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These notes are AI-assisted study material. Always cross-check against the official 9702 syllabus or your teacher before relying on them in an exam.

9702 AS Level Physics

Comprehensive AS Notes · Cambridge International AS Level (2025–2027)
Authors: Colin Young, Yuchen Wang
Paper 1 · MCQ Paper 2 · Structured Paper 3 · Practical 11 Topics

01Physical Quantities and Units

Foundations: every measurement combines a numerical magnitude and a unit. Mastery of SI units, dimensional analysis, errors, and uncertainties underpins every other topic.

1.1 SI Base Units

All physical quantities are derived from seven SI base quantities. In 9702 you need to know six (luminous intensity not required):

Base QuantitySymbolBase UnitSymbol
Massmkilogramkg
Lengthlmetrem
Timetseconds
Electric currentIampereA
Thermodynamic temp.TkelvinK
Amount of substancenmolemol

1.2 Derived Units & Dimensional Analysis

Every other quantity has a unit built from products and quotients of base units. The dimension of a quantity shows which base units it involves, written as [M]a[L]b[T]c[A]d.

QuantityDerived UnitIn Base UnitsDimensions
Forcenewton (N)kg m s-2[M][L][T]-2
Energy / Workjoule (J)kg m2 s-2[M][L]2[T]-2
Powerwatt (W)kg m2 s-3[M][L]2[T]-3
Pressure / Stresspascal (Pa)kg m-1 s-2[M][L]-1[T]-2
Chargecoulomb (C)A s[A][T]
Potential diff.volt (V)kg m2 s-3 A-1[M][L]2[T]-3[A]-1
Resistanceohm (Ω)kg m2 s-3 A-2[M][L]2[T]-3[A]-2
Homogeneous equation: the units (or dimensions) on both sides must be the same. Dimensional analysis detects algebraic errors but cannot verify dimensionless constants or sign correctness.
Example — checking homogeneity
Verify T = 2π√(l/g): Left side [T]. Right side: √([L] / [L][T]-2) = √([T]2) = [T]. ✓ Homogeneous.

1.3 SI Prefixes

NameSymbolFactor NameSymbolFactor
picop10-12kilok103
nanon10-9megaM106
microμ10-6gigaG109
millim10-3teraT1012
centic10-2

1.4 Scalars and Vectors

Scalar: a quantity with magnitude only (e.g. mass, speed, distance, time, energy, temperature, density).
Vector: a quantity with magnitude and direction (e.g. displacement, velocity, acceleration, force, momentum, field strength).

Vector addition: tip-to-tail (head-to-tail) method or parallelogram rule. Resolution splits a vector into perpendicular components.

Component resolutionFx = F cos θ,  Fy = F sin θ
Resultant magnitude and directionR = √(Fx2 + Fy2),  tan θ = Fy / Fx
Choose θ from the horizontal axis consistently. The angle of the resultant is measured anticlockwise from the positive x-axis.

1.5 Errors and Uncertainties

Absolute uncertainty (Δx): half the range of repeated readings: Δx = ½(xmax - xmin). Same unit as x.
Fractional uncertainty: Δx / x (unit-free).
Percentage uncertainty:x / x) × 100%.
Systematic error: consistent bias (zero error, parallax error, calibration errors). Not reduced by repeating; accuracy is affected.
Random error: unpredictable scatter (reaction time, electronic noise). Reduced by repeating and averaging; precision is affected.
Precision: how close repeated readings are to each other (indicated by % uncertainty and sig. figs.).
Accuracy: how close the mean is to the true value.
Propagation rules — must know for Paper 3:
• Addition / subtraction: add absolute uncertainties: ΔS = ΔA + ΔB (for S = A + B or A - B)
• Multiplication / division: add percentage (or fractional) uncertainties.
• Power n: multiply the percentage uncertainty by |n|.
• Multiplication by a constant: % uncertainty is unchanged.
• General: for Q = Al Bm Cn …,   ΔQ/Q = |l|(ΔA/A) + |m|(ΔB/B) + |n|(ΔC/C) + …
Worked example — propagation
L = (1.250 ± 0.005) m → % unc. = 0.4%.  d = (0.40 ± 0.01) mm → % unc. = 2.5%.
Area A = πd2/4. % unc. in A = 2 × 2.5 = 5.0 %. (π and 4 are constants — ignore.)
g = 4π2L/T2. % unc. in g = % unc. in L + 2 × % unc. in T.

Concept check: measurements are models of reality

A unit states the scale used to compare a measurement; a dimension states how a quantity is built from base quantities. Dimensional analysis can reject an equation with inconsistent units, but it cannot prove an equation is physically correct because a missing numerical factor or wrong sign may still have the right dimensions.

