AQA A-Level Physics: Paper 1

7408/1  ·  2 hours  ·  85 marks  ·  34% of A-Level  ·  Sections 1 – 5

Section 1 - Measurements and their errors

1.1  SI units and standard form

All physical quantities have a numerical value and a unit. SI (Systeme International) base units underpin all derived units used in physics.

Metre (m)
Length
Kilogram (kg)
Mass
Second (s)
Time
Ampere (A)
Electric current
Kelvin (K)
Temperature
Mole (mol)
Amount of substance

Common prefixes:

PrefixSymbolMultiplier
TeraT1012
GigaG109
MegaM106
Kilok103
Centic10-2
Millim10-3
Microμ10-6
Nanon10-9
Picop10-12
Femtof10-15

Unit conversions to know:

J and eV
1 eV = 1.6 × 10-19 J. To convert eV → J: multiply by 1.6 × 10-19. To convert J → eV: divide by 1.6 × 10-19.
J and kWh
1 kWh = 3.6 × 106 J. Derived from: 1 kW × 3600 s = 1000 × 3600 = 3.6 × 106 J. To convert kWh → J: multiply by 3.6 × 106.

Unit checking (dimensional analysis) is a powerful tool: if both sides of an equation have the same base units, the equation is dimensionally consistent. Use it to check unfamiliar formulae.

1.2  Errors and uncertainties

Random error
Unpredictable variation around the true value. Causes scatter in repeated measurements. Reduced by taking many repeats and averaging. Cannot be eliminated entirely.
Systematic error
A consistent offset in the same direction for every measurement. Caused by instrument calibration errors, zero errors, or flawed method. Repeating measurements does not reduce it.
Precision
How close repeated measurements are to each other (low random error = high precision). A precise result has a small spread around its mean.
Accuracy
How close the measured value is to the true value (low systematic error = high accuracy). An accurate result may still have low precision if random errors are large.
Repeatability
A result is repeatable if the same experimenter using the same equipment in the same conditions obtains the same result on repeated attempts.
Reproducibility
A result is reproducible if different experimenters (or different equipment or methods) obtain the same result. A higher standard than repeatability.
Resolution
The smallest change in a quantity that an instrument can detect. A ruler with 1 mm markings has a resolution of 1 mm. Higher resolution instruments reduce reading uncertainty.
Absolute uncertainty
The uncertainty expressed in the same units as the measurement, e.g. 4.5 ± 0.1 cm. For a set of repeats: half the range of the data.
Percentage uncertainty
(Absolute uncertainty / Measured value) × 100%. Allows uncertainties in different quantities to be compared directly.

Combining uncertainties:

Addition / Subtraction: add absolute uncertainties e.g. if A = 5.0 ± 0.2 and B = 3.0 ± 0.1, then A + B = 8.0 ± 0.3 Multiplication / Division: add percentage uncertainties e.g. if %ΔA = 4% and %ΔB = 3%, then A × B has uncertainty 7% Powers: multiply percentage uncertainty by the power e.g. if %Δr = 2%, then r³ has uncertainty 6%

Error bars on graphs: each data point may be plotted with a vertical (and/or horizontal) error bar representing the uncertainty in that measurement. The bar extends by ±(absolute uncertainty) above and below the point.

Uncertainties in gradient and intercept of a best-fit straight line:

  1. Draw the line of best fit through the data points
  2. Draw the steepest and shallowest lines that still pass through all error bars
  3. Uncertainty in gradient = ½(max gradient − min gradient)
  4. Uncertainty in intercept = ½(max intercept − min intercept)

In practicals, the instrument with the largest percentage uncertainty dominates the overall result. Always calculate the percentage uncertainty for each measurement before deciding where to focus precision improvements.

1.3  Estimation of physical quantities

Being able to estimate the order of magnitude of physical quantities is an important skill. Use known values as anchors and reason from them.

Height of a person
~1.7 m
Mass of a car
~1000 kg (103 kg)
Diameter of an atom
~10-10 m
Diameter of a nucleus
~10-15 m (femtometres)
Speed of sound in air
~340 m s-1
Speed of light
~3 × 108 m s-1

Estimation questions award marks for a valid method and a reasonable order of magnitude, not an exact answer. Show your working and justify any assumed values.

