NSSCAS Physics (8225) study materials
NSSCAS Physics (8225) study resources

NSSCAS Physics (8225) cheat sheet

NSSCAS Physics (8225) · Keep the key ideas within reach.

Quick reference

Mechanics and kinematics

  • Average velocity = displacement / time; average speed = distance / time. Both are scalars except velocity, which is a vector.

  • Equations for uniform acceleration: v = u + at; s = ut + ½at²; v² = u² + 2as; s = ½(u + v)t.

  • Projectile motion: horizontal component of velocity is constant (if air resistance negligible); vertical acceleration is g downward.

  • For projectile launched at speed u and angle θ: time of flight = 2u sinθ / g (to same level); range = u² sin2θ / g.

  • Displacement–time graph gradient = velocity; velocity–time graph gradient = acceleration; area under velocity–time graph = displacement.

  • Relative velocity: v_AB = v_A − v_B (vector subtraction).

  • Angular velocity ω = 2π/T = 2πf; linear speed v = rω for circular motion.

  • Centripetal acceleration a = v²/r = rω² directed toward centre; centripetal force F = mv²/r.

Quick reference

Forces, momentum and Newtonian mechanics

  • Newton's first law: a body remains at rest or in uniform motion unless acted on by a resultant force.

  • Newton's second law: resultant force F = ma (or F = dp/dt).

  • Newton's third law: if A exerts a force on B, B exerts an equal and opposite force on A; forces act on different bodies.

  • Momentum p = mv (vector). Impulse = change in momentum = FΔt (area under force–time graph).

  • Conservation of linear momentum: total momentum of an isolated system remains constant.

  • Friction: limiting static friction F_max = μ_s N; kinetic friction F_k = μ_k N.

  • Moments: moment = force × perpendicular distance from pivot; principle of moments for equilibrium: sum of clockwise moments = sum of anticlockwise moments.

  • Centre of gravity: point where weight of body may be considered to act; for uniform regular shapes it is at the geometric centre.

Quick reference

Work, energy and power

  • Work done by a constant force: W = Fs cosθ, where θ is angle between force and displacement.

  • Kinetic energy KE = ½mv²; gravitational potential energy change ΔPE = mgΔh (near Earth's surface).

  • Elastic potential energy stored in a spring = ½kx² (or area under force–extension graph).

  • Work–energy theorem: net work done on an object equals its change in kinetic energy.

  • Conservation of energy: energy cannot be created or destroyed, only transferred between forms; total energy in a closed system is constant.

  • Power P = work done / time = energy transferred / time; average power P = Fv for constant force.

  • Efficiency = useful energy output / total energy input × 100% (or useful power output / total power input × 100%).

Quick reference

Materials and properties of matter

  • Density ρ = m/V; relative density = density of substance / density of water.

  • Hooke's law: extension is directly proportional to applied force up to the limit of proportionality: F = kx.

  • Stress = force / cross-sectional area (σ = F/A); strain = extension / original length (ε = x/L).

  • Young modulus E = stress / strain = (F/A) / (x/L) = FL/(Ax) for a wire.

  • Elastic deformation: material returns to original shape when force removed; plastic deformation: permanent change.

  • Ultimate tensile strength is the maximum stress a material can withstand before breaking.

  • Pressure in a fluid: p = F/A; pressure at depth h in a fluid of density ρ: p = p₀ + ρgh.

  • Archimedes' principle: upthrust on a body in a fluid equals the weight of fluid displaced.

Quick reference

Waves, sound and optics

  • Wave equation: v = fλ, where v is wave speed, f frequency, λ wavelength.

  • Transverse waves: oscillations perpendicular to direction of energy transfer (e.g., light). Longitudinal waves: oscillations parallel to direction of energy transfer (e.g., sound).

  • Refraction: n₁ sinθ₁ = n₂ sinθ₂ (Snell's law); refractive index n = c/v = sin i / sin r for light entering medium from vacuum/air.

  • Total internal reflection occurs when light travels from denser to less dense medium and angle of incidence exceeds critical angle C, where sin C = n₂/n₁.