Random uncertainty causes readings to scatter around a mean and is reduced by repeats. Systematic error shifts readings consistently and requires calibration, a zero correction or a better method. Quote uncertainty honestly: more decimal places do not make a measurement more accurate.

1.6 Checking Homogeneity and Making Estimates

Every physical quantity is a magnitude and a unit. Use base units to test an equation: both sides must have the same combination of kg, m, s, A and K. Prefixes from pico (10−12) to tera (1012) must be converted before substituting.

You must be able to make a reasonable order-of-magnitude estimate (mass of a person ~70 kg, walking speed ~1.5 m s−1, atmospheric pressure ~105 Pa, visible wavelength ~5×10−7 m).

1.7 Combining Uncertainties

  • Sums and differences: add absolute uncertainties.
  • Products, quotients and powers: add percentage (or fractional) uncertainties. For xn multiply the % uncertainty by |n|.
  • A zero error is systematic. Repeating and averaging reduces random error, not systematic error. Precise = small scatter; accurate = close to the true value.

02Kinematics

Describing motion: distance, displacement, velocity, acceleration, motion graphs, SUVAT, projectiles.

2.1 Core Definitions

Distance: total path length (scalar).
Displacement: vector from start to finish.
Speed: rate of change of distance.
Velocity: rate of change of displacement.
Acceleration: rate of change of velocity (m s-2).

2.2 Motion Graphs

GraphGradientArea under
stVelocity
vtAccelerationDisplacement
atChange in velocity

2.3 SUVAT (Constant Acceleration)

v = u + at
s = ut + 1/2at2
v2 = u2 + 2as
s = 1/2(u + v)t

2.4 Free Fall

g = 9.81 m s-2 downward, neglecting air resistance.

2.5 Projectile Motion

Horizontal and vertical components are independent. Horizontal: constant velocity. Vertical: uniform acceleration g. Trajectory is a parabola.

Worked example
Ball launched horizontally at 15 m s-1 from a 20 m cliff. Time of flight: t = √(2×20/9.81) = 2.02 s. Range = 15 × 2.02 = 30.3 m.

2.6 Air Resistance and Terminal Velocity

Drag increases with speed. When drag = weight, resultant force = 0, body falls at terminal velocity.

Concept check: choose the quantity the graph represents

Distance is total path length and is scalar; displacement is the directed change in position. Likewise speed is scalar while velocity is vector. A negative velocity does not mean an object is slowing down - it means it is moving in the chosen negative direction.

On a displacement-time graph, gradient is velocity. On a velocity-time graph, gradient is acceleration and signed area is displacement. SUVAT equations are only a compact form of constant-acceleration motion; use components independently for projectile motion and do not apply one SUVAT equation across a stage where acceleration changes.

2.7 Deriving the SUVAT Equations

From the definitions a = dv/dt and v = ds/dt with constant a:

  • v = u + at follows at once by integrating constant acceleration.
  • Displacement is the area under the vt graph: a trapezium of sides u and v gives s = ½(u+v)t.
  • Eliminate t or v to obtain s = ut + ½at2 and v2 = u2 + 2as.

2.8 Experiment: Acceleration of Free Fall

Drop an object through a measured height from rest and time the fall (light gates or a trapdoor–electromagnet). From s = ½gt2, a graph of s against t2 is a straight line of gradient g/2. Repeat, use a small dense object to reduce drag, and include the uncertainty in t (which is squared).

03Dynamics

Newton's laws, mass, weight, free-body diagrams, friction, drag, inclined planes, connected bodies and momentum conservation.

3.1 Newton's Three Laws

1st Law (Inertia): a body remains at rest or moves with constant velocity unless acted on by a resultant force. If ΣF = 0, the body is in equilibrium.
2nd Law: the resultant force on a body equals its rate of change of momentum: F = Δpt. For constant mass: F = ma. 1 N = 1 kg m s-2.
3rd Law (Action-Reaction): when body A exerts a force on body B, body B exerts an equal and opposite force on body A. The forces act on different bodies, are of the same type, and are equal in magnitude and opposite in direction.
N3 pitfall: the reaction to a book's weight (mg downwards) is the book's gravitational pull upwards on the Earth — NOT the normal contact force from the table. Weight and normal force act on the same body so cannot be an action-reaction pair.