Section 2 - Particles and radiation

2.1.1  Constituents of the atom

ParticleRelative massRelative chargeMass (SI)Charge (SI)
Proton1+11.673 × 10-27 kg+1.6 × 10-19 C
Neutron101.675 × 10-27 kg0
Electron1/1836−19.11 × 10-31 kg−1.6 × 10-19 C
Specific charge = charge / mass (units: C kg-1) Proton: specific charge = 1.6×10-19 / 1.673×10-27 ≈ 9.6 × 107 C kg-1 Electron: specific charge ≈ 1.76 × 1011 C kg-1 (much larger due to very small mass)

An atom is described as AZX where A = mass number (protons + neutrons) and Z = atomic number (protons only). Isotopes have the same Z but different A (same element, different number of neutrons).

The electron has a much higher specific charge than the proton because it has the same magnitude of charge but ~1836 times less mass. This is a commonly examined comparison.

2.1.2  Stable and unstable nuclei

The strong nuclear force holds the nucleus together against the electrostatic repulsion between protons. It acts between all nucleons (proton-proton, neutron-neutron, proton-neutron).

Strong nuclear force properties
Range: up to ~3 fm. Attractive up to ~3 fm; repulsive below ~0.5 fm (prevents nucleons collapsing). Acts equally on protons and neutrons (charge-independent).
Nuclear stability
Stable nuclei have a balance of protons and neutrons. For small nuclei (Z ≤ 20) the ratio N/Z ≈ 1. For larger nuclei, extra neutrons are needed to provide sufficient strong force without adding to electrostatic repulsion.

Radioactive decay modes:

Alpha (α) decay
Emits 42He nucleus. A decreases by 4; Z decreases by 2. Occurs in heavy nuclei (typically A > 200, Z > 82) where the nucleus is too large for the strong force to maintain stability.
Beta-minus (β-) decay
Neutron → proton + electron + antineutrino. A unchanged; Z increases by 1. Occurs in nuclei with too many neutrons.
Beta-plus (β+) decay
Proton → neutron + positron + neutrino. A unchanged; Z decreases by 1. Occurs in nuclei with too many protons.

Always check that both mass number and atomic number are conserved in a nuclear equation. Neutrinos and antineutrinos carry away energy and momentum but have negligible mass and no charge.

2.1.3  Particles, antiparticles and photons

Every particle has a corresponding antiparticle with the same mass but opposite charge (and opposite quantum numbers).

ParticleAntiparticleChargeRest energy (MeV)
Electron (e-)Positron (e+)+10.511
Proton (p)Antiproton (p̄)−1938.3
Neutron (n)Antineutron (n̄)0939.6
Neutrino (νe)Antineutrino (ν̄e)0≈0

Particle and antiparticle have identical rest mass (and rest energy); they differ in charge and all other quantum numbers (baryon number, lepton number, strangeness).

Pair production
A photon of sufficient energy spontaneously creates a particle-antiparticle pair. Energy of photon must be ≥ 2m0c². Occurs near a nucleus (to conserve momentum).
Annihilation
A particle and its antiparticle collide and are converted into two photons moving in opposite directions (to conserve momentum). Each photon has energy ≥ m0c² (equals m0c² when the pair annihilate at rest).
Photon energy: E = hf = hc/λ h = 6.63 × 10-34 J s (Planck's constant) c = 3.00 × 108 m s-1 Minimum photon energy for pair production: E ≥ 2m0c² For electron-positron pair: E ≥ 2 × 9.11×10-31 × (3×108)² ≈ 1.64 × 10-13 J

Pair production and annihilation are direct applications of E = mc². In annihilation, two photons are produced (not one) to conserve momentum.

2.1.4 – 2.1.6  Particle interactions, classification and quarks

Four fundamental forces and their exchange particles (2.1.4):

ForceExchange particleActs onRange
Strong nuclearGluons (pions at nuclear level)Quarks / hadrons~10-15 m
ElectromagneticVirtual photon (γ)Charged particlesInfinite
Weak nuclearW+, W- bosonsAll quarks and leptons~10-18 m
GravityGraviton (theoretical)All particles with massInfinite

Feynman diagrams represent particle interactions using exchange particles. Key interactions to know:

β decay (weak)
A down quark emits a W boson and becomes an up quark. The W decays to an electron + electron antineutrino. Net: n → p + e + ν¯e.
β+ decay (weak)
An up quark emits a W+ boson and becomes a down quark. The W+ decays to a positron + electron neutrino. Net: p → n + e+ + νe.
Electron capture (weak)
An up quark in the proton emits a W+ boson and becomes a down quark. The W+ is absorbed by the orbital electron, converting it into an electron neutrino. Net: p + e → n + νe.
Electron–proton collision (weak)
An electron and proton interact via W+ exchange: e + p → n + νe. Same result as electron capture but occurs via collision rather than orbital absorption.

