Pancyprian Technical School Physics (4-hour) study materials
Pancyprian Technical School Physics (4-hour) study resources

Pancyprian Technical School Physics (4-hour) cheat sheet

Pancyprian Technical School Physics (4-hour) · Keep the key ideas within reach.

Quick reference

Mechanics: Kinematics and Dynamics

  • Uniformly accelerated motion: v = u + at, s = ut + ½at², v² = u² + 2as; valid only for constant acceleration in a straight line.

  • Projectile motion separates into independent horizontal (constant velocity) and vertical (acceleration g) components; time of flight from vertical motion alone.

  • Newton's second law as a vector equation: ΣF = ma; resolve forces into perpendicular components before summing.

  • Friction: limiting static friction f ≤ μsN; kinetic friction f = μkN, acting opposite to relative sliding.

  • Inclined plane without friction: a = g sinθ; with friction on the way up a = g(sinθ + μcosθ).

  • Momentum form of Newton's second law: F = Δp/Δt, which remains valid when mass changes (rockets, chains).

  • Equilibrium of a rigid body requires both ΣF = 0 and Στ = 0 about any chosen axis; choose the axis to eliminate unknown forces.

  • For connected bodies over a pulley, apply ΣF = ma to each mass separately and equate the common tension/acceleration.

Quick reference

Work, Energy, Power and Momentum

  • Work done by a constant force: W = Fs cosθ, where θ is the angle between force and displacement; perpendicular forces do no work.

  • Work–energy theorem: W_net = ΔKE = ½mv² − ½mu², including work by friction and gravity.

  • Conservative forces (gravity, spring, electrostatic) have potential energy; friction is non-conservative and dissipates mechanical energy.

  • Power: P = W/t = Fv cosθ; average versus instantaneous power differ when speed varies.

  • Conservation of linear momentum applies when net external force is zero, e.g. collisions and explosions; kinetic energy is conserved only in elastic collisions.

  • Perfectly inelastic collision: bodies stick, common velocity v = (m₁u₁ + m₂u₂)/(m₁ + m₂); lost KE = ½m₁u₁² + ½m₂u₂² − ½(m₁+m₂)v².

  • Impulse J = FΔt = Δp; the area under a force–time graph equals impulse.

  • Efficiency = useful output energy / total input energy × 100%; losses usually appear as thermal energy.

Quick reference

Circular Motion

  • Angular speed ω = 2π/T = 2πf; linear speed v = ωr; centripetal acceleration a = v²/r = ω²r directed toward the centre.

  • Centripetal force is a net resultant, not an extra force: F = mv²/r supplied by tension, friction, gravity, or normal force.

  • Vertical circle: at the top mg + N = mv²/r; at the bottom N − mg = mv²/r; minimum speed at top for a string is v = √(gr).

  • Banked track without friction: tanθ = v²/(rg); with friction the safe speed range widens.

  • Conical pendulum: T cosθ = mg and T sinθ = mv²/r, giving tanθ = v²/(rg).

  • Angular displacement in radians: θ = s/r; tangential acceleration a_t = rα changes speed while centripetal acceleration changes direction.

  • Centripetal force does no work because it is always perpendicular to velocity, so speed and kinetic energy stay constant in uniform circular motion.

Quick reference

Oscillations and Gravitation

  • SHM defining condition: a = −ω²x, with displacement measured from equilibrium; ω = 2π/T.

  • SHM solutions: x = A sin(ωt + φ), v = ωA cos(ωt + φ), maximum speed v_max = ωA, maximum acceleration a_max = ω²A.

  • Mass–spring: T = 2π√(m/k), independent of amplitude and of g.

  • Simple pendulum: T = 2π√(l/g) for small angles (typically θ < 10°); T is independent of bob mass.

  • Energy in SHM: total E = ½kA² = ½mω²A²; KE and PE interchange, with KE maximum at equilibrium.

  • Newton's law of gravitation: F = Gm₁m₂/r², G = 6.67 × 10⁻¹¹ N·m²/kg²; field strength g = GM/r² outside a spherical mass.

  • Orbital speed v = √(GM/r); period T = 2π√(r³/GM), so T² ∝ r³ (Kepler's third law).

  • Escape speed from a body of mass M and radius R: v = √(2GM/R); for Earth it is about 11.2 km/s.

Quick reference

Fluid Mechanics and Properties of Matter

  • Pressure p = F/A; in a liquid p = p₀ + ρgh, and pressure depends only on depth, not on container shape.

  • Archimedes' principle: upthrust = weight of displaced fluid = ρ_fluid V_submerged g; floating body displaces its own weight.

  • Continuity equation for incompressible flow: A₁v₁ = A₂v₂.

  • Bernoulli's equation: p + ½ρv² + ρgh = constant along a streamline for steady, non-viscous, incompressible flow.

  • Viscous drag on a sphere at low speed (Stokes' law): F = 6πηrv; terminal velocity when 6πηrv = (ρ_sphere − ρ_fluid)Vg.