3.2 Mass and Weight

Mass (m): scalar measure of inertia — resistance to change in motion. Unit: kg. Constant everywhere.
Weight (W): gravitational force on a body: W = mg. Vector, unit: N. Varies with g. On Earth, g ≈ 9.81 N kg-1.
W = mg

3.3 Free-Body Diagrams (FBD)

Reduce an object to a point mass and draw all forces as labelled arrows from that point. Include: weight (downwards), normal contact (perpendicular to surface), friction (parallel to surface, opposing motion), tension (along string, away from body), drag (opposite to velocity).

Always draw forces on the body you are analysing. Do not include forces exerted by that body on other objects.

3.4 Drag Force

Drag opposes motion through a fluid. It depends on speed, shape, cross-sectional area and fluid density.

Low speed (laminar flow): f = bv — drag ∝ velocity.
High speed (turbulent flow): f = ½ρCDAv2 — drag ∝ velocity2.

Falling through a fluid: Fnet = mg - f. Initially a = g; as speed increases, f increases, acceleration decreases. When f = mg, a = 0 and the body falls at terminal velocity.

3.5 Normal Contact Force and Friction

Normal contact force (R): perpendicular component of contact force between two surfaces. Arises from electrostatic repulsion between surface atoms.

Friction (f): component of contact force parallel to the surface, opposing relative motion.
Static friction (fS): self-adjusting up to a limit; opposes tendency of motion.
Limiting friction (flim): maximum static friction: flim = μR, where μ = coefficient of friction.
Kinetic friction (fK): opposes actual sliding. For most surfaces fKflim = μR.

3.6 Inclined Slope

For a body of mass m on a slope inclined at angle θ to the horizontal:

Component parallel to slope: W = mg sinθ
Component perpendicular to slope: W = mg cosθ

For a smooth (frictionless) slope: Fnet = mg sinθ = ma, so a = g sinθ. For a rough slope: Fnet = mg sinθ - μmg cosθ.

The normal reaction R = mg cosθ (not mg) on an inclined slope. Students often forget this.

3.7 Connected Bodies

For two masses mA and mB connected by a light inextensible string over a smooth pulley:

Atwood machine (both hanging)a = (mA - mB)g / (mA + mB)
TensionT = 2mAmBg / (mA + mB)
Mass on table + hanging massa = mg / (M + m)
Method: (1) Draw separate FBDs for each body. (2) Apply Fnet = ma to each. (3) Use the same a and T for both (light inextensible string).

3.8 Momentum

Momentum (p): product of mass and velocity: p = mv. Vector. Unit: kg m s-1 = N s.
Impulse–momentum relationF = Δpt;  Impulse = FΔt = Δp

The area under an F-t graph equals the change in momentum (= impulse). The gradient of a p-t graph gives the net force.

3.9 Conservation of Momentum

For a closed system with zero net external force, total momentum remains constant: m1u1 + m2u2 = m1v1 + m2v2.

For 2-D collisions, apply conservation independently to x and y components.

3.10 Elastic vs Inelastic Collisions

TypeMomentumK.E.Relative speed
Perfectly elasticConservedConservedv2-v1 = u1-u2
InelasticConservedNot conservedReduced
Perfectly inelasticConservedMax K.E. lostBodies stick together
Momentum is always conserved in collisions (no external force). Kinetic energy is only conserved in perfectly elastic collisions.

Concept check: always identify the system first

A force is an interaction, not a property carried by an object. Draw only forces acting on the chosen body. Newton's third-law pair acts on two different bodies, so it never cancels on one free-body diagram.

Friction and drag oppose relative motion or attempted relative motion, while a normal contact force is perpendicular to the surface. Terminal speed occurs when drag plus upthrust balances weight, so resultant force and acceleration become zero even though the object keeps moving at constant speed.

3.11 Elastic Collision Extra Condition

Momentum of an isolated system is always conserved. For a perfectly elastic collision, kinetic energy is also conserved and the relative speed of approach equals the relative speed of separation along the line of centres.

3.12 Two-Dimensional Collisions

Resolve into two perpendicular components. Momentum is conserved separately in each direction. Do not apply the 1-D relative-speed rule unless the collision is head-on. After the collision, recombine components to find speed and direction.

04Forces, Density and Pressure

Turning effects of forces, equilibrium conditions, centre of gravity, density, fluid pressure and Archimedes' upthrust.

4.1 Moment of a Force

Moment (torque, τ): the product of a force and the perpendicular distance from the pivot to its line of action: τ = F d. Unit: N m. Vector direction: clockwise or anticlockwise.
τ = F d sin θ,  where d sinθ = lever arm

If the force is not perpendicular to the lever, resolve it into components or find the perpendicular distance from the pivot to the force's line of action.