Particle classification (2.1.5):

Hadrons
Composed of quarks. Experience the strong nuclear force. Two sub-types: Baryons (3 quarks: proton, neutron, their antiparticles; B = +1 or −1) and Mesons (quark + antiquark: pions, kaons; B = 0). The proton is the only stable baryon.
Leptons
Fundamental particles, not made of quarks. Do not experience the strong force. Four types (+antiparticles): electron (e), muon (μ), electron neutrino (νe), muon neutrino (νμ). Baryon number B = 0.

Strange particles: particles that are produced through the strong interaction but decay through the weak interaction (e.g. kaons). This accounts for why they are produced rapidly but decay relatively slowly. Strange particles are always created in pairs (strangeness is conserved in production). Strangeness (symbol S) is a quantum number: S = +1 for the K+ kaon (us̄); S = −1 for the K antikaon (ūs).

  • Strong and EM interactions: strangeness is conserved (total strangeness before = total after)
  • Weak interactions: strangeness can change by 0, +1 or −1 (hence strange particles can decay into non-strange particles via the weak interaction)

Quarks (2.1.6):

QuarkSymbolChargeBaryon numberStrangeness
Upu+2/3 e+1/30
Downd−1/3 e+1/30
Stranges−1/3 e+1/3−1
Anti-up−2/3 e−1/30
Anti-down+1/3 e−1/30
Anti-strange+1/3 e−1/3+1
Proton = uud charge: 2/3 + 2/3 − 1/3 = +1 Neutron = udd charge: 2/3 − 1/3 − 1/3 = 0 π+ (pion) = ud̄ (meson) strangeness: 0 K+ (kaon) = us̄ (strange meson) strangeness: +1 Quark changes in beta decay (weak interaction): β decay: d → u + W (W → e + ν̄e) β+ decay: u → d + W+ (W+ → e+ + νe) Electron capture: u + e → d + νe (via W+)

Conservation laws in particle interactions:

  • Charge: always conserved
  • Baryon number (B): always conserved. Quarks have B = +1/3; antiquarks B = −1/3; proton/neutron B = +1.
  • Lepton numbers, conserved separately:
    • Electron lepton number (Le): e and νe have Le = +1; e+ and ν̄e have Le = −1
    • Muon lepton number (Lμ): μ and νμ have Lμ = +1; μ+ and ν̄μ have Lμ = −1
  • Strangeness: conserved in strong and EM interactions; can change by ±1 in weak interactions (hence strange particles decay weakly)

Le and Lμ are conserved separately: check each independently. A reaction producing e must also produce ν̄e (not ν̄μ). In β decay the antineutrino is an electron antineutrino (ν̄e), not a muon antineutrino. This is a frequent exam trap.

2.2.1  The photoelectric effect

When electromagnetic radiation above a threshold frequency strikes a metal surface, electrons are emitted. This cannot be explained by wave theory - it provides evidence for the photon model of light.

Threshold frequency (f0)
The minimum frequency of radiation that will cause photoelectric emission from a given metal surface. Below this frequency, no electrons are emitted regardless of intensity.
Work function (φ)
The minimum energy needed to liberate one electron from the metal surface. φ = hf0. Different metals have different work functions.
Einstein's photoelectric equation: hf = φ + ½mv²max where: hf = energy of incident photon φ = work function of the metal ½mv²max = maximum kinetic energy of emitted electron Stopping potential Vs: eVs = ½mv²max

Key observations that wave theory cannot explain: (1) instantaneous emission - no time delay; (2) threshold frequency - below it, no emission regardless of intensity; (3) maximum KE depends on frequency, not intensity. Each one-to-one photon-electron interaction explains all three.

2.2.2 – 2.2.4  Electron collisions, energy levels, spectra and wave-particle duality

Excitation by electron collision (2.2.2): a free electron collides with an atom and transfers energy to a bound electron, raising it to a higher energy level. Unlike photon absorption, the colliding electron does not need to supply exactly the right energy; it simply loses some of its kinetic energy. The atom then de-excites by emitting a photon of energy E = hf = Eupper − Elower.

Excitation by collision
Colliding electron transfers any amount of KE ≥ the energy gap to the atom. The atom moves to a higher energy level. The colliding electron continues with less KE. No energy is radiated during the collision itself.
Fluorescent tubes
Electric discharge accelerates electrons through mercury vapour → electrons collide with Hg atoms → Hg atoms excite and emit UV photons on de-excitation → UV absorbed by phosphor coating on the tube → phosphor re-emits visible light. More efficient than filament lamps.

Energy levels in atoms (2.2.3): electrons occupy discrete energy levels. Ground state is the lowest energy level (most negative). Energy is quantised; electrons can only have specific energies.