  • Hooke's law: stress ∝ strain within the elastic limit; Young's modulus E = (F/A)/(Δl/l).

  • Stress = force/cross-sectional area (Pa); strain is dimensionless; the area under a stress–strain curve up to fracture is toughness.

  • Density ρ = m/V; relative density compares a substance to water; specific heat and latent heat are intensive properties.

Quick reference

Thermal Physics: Heat, Temperature and Gas Laws

  • Temperature conversion: T(K) = θ(°C) + 273.15; absolute zero is 0 K = −273.15 °C.

  • Linear expansion: ΔL = αL₀Δθ; area and volume expansions use 2α and 3α for isotropic solids.

  • Heat transfer: Q = mcΔθ for temperature change; Q = mL at a phase change with no temperature change.

  • Ideal gas law: pV = nRT with R = 8.31 J/(mol·K); alternatively pV = NkT with k = 1.38 × 10⁻²³ J/K.

  • Combined gas law for a fixed mass: p₁V₁/T₁ = p₂V₂/T₂; isothermal pV = constant, isobaric V/T = constant, isochoric p/T = constant.

  • Kinetic theory: average translational KE per molecule = (3/2)kT, so internal energy of an ideal gas depends only on temperature.

  • First law of thermodynamics: ΔU = Q − W, where W is work done by the gas; W = pΔV at constant pressure.

  • Absolute humidity is vapour mass per unit volume; relative humidity = partial vapour pressure / saturated vapour pressure × 100%.

Quick reference

Electrostatics and Direct Current Circuits

  • Coulomb's law: F = kQ₁Q₂/r² with k = 1/(4πε₀) ≈ 9 × 10⁹ N·m²/C²; force is along the line joining the charges, attractive for unlike signs.

  • Uniform field between parallel plates: E = V/d; force on charge q is F = qE; work done moving q through V is qV.

  • Electric potential V = kQ/r; potential is a scalar, field is a vector pointing from high to low potential.

  • Capacitance C = Q/V; parallel plates C = ε₀ε_rA/d; energy stored = ½QV = ½CV².

  • Ohm's law V = IR applies to ohmic conductors at constant temperature; resistance of a wire R = ρl/A.

  • Series: R = R₁ + R₂ + …, same current; parallel: 1/R = 1/R₁ + 1/R₂ + …, same voltage.

  • Electrical power: P = VI = I²R = V²/R; energy in kWh = power(kW) × time(h).

  • Kirchhoff's rules: junction rule (charge conservation) ΣI_in = ΣI_out; loop rule (energy conservation) ΣEMF = ΣIR around any closed loop.

  • EMF and internal resistance: terminal voltage V = ε − Ir; maximum power transfer to load when R = r.

Quick reference

Magnetism and Electromagnetic Induction

  • Force on a current-carrying conductor: F = BIl sinθ, direction by Fleming's left-hand rule; maximum when conductor is perpendicular to B.

  • Force on a moving charge: F = qvB sinθ; it is always perpendicular to velocity, so magnetic force does no work and cannot change speed.

  • Radius of a charged particle's circular path in a magnetic field: r = mv/(qB); period T = 2πm/(qB) is independent of speed.

  • Magnetic flux Φ = BA cosθ; flux is measured in webers (Wb), flux density B in tesla (T).

  • Faraday's law: induced EMF ε = −N dΦ/dt; the magnitude depends on rate of change of flux linkage, not on flux itself.

  • Lenz's law: induced current opposes the change producing it; this is a statement of energy conservation.

  • Straight conductor moving through a field: motional EMF ε = Blv (when B, l, v are mutually perpendicular).

  • Transformer (ideal): V_s/V_p = N_s/N_p = I_p/I_s; a step-up voltage transformer steps current down.

Quick reference

Waves, Sound and Geometric Optics

  • Wave equation: v = fλ; for a stretched string v = √(T/μ) with μ = mass per unit length.

  • Speed of sound in air ≈ 340 m/s at room temperature and rises with temperature; sound needs a material medium.

  • Sound intensity level β = 10 log₁₀(I/I₀) dB with I₀ = 1 × 10⁻¹² W/m²; doubling intensity adds about 3 dB.

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

  • String and pipe modes: string fixed both ends f_n = nv/(2L); open pipe f_n = nv/(2L); pipe closed at one end gives odd harmonics only, f_n = nv/(4L), n odd.

  • Snell's law: n₁ sinθ₁ = n₂ sinθ₂; refractive index n = c/v; total internal reflection requires travel from denser to less dense medium and θ > critical angle sinθ_c = n₂/n₁.

  • Thin lens/mirror equation: 1/f = 1/v + 1/u with sign convention stated explicitly; magnification m = v/u (or −v/u depending on convention).

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

Quick reference

Modern Physics: Atomic, Nuclear and Quantum Phenomena

  • Photon energy E = hf = hc/λ; h = 6.63 × 10⁻³⁴ J·s; 1 eV = 1.60 × 10⁻¹⁹ J.

  • Photoelectric equation: hf = W + KE_max, with threshold frequency f₀ = W/h; maximum KE depends on frequency, not intensity.