4.2 Couple and Torque

Couple: a pair of equal and opposite parallel forces whose lines of action do not coincide. Produces pure rotation with no net translational force.
τcouple = F L

where L is the perpendicular distance between the two force lines. The torque of a couple is independent of the choice of pivot.

4.3 Mechanical Equilibrium

A rigid body is in equilibrium when both conditions are satisfied:
1. Resultant force = 0 in any direction: ΣF = 0 (translational equilibrium).
2. Resultant moment = 0 about any point: Στ = 0 (rotational equilibrium).
Principle of momentsΣ clockwise moments = Σ anticlockwise moments  (about any pivot)
When solving equilibrium problems, choose a pivot that eliminates unknown forces (where lines of action intersect).

4.4 Centre of Gravity / Centre of Mass

Centre of gravity: the point at which the entire weight of the body may be considered to act.
Centre of mass: the average position of all the mass in an object.
Near Earth's surface, centre of mass = centre of gravity. For uniform bodies: at the geometrical centre. Found experimentally by suspending from multiple points and tracing plumb-lines.

4.5 Forces in Equilibrium

Two forces: equal, opposite, same line of action.

Three forces: their vector sum forms a closed force triangle, and their lines of action must be concurrent (pass through a single point). Use the Law of Sines to find unknown magnitudes.

n forces: general condition: the force vectors form a closed polygon.

4.6 Density and Pressure

ρ = m/V  (kg m-3);  p = F/A  (Pa = N m-2)

4.7 Hydrostatic Pressure

At depth h in a fluid of uniform density ρ, the pressure due to the fluid alone is p = ρgh. Total pressure = ρgh + Patm.
Δp = ρgΔh

Derivation: column of cross-section A, height h: weight = ρAhg, pressure on base = ρAhg/A = ρgh.

Manometer: U-tube with liquid (often mercury, ρHg = 1.36 × 104 kg m-3): P1 - P2 = ρgΔh.

Barometer: inverted mercury-filled tube in basin; Patm = ρgh.

4.8 Upthrust (Archimedes' Principle)

Upthrust (FU): the upward buoyant force on a body immersed (partially or fully) in a fluid. It equals the weight of the fluid displaced.
FU = ρfluid gVdisplaced

Origin: the pressure on the bottom face (at greater depth) exceeds the pressure on the top face. Net force is upward.

Floating/sinking: Fnet = W - FU = (ρbody - ρfluid)gV. Body sinks if ρbody > ρfluid; rises if ρbody < ρfluid; floats partially submerged when FU = W.

Concept check: equilibrium needs both force and turning balance

A body in equilibrium has zero resultant force and zero resultant moment. A moment is a turning effect, so its perpendicular distance is measured from the pivot to the line of action of the force - not simply to the point where the force is drawn.

Pressure is normal force per unit area; in a stationary liquid, pressure difference depends on vertical depth because lower fluid supports the weight of liquid above. Upthrust is the resultant of the larger pressure on the bottom surface than on the top, and equals the weight of fluid displaced.

05Work, Energy and Power

Mechanical work, kinetic and potential energy, energy conservation, efficiency and power.

5.1 Work Done by a Force

Work (W): the product of a force and the displacement of its point of application in the direction of the force. W = F s cos θ. Scalar. Unit: joule (J); 1 J = 1 N m.
W = F s cos θ

When the force is perpendicular to the motion (θ = 90°), no work is done. Example: centripetal force does zero work. For a varying force, work = area under an F-s graph. For a gas expanding at constant pressure: W = pΔV.

5.2 Types of Energy

Kinetic energy: energy due to motion: Ek = ½mv2.
Derivation: W = F s = ma s. With v2 = u2 + 2as, W = ½m(v2 - u2) = ΔEk.
Gravitational potential energy: energy due to position in a gravitational field: ΔEp = mgΔh. GPE is relative — only changes matter.
Elastic potential energy (strain energy): energy stored in a deformed elastic body: Ep = ½kx2 = ½Fx.

5.3 Work–Energy Theorem

Work–energy theorem: the net work done on a body equals its change in kinetic energy: Wtotal = ΔEk = ½mv2 - ½mu2.

5.4 Conservative and Non-Conservative Forces

Conservative force: the work done is independent of the path taken and depends only on the initial and final positions. Examples: gravity, electric force, spring force. For a conservative force, ΔEp = -Wc.
Non-conservative force: the work done depends on the path taken. Examples: friction, drag, air resistance. The work done by non-conservative forces equals the change in total mechanical energy: Wnc = ΔEm.