Photon emitted when electron drops between levels: E = hf = E1 - E2 (where E1 is higher level, E2 lower) Photon absorbed when electron rises between levels: hf = Eupper - Elower Ionisation energy: minimum energy to completely remove an electron from the ground state

Emission spectrum
Bright lines on a dark background. Each line corresponds to a photon emitted when an electron drops from a higher to a lower energy level. Unique to each element.
Absorption spectrum
Dark lines on a continuous spectrum background. Photons at specific frequencies are absorbed as electrons jump to higher levels. Lines appear at the same frequencies as the emission spectrum.
Excitation
An electron absorbs a photon and jumps to a higher energy level. The photon energy must exactly match the energy gap; if not, the photon passes through.
Ionisation
An electron gains enough energy to completely escape the atom (energy ≥ ionisation energy). Can occur via photon absorption or electron collision.

Wave-particle duality: particles exhibit wave behaviour and waves exhibit particle behaviour. de Broglie proposed that all moving particles have an associated wavelength.

de Broglie wavelength: λ = h / p = h / (mv) where p = momentum, m = mass, v = velocity Higher momentum (faster or heavier) → shorter wavelength Electron diffraction confirms wave behaviour of particles

Wave-particle duality: light behaves as a wave (diffraction, interference) and as a particle (photoelectric effect). Electrons behave as particles (ionisation, deflection in fields) and as waves (electron diffraction). The behaviour observed depends on the experiment.

Section 3 - Waves

3.1.1 – 3.1.2  Progressive waves and wave types

Amplitude (A)
Maximum displacement of a particle from its equilibrium position. Unit: metres.
Frequency (f)
Number of complete oscillations per second. Unit: Hz (s-1). T = 1/f.
Wavelength (λ)
Distance between two adjacent points in phase (e.g. crest to crest). Unit: metres.
Wave speed (v)
Speed at which the wave pattern moves through the medium. v = fλ. Unit: m s-1.
Phase difference
The fraction of a cycle by which one wave leads or lags another. Measured in radians or degrees. One full cycle = 2π rad = 360°.
Path difference
Difference in distance travelled by two waves from their sources to a given point. A path difference of nλ gives constructive interference; (n+½)λ gives destructive interference.
Wave equation: v = fλ Period: T = 1/f Phase difference (φ) for path difference x: φ = (2π/λ) × x

Transverse waves
Oscillations are perpendicular to the direction of wave travel. Examples: all EM waves, waves on a string, S-waves (seismic). Can be polarised.
Longitudinal waves
Oscillations are parallel to the direction of wave travel. Compressions and rarefactions. Examples: sound, P-waves (seismic). Cannot be polarised.

Polarisation: a transverse wave is plane polarised when its oscillations are confined to a single plane (perpendicular to the direction of propagation). Unpolarised light oscillates in all planes simultaneously. Only transverse waves can be polarised; this is used as experimental evidence that light is a transverse wave.

Unpolarised light
Oscillations occur in all planes perpendicular to the direction of travel. Intensity is distributed equally across all planes.
Polarising filter (polariser)
Only transmits oscillations in one specific plane. Reduces intensity of unpolarised light by half: I = I₀/2 after the first filter.
Analyser
A second polarising filter placed after the polariser. Rotating the analyser varies transmitted intensity. At 90° (crossed polarisers), no light is transmitted.
Unpolarised light through one polariser: I = I₀ / 2
Uses of polarisation
Polaroid sunglasses: reduce glare by blocking horizontally polarised reflected light. LCD screens: liquid crystals rotate polarisation to control pixel brightness. Stress analysis: photoelastic materials show fringe patterns under polarised light, revealing stress in structures.
Polarisation in radio/microwaves
Aerials must be aligned with the polarisation of the transmitted signal. Rotating a microwave receiver relative to the transmitter varies the received signal strength (standard practical).

Polarisation is evidence that light is a transverse wave. Know that crossed polarisers (90°) give zero transmission – no component of the polarisation lies along the analyser axis. Unpolarised light loses half its intensity through a single polariser.

Intensity of a wave is proportional to amplitude squared: I ∝ A². Doubling the amplitude increases intensity by a factor of 4.

3.1.3  Superposition and stationary waves

The principle of superposition: when two or more waves overlap, the resultant displacement at any point is the algebraic sum of the individual displacements.

A stationary (standing) wave is formed when two waves of the same frequency and amplitude travel in opposite directions and superpose. Energy is stored, not transmitted.

