HKDSE Physics study materials
HKDSE Physics study resources

HKDSE Physics cheat sheet

HKDSE Physics · Keep the key ideas within reach.

Quick reference

Mechanics

  • Kinematic equations apply only for uniform acceleration: v = u + at, s = ut + ½at², v² = u² + 2as, s = ½(u + v)t.

  • Newton's second law is a vector relation: net force F = ma, so resolve forces into perpendicular components before applying it.

  • In a uniform gravitational field, weight W = mg and the centre of gravity coincides with the centre of mass for a uniform body.

  • Moment of a force about a point = F × perpendicular distance from the point to the line of action; for equilibrium, net moment about any point is zero.

  • Momentum p = mv is conserved in any collision or explosion with no net external force; kinetic energy is conserved only in elastic collisions.

  • Projectile motion: horizontal velocity stays constant while vertical motion has acceleration g downward; time of flight depends only on vertical displacement.

  • Circular motion requires a centripetal force of magnitude mv²/r directed toward the centre; the speed is constant but velocity changes.

  • Work done W = Fs cos θ and power P = W/t = Fv cos θ; gravitational potential energy change near Earth is mgh.

  • For a body in equilibrium under three non-parallel forces, the lines of action of the three forces must be concurrent.

Quick reference

Heat and Gases

  • Specific heat capacity c: energy = mcΔT; specific latent heat L: energy = mL, applied at constant temperature during a change of state.

  • Internal energy of an ideal gas depends only on its temperature; for a monatomic ideal gas, average kinetic energy per molecule = (3/2)kT.

  • Ideal gas law pV = nRT = NkT, with R = 8.31 J mol⁻¹ K⁻¹ and k = 1.38 × 10⁻²³ J K⁻¹; T must be in kelvin.

  • Boyle's law: pV = constant at constant temperature; pressure law: p/T = constant at constant volume; Charles's law: V/T = constant at constant pressure.

  • Pressure exerted by a gas arises from molecular collisions with the container walls; p = (1/3)ρ⟨c²⟩ for a gas of density ρ.

  • Conduction transfers energy by molecular vibration and free electrons without bulk movement of the material; metals conduct better than non-metals.

  • Convection requires bulk fluid movement driven by density differences; it cannot occur in solids.

  • Net rate of energy transfer by radiation depends on surface temperature and area; black surfaces are good absorbers and emitters, shiny surfaces poor.

  • At constant temperature, rate of evaporation depends on surface area, temperature, air movement and humidity, but not on the volume above the liquid once saturated.

Quick reference

Waves

  • Wave equation v = fλ; for a wave crossing a boundary, frequency stays constant while speed and wavelength change.

  • Transverse waves have displacement perpendicular to energy transfer (light, water surface); longitudinal waves have displacement parallel (sound).

  • Reflection: angle of incidence equals angle of reflection, measured from the normal; the image in a plane mirror is virtual, same size, laterally inverted.

  • Refraction obeys Snell's law n₁ sin θ₁ = n₂ sin θ₂; light bends toward the normal when entering a denser medium.

  • Total internal reflection occurs only when light travels from a denser to a less dense medium and the angle of incidence exceeds the critical angle, sin C = 1/n.

  • For a thin converging lens, 1/f = 1/u + 1/v with real-is-positive convention; magnification m = v/u.

  • Diffraction is most noticeable when the slit width is comparable to or smaller than the wavelength.

  • For two-source interference, constructive interference occurs where path difference = mλ and destructive where it is (m + ½)λ.

  • In a stationary wave, adjacent nodes are separated by λ/2, and the distance between a node and the next antinode is λ/4.

Quick reference

Electricity and Magnetism

  • Ohm's law V = IR holds for ohmic conductors at constant temperature; resistance R = ρL/A depends on material, length and cross-sectional area.

  • For resistors in series, R = R₁ + R₂ + …; in parallel, 1/R = 1/R₁ + 1/R₂ + …; voltage divides in series and current divides in parallel.

  • Electrical power P = VI = I²R = V²/R; energy consumed = Pt, billed in kilowatt-hours.

  • Kirchhoff's laws: at a junction, sum of currents in equals sum out; around any closed loop, sum of potential differences is zero.

  • Ammeters are connected in series and have low resistance; voltmeters are connected in parallel and have high resistance.

  • Coulomb's law: force between point charges F = kQ₁Q₂/r², attractive for opposite signs and repulsive for like signs.

  • Magnetic flux density B is measured in tesla; a straight wire carrying current I in a field B experiences force F = BIL sin θ.

  • A charged particle moving perpendicular to a magnetic field follows a circular path of radius r = mv/(qB).

  • Electromagnetic induction: induced e.m.f. equals the rate of change of magnetic flux linkage, ε = −N ΔΦ/Δt (Faraday's law).

Quick reference

Radioactivity and Nuclear Energy

  • Alpha decay emits a helium nucleus (⁴₂He): mass number decreases by 4 and atomic number by 2.

  • Beta-minus decay converts a neutron into a proton, emitting an electron and an antineutrino: atomic number increases by 1, mass number unchanged.

  • Gamma emission is a photon released from an excited nucleus; mass number and atomic number are unchanged.

  • Radioactive decay is random and spontaneous; the number of undecayed nuclei follows N = N₀e^(−λt), and activity A = λN.

  • Half-life t½ = ln 2/λ ≈ 0.693/λ; after n half-lives the remaining fraction is (1/2)ⁿ.

  • Alpha particles are the most ionising but least penetrating; gamma radiation is the least ionising but most penetrating.

  • Mass defect in a nucleus is converted to binding energy by E = mc²; binding energy per nucleon peaks near iron-56.

  • Nuclear fission splits a heavy nucleus and releases energy; nuclear fusion joins light nuclei and powers stars.

  • Background radiation comes from cosmic rays, radon gas, rocks and medical sources; it must be subtracted when measuring a source's count rate.