5.5 Conservation of Energy

Energy cannot be created or destroyed; it can only be transferred between different forms. In the absence of non-conservative forces, mechanical energy is conserved: Ek + Ep = constant.

5.6 Power

Power (P): the rate of doing work: P = ΔWt. Unit: watt (W); 1 W = 1 J s-1.
P = W/t = F v  (for constant force and velocity along same line)

P = F v is used for vehicles at constant speed against resistive forces. At maximum speed, driving force = resistive force.

5.7 Efficiency

Efficiency (η): the ratio of useful output to total input, often expressed as a percentage.
η = (useful energy output / total energy input) = (useful power output / total power input)

η is always < 1 (or < 100 %) due to energy dissipated as heat, sound, etc.

Concept check: energy is transferred, not used up

Work is energy transferred when a force has a component along a displacement. The work-energy theorem connects resultant work to change in kinetic energy. Conservation of energy still holds when a system slows due to friction; organised kinetic energy is transferred mainly to less useful thermal energy in the object and surroundings.

Power is the rate of energy transfer. Efficiency compares useful output with total input and has no unit; state clearly what counts as useful in the context. A force perpendicular to motion does no work, even if the force itself is large.

5.8 Useful Derivations

Power: P = W/t = F × (s/t) = Fv when the force is in the direction of the velocity.

Gravitational PE near Earth: work done lifting at constant speed is W = mg × Δh, so ΔEP = mgΔh.

Kinetic energy: a resultant force F = ma does work Fs. Using v2 = u2 + 2as with u = 0 gives EK = ½mv2.

06Deformation of Solids

Hooke's law, spring combinations, stress, strain, Young modulus, stress–strain curves, elastic limit and elastic potential energy.

6.1 Elasticity

Elastic material: returns to its original shape when the deforming force is removed.
Plastic (inelastic) material: retains permanent deformation after the force is removed.

6.2 Hooke's Law

Hooke's law: the extension of an ideal spring is proportional to the applied force, up to the limit of proportionality. F = kx. The spring constant k (force constant) measures stiffness: larger k = stiffer spring. Unit: N m-1.
F = kx

On a F-x graph: the straight-line region obeys Hooke's law. Beyond the limit of proportionality, the graph curves. Beyond the elastic limit, the spring does not return to its original length on unloading.

6.3 Spring Combinations

Parallel springsk = k1 + k2 + …  (same extension for each spring)
Series springs1/k = 1/k1 + 1/k2 + …  (same force through each spring)

6.4 Elastic Potential Energy (Strain Energy)

Ep = ½Fx = ½kx2

The area under a F-x graph up to extension x equals the elastic potential energy stored. For Hookean springs: triangular area = ½ × base × height = ½kx2.

6.5 Stress, Strain, Young Modulus

Tensile stress (σ): force per unit cross-sectional area: σ = F/A. Unit: Pa (N m-2).
Tensile strain (ε): extension per unit original length: ε = x/L (unit-free).
Young modulus (E): ratio of tensile stress to tensile strain within the limit of proportionality: E = σ/ε. Unit: Pa. It is a property of the material — independent of the dimensions of the sample.
E = σ / ε =  (F/A) / (x/L) = FL/(Ax)

For metals: Emetal ~ 1011 Pa. Related to spring constant: k = EA/L.

6.6 Stress–Strain Curve for a Metal Wire

Key points on a typical stress–strain curve for a ductile metal (e.g. copper):

Limit of proportionality (LP): end of the straight-line (linear) region. Beyond LP, Hooke's law (E = σ/ε) no longer holds.
Elastic limit (LE): up to this point the wire returns to its original length when unloaded. Beyond LE, permanent deformation occurs (plastic). Usually LP ≈ LE for metals.
Yield point: sudden extension without increased load. The wire yields.
Ultimate tensile stress (UTS): the maximum stress the material can withstand before it fractures. Corresponds to the highest point on the curve.
Breaking stress (fracture): the stress at which the material breaks. Occurs after necking.

Loading/unloading hysteresis: after plastic deformation, the unloading path is parallel to the original elastic line. The area enclosed between loading and unloading curves = energy dissipated as heat.

6.7 Ductile vs Brittle Materials

Ductile (e.g. copper, mild steel): large plastic region, significant necking before fracture. Brittle (e.g. glass, cast iron): no plastic region — fractures at the elastic limit.

Polymeric materials (e.g. rubber): very different stress–strain behaviour. Large strain for small stress; does not obey Hooke's law except at very small extensions. Shows hysteresis when loaded and unloaded.