  • Diffraction: spreading of waves when they pass through a gap or around an obstacle; significant when gap width ≈ wavelength.

  • Two-source interference: constructive interference when path difference = nλ; destructive when path difference = (n + ½)λ.

  • For double-slit interference: fringe spacing Δy = λD/d, where D is slit-to-screen distance and d is slit separation.

  • Sound intensity level β = 10 log₁₀(I/I₀) dB, with I₀ = 1 × 10⁻¹² W m⁻².

Quick reference

Electricity and DC circuits

  • Electric current I = ΔQ/Δt; conventional current direction is opposite to electron flow.

  • Ohm's law: V = IR for a conductor at constant temperature; resistance R = V/I.

  • Resistivity ρ: R = ρL/A; resistance increases with length and decreases with cross-sectional area.

  • Resistors in series: R_total = R₁ + R₂ + …; in parallel: 1/R_total = 1/R₁ + 1/R₂ + …

  • Electrical power P = VI = I²R = V²/R.

  • Kirchhoff's laws: junction rule (sum of currents entering = sum leaving); loop rule (sum of e.m.f.s = sum of p.d.s around any closed loop).

  • E.m.f. ε and internal resistance r: terminal p.d. V = ε − Ir; power output = Iε − I²r.

  • Potential divider: V_out = V_in × R₂/(R₁ + R₂) for two resistors in series.

Quick reference

Fields, electromagnetism and induction

  • Gravitational field strength g = F/m; for a point mass g = GM/r²; gravitational potential energy U = −GMm/r.

  • Newton's law of gravitation: F = Gm₁m₂/r².

  • Electric field strength E = F/q; for a point charge E = kQ/r² (k = 1/(4πε₀)); electric potential V = kQ/r.

  • Coulomb's law: F = kQ₁Q₂/r².

  • Magnetic flux density B: force on current-carrying conductor F = BIL sinθ; force on moving charge F = Bqv sinθ.

  • Magnetic flux Φ = BA cosθ; Faraday's law: induced e.m.f. ε = −dΦ/dt; Lenz's law: induced current opposes change in flux.

  • Transformer equation: V_s/V_p = N_s/N_p (ideal transformer); power input = power output for ideal transformer.

  • Motion of charged particle in uniform magnetic field: circular path with radius r = mv/(Bq).

Quick reference

Thermal physics

  • Temperature is a measure of average kinetic energy of particles; absolute zero = −273.15 °C = 0 K.

  • Specific heat capacity c: energy Q = mcΔT.

  • Specific latent heat L: energy Q = mL (for change of state at constant temperature).

  • Ideal gas equation: pV = nRT, where R = 8.31 J mol⁻¹ K⁻¹; also pV = NkT with k = 1.38 × 10⁻²³ J K⁻¹.

  • Kinetic theory: average kinetic energy of gas molecules = (3/2)kT; root-mean-square speed v_rms = √(3kT/m) = √(3RT/M).

  • First law of thermodynamics: ΔU = Q − W, where Q is heat added to system and W is work done by system.

  • Thermal conduction: rate of heat transfer P = kAΔT/L (k = thermal conductivity).

  • Boyle's law: p ∝ 1/V at constant T; Charles's law: V ∝ T at constant p; pressure law: p ∝ T at constant V.

Quick reference

Practical skills and experimental methods

  • Precision: closeness of repeated measurements to each other; accuracy: closeness to true value.

  • Random errors affect precision and can be reduced by repeating measurements and averaging; systematic errors affect accuracy and cannot be reduced by averaging.

  • Uncertainty: for a single reading, use ± half the smallest division; for digital instruments, ± the last digit.

  • Combining uncertainties: for addition/subtraction, add absolute uncertainties; for multiplication/division, add percentage uncertainties.

  • Percentage uncertainty = (absolute uncertainty / measured value) × 100%.

  • Graph plotting: plot independent variable on x-axis and dependent variable on y-axis; draw line of best fit; gradient = Δy/Δx.

  • Determining uncertainty in gradient: use maximum and minimum gradient lines from error bars or extreme points.

  • Significant figures: final answer should have same number of significant figures as the least precise measurement used in calculation.