Nodes
Points of zero displacement. Destructive superposition occurs here at all times. Fixed in position.
Antinodes
Points of maximum displacement (amplitude = 2A). Constructive superposition. Fixed in position, oscillate with maximum amplitude.
Distance between adjacent nodes = λ/2 Distance between adjacent antinode and node = λ/4 Fundamental frequency (1st harmonic) of a string: f = (1/2L) × √(T/μ) where L = length, T = tension, μ = mass per unit length

For a string fixed at both ends: harmonics occur at L = nλ/2 (n = 1, 2, 3...). For an open pipe: same as string. For a closed pipe: only odd harmonics; L = nλ/4 (n = 1, 3, 5...).

Distinguish stationary and progressive waves: in a stationary wave, all points between two nodes oscillate in phase with each other (amplitude varies by position). In a progressive wave, phase varies continuously along the wave.

3.2.3  Interference

Interference occurs when two coherent waves overlap. Coherent sources have the same frequency and a constant phase difference.

Constructive interference
Waves arrive in phase (path difference = nλ). Displacement adds up; maximum amplitude. Produces bright fringes.
Destructive interference
Waves arrive in antiphase (path difference = (n + ½)λ). Displacements cancel; zero amplitude. Produces dark fringes.
Young's double-slit formula: λ = ay / D where: a = slit separation y = fringe spacing (distance between adjacent bright fringes) D = distance from slits to screen Rearranged: y = λD / a

White light interference: each wavelength produces its own fringe pattern with a different spacing. The central maximum (zero order) is white (all wavelengths overlap). Higher orders show coloured fringes: violet is closest to the centre (shortest λ, smallest spacing), red is furthest. The fringes overlap and become indistinct at high orders.

Laser safety: lasers produce intense, coherent, collimated beams and can cause permanent retinal damage. Never look directly into a laser beam or point it at people. Use laser safety goggles at appropriate wavelengths; ensure the beam is at bench level with no reflective surfaces nearby.

Young's double-slit experiment provides evidence for the wave nature of light. The fringes are equally spaced. Larger λ or larger D gives wider fringes; larger slit separation a gives narrower fringes.

3.2.2  Diffraction

Diffraction is the spreading of a wave as it passes through a gap or around an obstacle. Maximum diffraction occurs when the gap width is approximately equal to the wavelength.

Single slit diffraction: a monochromatic source passing through a narrow slit produces a pattern with a wide, bright central maximum flanked by alternating dark minima and weaker secondary maxima.

Central maximum
Twice as wide as any subsidiary maximum. Much brighter than secondary maxima. Increasing wavelength or decreasing slit width both make the central maximum wider and more spread out.
Effect of slit width (a)
Narrower slit → greater diffraction → wider central maximum. Wider slit → less diffraction → narrower, more intense central maximum. For a >> λ, diffraction is negligible.
First minimum (single slit): sin θ = λ / a where a = slit width, θ = angle to first dark fringe Central maximum half-width: θ ≈ λ / a (for small angles)

The single slit and double slit patterns combine: the double-slit interference fringes are modulated by the single-slit envelope. Fringes near the centre are bright; those near the single-slit minima disappear. This is why some orders are missing in double-slit patterns.


Diffraction grating equation: d sin θ = nλ where: d = slit spacing = 1 / (number of slits per metre) θ = angle to the nth order maximum n = order number (0, 1, 2...) λ = wavelength of light Maximum order: nmax = d / λ (when sin θ ≤ 1)

The diffraction grating produces very sharp, bright maxima (unlike the broad fringes from a double slit). Used to measure wavelengths of light precisely.

In the diffraction grating equation, check that nλ/d ≤ 1 before calculating θ. If nλ > d, that order does not exist. The zero-order maximum (n=0) is always straight ahead at θ = 0.

3.2.1  Refraction at a plane surface

Refraction is the change in direction of a wave when it passes from one medium to another due to a change in wave speed.

Snell's law: n1 sin θ1 = n2 sin θ2 Refractive index: n = c / v (ratio of speed of light in vacuum to speed in medium) Critical angle C: sin C = n2 / n1 = 1/n (if medium 2 is air, n2 = 1) Total internal reflection occurs when: - light travels from denser to less dense medium (n1 > n2) - angle of incidence > critical angle

Optical fibres (step-index) consist of a high-refractive-index core surrounded by a lower-refractive-index cladding. Light travels in the core and undergoes total internal reflection at the core-cladding boundary. The cladding: (1) enables TIR by providing a lower-index boundary; (2) protects the core; (3) prevents light leaking between adjacent fibres (crosstalk). Used in communications (digital signals) and medical imaging (endoscopes).