6.8 Experiment — Measuring Young Modulus

clamp long thin wire, original length L load F micrometer: diameter d extension x gradient = EA/L F x
  1. Use a long thin wire (≥ 2 m), clamped securely at the top.
  2. Measure the original length L with a metre rule.
  3. Measure the diameter d with a micrometer screw gauge at several points along the wire → average → \( A = \dfrac{\pi d^2}{4} \).
  4. Apply increasing loads, measure extension x each time (use a vernier scale or travelling microscope).
  5. Plot F vs x; gradient = \( \dfrac{EA}{L} \)  →  \( E = \dfrac{\text{gradient} \times L}{A} \).
  6. Safety: wear goggles; place a soft landing pad beneath the load; do not exceed the elastic limit.

Concept check: elastic does not mean perfectly proportional

An object is elastic if it returns to its original shape when the load is removed. Hooke's law is stricter: extension must be proportional to force, and applies only up to the limit of proportionality. The area under a force-extension graph is work done and hence elastic potential energy.

Stress compares force with cross-sectional area; strain compares extension with original length, so strain has no unit. Young modulus is a material property: a large value means a material is stiff, not necessarily strong or tough.

07Waves

Wave basics, progressive waves, intensity, transverse/longitudinal, Doppler, EM spectrum and polarisation.

7.1 Key Quantities

Displacement = distance from equilibrium position.
Amplitude = maximum displacement.
Period T = time for one complete oscillation.
Frequency f = 1/T = number of oscillations per second.
Wavelength = distance travelled by a wave in one period, or distance between neighbouring points in phase.

7.2 Wave Equation

v = fλ = λ/T

Crossing media: v and λ change; f stays the same.

7.3 Intensity

I = P/A;  IA2;  point source: I ∝ 1/r2

7.4 Transverse vs Longitudinal

TransverseLongitudinal
Oscillation ⊥ propagationOscillation ∥ propagation
Crests & troughsCompressions & rarefactions
Can be polarisedCannot be polarised

Mechanical waves need a medium, e.g. sound and waves on a string. Electromagnetic waves are oscillations of electric and magnetic fields and can travel through vacuum.

1. Transverse Wave

Displacement is perpendicular to the direction of wave travel. Particles oscillate up and down; energy moves horizontally.
Wave particles
Tracked particle
Amplitude
Wavelength
0.50 Hz
20 px
100 px/s
λ = 200 px T = 2.00 s
Key idea: The medium moves up and down; the wave energy moves left to right. No net displacement of particles.

2. Longitudinal Wave — Sound

Displacement is parallel to the direction of wave travel. Compressions (high pressure) and rarefactions (low pressure) alternate.
Air particles
Tracked particle
Compression (high p)
Rarefaction (low p)
0.60 Hz
15 px
96 px/s
λ = 160 px T = 1.67 s
Key idea: In a sound wave, particles oscillate back and forth about their equilibrium positions. The pressure variations are what our ears detect.

7.5 Doppler Effect (moving source)

fobs = fsv/(v ± vs)

Relative motion changes the observed frequency and wavelength. Use minus in the denominator when the source approaches; use plus when it moves away.

The effect applies to sound and electromagnetic waves. Approaching source or observer: observed frequency increases and wavelength decreases; separating source or observer: observed frequency decreases and wavelength increases.

7.6 EM Spectrum

All electromagnetic waves are transverse and travel at c = 3.00 × 108 m s-1 in vacuum. Order: Radio → Microwave → Infrared → Visible (red about 700 nm, violet about 400 nm) → UV → X-ray → γ.

7.7 Polarisation

Only transverse waves can be polarised. A polaroid transmits vibrations parallel to its transmission axis.

Unpolarised light contains vibrations in many transverse directions. After one polaroid, the emergent light is plane-polarised in the direction of the transmission axis.

Unpolarised through one polaroidI = I0/2
Malus's LawI = I0 cos2θ

7.8 CRO

Time-base × horizontal divisions per cycle = period. Y-gain × vertical divisions to peak = amplitude. For stationary-wave measurements, adjacent nodes are separated by λ/2.

Concept check: a wave transports a disturbance and energy

Particles in a medium oscillate about equilibrium; they do not travel with a progressive wave overall. Frequency is fixed by the source, while wave speed depends on the medium, so wavelength changes when a wave enters a medium with a different speed.

Intensity is power per unit area and is proportional to amplitude squared. Only transverse waves can be polarised because polarisation restricts oscillations to one plane; longitudinal sound waves cannot be polarised.

7.9 Doppler Formula (moving source)

fo = fs v / (v ± vs)

Use + in the denominator when the source moves away (lower observed frequency) and − when it moves towards the observer. The syllabus does not require a moving observer.