  • Stopping potential: eV_s = KE_max; the photocurrent saturates with intensity at fixed frequency.

  • Hydrogen energy levels: E_n = −13.6/n² eV; photon energy for a transition = E_high − E_low.

  • de Broglie wavelength λ = h/p = h/(mv); electron diffraction confirms wave behaviour of matter.

  • Radioactive decay N = N₀e^(−λt); half-life T½ = ln2/λ = 0.693/λ; activity A = λN measured in becquerel.

  • Nuclear notation: mass number A = protons + neutrons; isotopes share Z but differ in N; alpha decay reduces A by 4 and Z by 2.

  • Mass–energy equivalence E = mc²; nuclear binding energy per nucleon peaks near iron-56, explaining fission of heavy and fusion of light nuclei.

Quick reference

Laboratory Practice, Measurement and Data Analysis

  • Absolute uncertainty of a single reading is typically half the smallest scale division; for a digital display use ±1 in the last digit.

  • Combining uncertainties: sums/differences add absolute uncertainties; products/quotients add percentage uncertainties; powers multiply percentage uncertainty by the exponent.

  • Report a result as value ± uncertainty with matching decimal places and an appropriate number of significant figures (usually 2–3).

  • Percentage difference from a stated value: |measured − accepted| / accepted × 100%.

  • Systematic errors shift all readings in one direction (zero error, calibration); random errors scatter and are reduced by averaging repeats.

  • Graph analysis: gradient of a straight-line graph gives the derived quantity; error bars show uncertainty and a line of best fit should pass through the bars.

  • Linearise a relationship before plotting, e.g. plot T² against l for a pendulum so that gradient = 4π²/g.

  • Precision describes repeatability of readings, accuracy describes closeness to the true value; a precise set can still be inaccurate.

Quick reference

Applications of Physics in Technology and Engineering

  • Electrical transmission at high voltage reduces I²R line losses for the same transmitted power P = VI.

  • Transformers enable efficient voltage change but work only with alternating current, since they rely on changing flux.

  • Internal combustion engine efficiency is limited by the Carnot bound η ≤ 1 − T_cold/T_hot; real engines fall well below it.

  • Hydraulic systems transmit force via Pascal's principle: F₁/A₁ = F₂/A₂, giving mechanical advantage from area ratio.

  • Heat pumps and refrigerators move heat against the temperature gradient and require work input; coefficient of performance = Q_desired/W.

  • Sensors convert physical quantities to electrical signals: thermistors change resistance with temperature, LDRs with light, strain gauges with deformation.

  • Renewable generation: a wind turbine's available power scales as P ∝ A v³, so doubling wind speed multiplies available power by eight.

  • Structural design uses stress = F/A and compares it with the material's yield strength, applying a safety factor greater than one.

Quick reference

Greek-Style Exam Technique for Physics Calculations

  • Write the formula symbolically, substitute values with units, then give the numerical answer with the correct unit and significant figures.

  • Convert all data to SI before substitution: cm to m, g to kg, minutes to seconds, kW·h to J (1 kW·h = 3.6 × 10⁶ J).

  • Check dimensional consistency: both sides of any physical equation must have identical base units.

  • When a question asks to 'show that', derive the stated result explicitly and do not simply quote it.

  • For multi-step problems, label intermediate results and carry them forward unrounded; round only the final answer.

  • In graphs, state what the gradient and intercept represent physically, not just their numerical values.

  • If an answer seems unphysical (negative time, speed above c, efficiency over 100%), recheck the sign convention or unit conversion.

Quick reference

Reference Constants and Unit Conversions

  • g ≈ 9.81 m/s² near Earth's surface; gravitational constant G = 6.67 × 10⁻¹¹ N·m²/kg².

  • Elementary charge e = 1.60 × 10⁻¹⁹ C; electron mass 9.11 × 10⁻³¹ kg; proton mass 1.67 × 10⁻²⁷ kg.

  • Speed of light c = 3.00 × 10⁸ m/s; Planck constant h = 6.63 × 10⁻³⁴ J·s.

  • Avogadro constant N_A = 6.02 × 10²³ mol⁻¹; molar gas constant R = 8.31 J/(mol·K); Boltzmann constant k = 1.38 × 10⁻²³ J/K.

  • Specific heat capacity of water ≈ 4200 J/(kg·K); specific latent heat of fusion of ice ≈ 3.34 × 10⁵ J/kg.

  • Permittivity of free space ε₀ = 8.85 × 10⁻¹² F/m; Coulomb constant k ≈ 9.0 × 10⁹ N·m²/C².

  • Unit conversions: 1 N = 1 kg·m/s²; 1 J = 1 N·m; 1 W = 1 J/s; 1 Pa = 1 N/m²; 1 T = 1 Wb/m²; 1 V = 1 J/C.

  • Prefixes: nano 10⁻⁹, micro 10⁻⁶, milli 10⁻³, kilo 10³, mega 10⁶, giga 10⁹.