Modal dispersion in step-index fibres: rays entering at different angles travel different path lengths, causing pulse broadening. Reduced by using monomode fibres (very narrow core). Material dispersion occurs because different wavelengths travel at different speeds; reduced by using monochromatic light.

When light goes from dense to less dense (e.g. glass to air), it bends away from the normal. When it goes from less dense to denser, it bends towards the normal. Light speeds up in less dense media.

Section 4 - Mechanics and materials

4.1.1 – 4.1.2  Scalars, vectors and moments

Scalar
Has magnitude only. Examples: mass, speed, distance, energy, temperature, time.
Vector
Has both magnitude and direction. Examples: force, velocity, displacement, acceleration, momentum.

Adding vectors: two vectors at right angles are added by calculation (Pythagoras for magnitude, trigonometry for direction). Vectors at any angle can be added by accurate scale drawing. For three coplanar forces in equilibrium, a closed triangle can be drawn the vectors form a closed loop placed head-to-tail.

Resolving vectors: Fx = F cos θ, Fy = F sin θ. Resolve each vector into horizontal and vertical components, sum each direction, then use Pythagoras for the resultant magnitude and trigonometry for its direction. Problems may also be solved using the closed triangle method.

An object is in equilibrium when the resultant force on it is zero and the resultant moment about any point is zero. This applies whether the object is at rest or moving at constant velocity.


Moment of a force: M = F × d where d is the perpendicular distance from the pivot to the line of action of the force. Unit: N m Principle of moments (equilibrium): Sum of clockwise moments = Sum of anticlockwise moments Couple: torque = F × d where d = perpendicular distance between the lines of action of the two forces

A couple is a pair of equal and opposite coplanar forces that produce a pure turning effect (no resultant force).

Centre of mass: the single point through which the weight of an object appears to act. For a uniform regular solid, the centre of mass is at its geometric centre.

For an object in equilibrium: (1) resultant force = 0 (no acceleration), AND (2) resultant moment about any point = 0 (no angular acceleration). Both conditions must be met simultaneously.

4.1.3 – 4.1.4  Motion and projectiles

Definitions:

velocity: v = Δs / Δt (rate of change of displacement) acceleration: a = Δv / Δt (rate of change of velocity) Average speed/velocity = total distance or displacement / total time Instantaneous velocity = gradient of displacement–time graph at that point

Graphical methods for uniform and non-uniform acceleration:

Displacement–time graph
Gradient = velocity. Straight line = uniform velocity; curved = changing velocity (e.g. bouncing ball).
Velocity–time graph
Gradient = acceleration. Area under graph = displacement. Straight line = uniform acceleration; curved = non-uniform.
Acceleration–time graph
Area under graph = change in velocity.
Bouncing ball
On a v–t graph, speed at each bounce decreases (energy lost); velocity reverses sign at each impact. On a s–t graph, successive peaks fall.

The SUVAT equations apply to constant (uniform) acceleration in a straight line:

v = u + at s = ut + ½at² v² = u² + 2as s = ½(u + v)t s = displacement (m), u = initial velocity (m s-1) v = final velocity (m s-1), a = acceleration (m s-2), t = time (s)

Acceleration due to gravity g ≈ 9.81 m s-2 downwards near Earth's surface.


Projectile motion: horizontal and vertical components are independent. No air resistance assumed.

Horizontal
Constant velocity (a = 0). x = vxt. No force acts horizontally (ignoring air resistance).
Vertical
Constant acceleration g = 9.81 m s-2 downwards. Use SUVAT with a = −g (taking up as positive).

Friction, drag and terminal speed:

Friction
A contact force opposing relative motion between surfaces. Treated qualitatively no distinction between static and dynamic friction is required.
Drag
A resistive force opposing motion through a fluid. Increases with speed. Reduces range and changes trajectory of a projectile compared with the no-drag case.
Lift
Force perpendicular to an object’s motion through a fluid, arising from its shape (e.g. aerofoil). Acts upward on an aircraft wing.
Terminal speed
Reached when drag equals the driving force (or weight for a falling object). Resultant force = 0, so acceleration = 0 and speed is constant. Air resistance limits the maximum speed of a vehicle.

To solve projectile problems: resolve the initial velocity into horizontal and vertical components, then treat each direction independently using the appropriate equations.