7.10 Malus's Law

Polarisation occurs only for transverse waves. After a polariser, intensity through an analyser at angle θ is

I = I0 cos2θ

Do not apply this formula to unpolarised incident light (that case is not required).

08Superposition

Principle of superposition, stationary waves, diffraction, interference, double-slit and diffraction grating.

8.1 Principle of Superposition

When two or more waves meet, the resultant displacement = vector sum of their individual displacements.

3. Superposition Principle

When two waves meet, the resultant displacement is the vector sum of the individual displacements.
Wave A (right-moving)
Wave B (left-moving)
Resultant (A + B)
18 px
0.55 Hz
Constructive interference: crest meets crest → larger amplitude. Destructive interference: crest meets trough → cancellation. After meeting, each wave continues unchanged.

8.2 Stationary Waves

Formed by two progressive waves of same frequency travelling in opposite directions.

Nodes: zero displacement. Antinodes: maximum displacement. Adjacent nodes = λ/2 apart. No net energy transfer.

For sound-speed experiments, adjacent nodes can be located with a CRO and microphone, or by sand / foam piling up at nodes in a tube. Measure the node-to-node separation, use λ = 2 × separation, then calculate v = .

  • Fixed or closed end → node.
  • Free or open end → antinode.
  • Two fixed ends or two open ends: allowed frequencies are f1, 2f1, 3f1, ...
  • One closed end and one open end: allowed frequencies are f1, 3f1, 5f1, ...

4. Standing (Stationary) Wave

Two progressive waves of the same frequency travelling in opposite directions superpose. Nodes (zero displacement) and antinodes (maximum displacement) form.
Particles
Antinode (max amplitude)
Node (zero displacement)
0.50 Hz
35 px
Nodes: 5 Antinodes: 4
Nodes (N) are points of zero displacement. Antinodes (A) are points of maximum amplitude. For a string of length L fixed at both ends: L = n·λ/2.

8.3 Diffraction

Spreading of a wave through a gap or around an obstacle. Most pronounced when gap ≈ λ.

Diffraction increases when wavelength increases, or when the gap / obstacle size becomes smaller.

8.4 Interference

Coherence: same frequency, constant phase difference.

Stable interference requires coherent sources. In practice, water-wave dippers may be driven by the same vibrator, sound sources by the same signal generator, and light sources by the same slit / double-slit system; two separate lamps are not coherent.

  • Path diff = → constructive (max).
  • Path diff = (n+1/2)λ → destructive (min).
  • Time diff = nT or phase diff = 2nπ → constructive.
  • Time diff = (n+1/2)T or phase diff = (2n+1)π → destructive.
Δt/T = ΔL/λ = Δφ/(2π)

8.5 Young's Double Slit

x = λD/a  or  λ = ax/D  (Da)

Bright fringes form where path difference = nλ. Changing slit width changes brightness, but not fringe spacing.

5. Double-Slit Interference

Two coherent sources produce an interference pattern. Bright fringes (constructive) and dark fringes (destructive) appear on a screen.
Wavefronts from slit 1
Wavefronts from slit 2
Constructive (bright)
Destructive (dark)
30 px
90 px
400 px
a/λ = 3.0 Fringe spacing w = λD/a
Fringe spacing: w = λD/a. Bright fringes occur where path difference = nλ; dark fringes where path difference = (n + 1/2)λ.

8.6 Diffraction Grating

d sinθ =

If there are N slits per metre, then d = 1/N. Highest possible order is nmax = floor(d/λ), so total number of principal maxima is 2nmax + 1.

With white light, the zero-order maximum is white, while first and higher orders are dispersed into colours; red appears at larger angles than violet.

Higher orders are more spread out. Maxima from different orders can overlap when different wavelengths satisfy n1λ1 = n2λ2 at the same angle.

6. Diffraction Grating

Multiple equally spaced slits produce sharp principal maxima. The grating equation: d sin θ = nλ. More slits → narrower, brighter peaks.
Principal maxima
Secondary maxima
Minima
30 px
120 px
5
Max orders n: 4 Angular resolution ∝ 1/N
Grating equation: d sin θ = . Principal maxima become sharper as N increases. Missing orders occur when a diffraction minimum coincides with an interference maximum.

Concept check: superposition is addition of displacement

When waves overlap, the resultant displacement is the algebraic sum of their individual displacements. Constructive interference occurs when waves arrive in phase; destructive interference occurs when they arrive in antiphase. Coherent sources must have the same frequency and a constant phase difference.

