelength λ = h/p = h/(m·v); matter waves become measurable for electrons and lighter particles.

  • Bohr model: E_n = −13.6 eV/n² for hydrogen; transition photon energy h·f = E_f − E_i.

  • Bohr angular momentum quantization: L = n·h/(2π); orbit radius r_n = n²·a₀ with a₀ ≈ 0.053 nm.

  • Heisenberg uncertainty principle: Δx·Δp ≥ ħ/2, with ħ = h/(2π); it is a fundamental limit, not a measurement flaw.

  • Wave–particle duality: interference and diffraction reveal wave behaviour, while the photoelectric effect reveals particle behaviour.

Quick reference

Nuclear physics and radioactivity

  • Nuclear notation ᴬ_ZX: Z protons, A − Z neutrons; isotopes share Z but differ in A.

  • Mass defect and binding energy: ΔE = Δm·c²; 1 u = 931.5 MeV/c², so 1 u of defect releases 931.5 MeV.

  • Alpha decay: A decreases by 4, Z by 2; beta-minus decay: n → p + e⁻ + ν̄, so Z increases by 1.

  • Beta-plus decay and electron capture reduce Z by 1; gamma emission changes neither A nor Z.

  • Radioactive decay law: N = N₀·e^(−λt); activity A = λ·N; half-life T½ = ln2/λ ≈ 0.693/λ.

  • After n half-lives the remaining fraction is (1/2)^n; the activity follows the same exponential law.

  • Conservation laws in nuclear reactions: charge Z, nucleon number A, energy–mass and momentum are conserved.

  • Fission of heavy nuclei and fusion of light nuclei both release energy because the products are more tightly bound (higher binding energy per nucleon).