4.1.5 – 4.1.6  Newton's laws and momentum

Newton's First Law
An object remains at rest or in uniform motion unless acted upon by a resultant external force.
Newton's Second Law
F = ma. The resultant force on an object equals its rate of change of momentum: F = Δp/Δt.
Newton's Third Law
For every action there is an equal and opposite reaction. Forces act on different objects and are of the same type.
Momentum: p = mv (unit: kg m s-1) Impulse: J = FΔt = Δp = mΔv (where F is constant) Impulse = area under a force–time graph (for variable forces) Conservation of momentum: In a closed system (no external forces), total momentum is constant. m1u1 + m2u2 = m1v1 + m2v2 Elastic collision: total KE conserved. Inelastic collision: KE not conserved (some converted to thermal energy/sound). Perfectly inelastic: objects stick together after collision. Explosion: system starts at rest; momenta of separating parts are equal and opposite (total = 0).

Understanding impulse and momentum underpins ethical transport design: crumple zones, airbags, and seatbelts all increase collision time, reducing the peak force on occupants. Impact forces are related to contact times (e.g. kicking a football, crumple zones, packaging). Quantitative questions may involve forces that vary with time.

Impulse = area under a force-time graph. A large force for a short time produces the same impulse (and change in momentum) as a small force for a long time. This is the principle behind crumple zones and airbags.

4.1.7 – 4.1.8  Work, energy and power

Work done: W = Fs cos θ (F = force, s = displacement, θ = angle between F and s) For a variable force: W = area under the force–displacement graph Kinetic energy: Ek = ½mv² Gravitational PE: ΔEp = mgΔh Power: P = ΔW / Δt = Fv Efficiency = (useful output power / total input power) × 100% (also expressible as a decimal) Work-energy theorem: net work done = change in kinetic energy

Conservation of energy: energy cannot be created or destroyed, only converted from one form to another. When resistive forces act, kinetic or potential energy is transferred to thermal energy; the total (Ek + Ep + energy dissipated against resistive forces) remains constant. Without resistive forces: Ek + Ep = constant.

Work is only done when the force has a component in the direction of motion. A centripetal force does no work because it is always perpendicular to the velocity.

4.2  Materials: stress, strain and the Young modulus

Density: ρ = m / V (unit: kg m-3)
Hooke's Law
Force is proportional to extension up to the limit of proportionality: F = kΔL, where k is the spring constant / stiffness (N m-1). Beyond the elastic limit, permanent deformation occurs.
Elastic deformation
Material returns to its original shape when the force is removed. The elastic limit is the maximum stress from which it fully recovers.
Plastic deformation
Permanent deformation beyond the elastic limit. Material does not return to its original shape or length.
Elastic strain energy
E = ½FΔL = ½kΔL². Equals the area under the force-extension graph (linear region). Energy stored in a spring can be transformed into kinetic and gravitational potential energy on release.

Force-extension behaviour and material types:

Ductile material
Large plastic region before fracture. Yields and stretches considerably (e.g. copper wire). Area under F-extension graph = total energy to deform.
Brittle material
Little or no plastic region; fractures suddenly near the elastic limit with no prior plastic deformation (e.g. glass, cast iron). Force-extension graph is linear to the point of fracture.

Tensile stress: σ = F / A (unit: Pa or N m-2) Tensile strain: ε = ΔL / L (dimensionless) Young modulus: E = σ / ε = FL / (AΔL) (unit: Pa) Breaking stress (UTS): maximum stress a material can withstand before fracture

Stress-strain graphs: gradient of the linear (Hooke's law) region = Young modulus; area under graph = elastic strain energy per unit volume. Ductile materials show a yield point then a long plastic region; brittle materials fracture near the elastic limit with no plastic region.

Required Practical 4: determination of the Young modulus by a simple method (e.g. measuring extension of a long wire under known loads using a vernier scale).

Appreciation of energy conservation in ethical transport design: materials that deform plastically absorb more energy (larger area under F-extension graph), informing the design of crumple zones and protective packaging.

The Young modulus is a property of the material (independent of dimensions). The spring constant k depends on both material and dimensions. Use a stress-strain graph to find E; use a force-extension graph to find k.

Section 5 - Electricity

5.1.1 – 5.1.2  Fundamentals and I-V characteristics

Charge: Q = It (unit: coulombs, C) Current: I = ΔQ / Δt (unit: amperes, A) Potential difference: V = W/Q (energy per unit charge; unit: volts, V) Resistance: R = V/I (unit: ohms, Ω) Power: P = IV = I²R = V²/R (unit: watts, W) Energy: E = Pt = IVt (unit: joules, J)

I-V characteristics show how current varies with potential difference:

Ohm's law is a special case: for an ohmic conductor, I ∝ V under constant physical conditions. This gives a straight-line I–V graph through the origin with constant gradient (constant resistance).

Ohmic conductor
Straight line through the origin. Resistance is constant (independent of current). Example: metal wire at constant temperature.
Filament lamp
Curve that flattens. Resistance increases with temperature (and hence current) as lattice vibrations increase. Non-ohmic.
Semiconductor diode
Conducts in forward bias above ~0.6 V (silicon); very high resistance in reverse bias. Non-ohmic. Threshold voltage ~0.6 V for silicon.

NTC thermistor: resistance decreases as temperature increases (opposite to a metal). LDR (light-dependent resistor): resistance decreases as light intensity increases. Both are non-ohmic.

Ideal meters: unless otherwise stated, ammeters have zero resistance (no voltage drop across them) and voltmeters have infinite resistance (no current through them). Questions can be set with either I or V on the horizontal axis of a characteristic graph.

Current is the same at all points in a series circuit. The sum of potential differences across components in a series circuit equals the supply voltage. These are direct consequences of charge conservation and energy conservation.

5.1.3  Resistivity

Resistivity: R = ρL / A where: R = resistance (Ω) ρ = resistivity of the material (Ω m) L = length of conductor (m) A = cross-sectional area (m²) Rearranged: ρ = RA / L

Resistivity is a property of the material (not the sample). It depends on temperature: metals increase in resistivity with temperature; semiconductors (including NTC thermistors) decrease in resistivity with temperature. Only negative temperature coefficient (NTC) thermistors are assessed. Thermistor applications include temperature sensors; behaviour is shown on resistance–temperature graphs.

Superconductivity: some materials have zero resistivity at and below a critical temperature Tc (which depends on the material). The resistance drops suddenly to exactly zero. Applications include: production of strong magnetic fields (e.g. MRI scanners, particle accelerators) and reduction of energy loss in transmission of electric power. Note: critical field is not assessed.

Required Practical 5: determination of the resistivity of a wire using a micrometer, ammeter, and voltmeter.

Resistivity and resistance are different: resistance (R) depends on the material AND dimensions; resistivity (ρ) depends only on the material and temperature. To find the resistivity of a wire, measure R, L, and diameter (to find A = πr²).

5.1.4  Circuits

Kirchhoff's First Law (charge conservation): ΣI = 0 at a junction (sum of currents entering = sum leaving) Kirchhoff's Second Law (energy conservation): ΣEMF = ΣIR around any closed loop Resistors in series: Rtotal = R1 + R2 + R3 + ... Current same through all; voltage divides. Resistors in parallel: 1/Rtotal = 1/R1 + 1/R2 + 1/R3 + ... Voltage same across all; current divides. Rtotal is always less than the smallest individual resistance. Cells in series: EMFtotal = ϵ1 + ϵ2 + ... (internal resistances add too) Identical cells in parallel: same EMF as one cell; internal resistance halved for two cells.

Conservation of charge (Kirchhoff's First Law) and conservation of energy (Kirchhoff's Second Law) apply throughout all dc circuits. Currents, voltages, and resistances in series and parallel combinations follow directly from these principles.

Adding a resistor in series always increases total resistance. Adding a resistor in parallel always decreases total resistance. Use this as a quick sanity check on your answers.

5.1.5  Potential divider

A potential divider is used to supply a constant or variable potential difference from a power supply. The output voltage is taken across one of the resistors in a series chain.

Vout = Vin × R2 / (R1 + R2) where R2 is the resistor across which Vout is measured.

Components used in the potential divider include variable resistors (to supply a variable output voltage), thermistors (output varies with temperature), and LDRs (output varies with light intensity). Note: the use of the potentiometer as a measuring instrument is not required.

If R2 increases (e.g. thermistor cools down → resistance rises), Vout increases. If R2 decreases, Vout decreases. This logic is essential for analysing sensor circuits.

5.1.6  EMF and internal resistance

Electromotive force (EMF, ϵ) is the total energy supplied per unit charge by the source: ϵ = E/Q. It differs from terminal pd because some energy is dissipated within the source due to internal resistance r.

EMF: ϵ = E / Q (energy per unit charge; unit: V) ϵ = I(R + r) = IR + Ir = Vterminal + Ir Terminal pd: V = ϵ - Ir "Lost volts" = Ir (energy dissipated per unit charge inside the source) At maximum current (short circuit, R = 0): Imax = ϵ / r At open circuit (no current, I = 0): V = ϵ Graphical method: plot V against I. y-intercept = ϵ Gradient = −r

Required Practical 6: investigation of the emf and internal resistance of electric cells and batteries by measuring the variation of the terminal pd of the cell with current in it.

As more current is drawn from a battery, the terminal pd falls because the "lost volts" (Ir) increase. A battery with a high internal resistance cannot deliver large currents without a significant voltage drop. This explains why old batteries struggle to start cars.