A stationary wave is made by two equal progressive waves travelling in opposite directions. It transfers no net energy along the medium and has fixed nodes and antinodes. Diffraction becomes significant when a gap or obstacle is comparable in size with the wavelength.

8.7 Stationary-Wave Experiments

  • Stretched string (sonometer / vibration generator): nodes at the fixed ends. λ = 2L/n. Speed from v = .
  • Air column (resonance tube): closed end is a node, open end an antinode. First resonance at L = λ/4 (end correction is neglected).
  • Microwaves: a metal plate reflects the wave; a probe finds nodes and antinodes. Node-to-node distance is λ/2.

8.8 Conditions for Two-Source Interference

The sources must be coherent (constant phase difference, same frequency) and of comparable amplitude. For light this usually means one source split into two paths. Fringe spacing x = λD/a.

09Electricity

Charge, current, pd, emf, resistance, Ohm's law, I–V graphs, resistivity and electrical power.

9.1 Current

I = Q/t;  Q = Ne

9.2 Drift Velocity

I = Anvq

For metals, drift speed is typically < 1 mm s-1.

9.3 PD and EMF

Pd: energy per unit charge transferred from electrical to other forms (component).
EMF: energy per unit charge transferred from other forms to electrical (source).
V = W/Q

9.4 Ohm's Law

For a metallic conductor at constant temperature, IV.

9.5 I–V Characteristics

ComponentBehaviour
Resistor (ohmic)Straight line through origin
Filament lampS-curve; R rises with T
DiodeThreshold ~0.6 V forward; almost no reverse current
NTC thermistorR falls as T rises

9.6 Power

P = VI = I2R = V2/R

9.7 Resistivity

R = ρL/A

9.8 LDR and Thermistor

LDR: R ↓ as light ↑. NTC thermistor: R ↓ as T ↑.

Concept check: current is charge flow, not energy flow

Current is the rate at which charge passes a point; conventional current is defined as the direction positive charge would move. In metals, electrons drift slowly opposite to conventional current while the electric field and energy transfer are established through the circuit much more quickly.

Potential difference is energy transferred per unit charge between two points. Emf is energy supplied per unit charge by a source. Resistance is the ratio of p.d. to current only for an ohmic conductor at constant temperature; a non-ohmic I-V curve needs a microscopic explanation involving temperature, carriers or a potential barrier.

9.9 Charge is Quantised

Charge comes in integer multiples of e = 1.60×10−19 C, so Q = Ne. Current is a flow of these carriers: I = Anvq.

9.10 Why a Filament Lamp is Non-Ohmic

Larger current heats the filament. Higher temperature increases the amplitude of ion vibrations, so the drift of electrons is hindered and resistance rises. The IV graph therefore curves towards the V axis.

10D.C. Circuits

EMF, internal resistance, Kirchhoff's laws, combinations, potential divider, bridge circuits, potentiometer and practical power.

10.1 EMF and Internal Resistance

Vterminal = ε - Ir
ε = VR + Vr = I(R+r)

Vterminal vs I: y-intercept = ε, gradient = -r. When R → 0, the short-circuit current is Imax = ε/r.

10.2 Kirchhoff's Laws

1st (junction): ΣI in = ΣI out (charge conservation).
2nd (loop): Σε = ΣIR (energy conservation).

10.3 Series and Parallel

SeriesR = R1 + R2 + ...
Parallel1/R = 1/R1 + 1/R2 + ...

10.4 Potential Divider

V1/V2 = R1/R2
V1 = R1Vin/(R1 + R2),  V2 = R2Vin/(R1 + R2)

Potential at a point is measured relative to a chosen zero-potential reference, often earth. Sensor circuits use this because changing one resistance changes the output pd.

10.5 Bridge Circuits

For the two divider branches, potential at the midpoints are VX = R2ε/(R1+R2) and VY = R4ε/(R3+R4).

VXY = VX - VY

A bridge is balanced when VXY = 0, so VX = VY and R1/R2 = R3/R4. This is useful for finding unknown resistances accurately.

10.6 Potentiometer

Long uniform wire; null method — no current at balance, so internal resistance of the test cell does not affect the reading.

Etest/Edrive = AP/AB

The emf or pd being tested is proportional to the balancing length along the wire.

The driver cell should have a known emf larger than the test emf, and its internal resistance should be negligible compared with the resistance wire. At null balance the galvanometer reads zero, so no current is drawn from the test cell.

10.7 Electrical Power in Practical Circuits

Ptotal = Iε = I2(R+r)
Pload = IVR = I2R
Pinternal = IVr = I2r
Pout = ε2R/(R+r)2

Power delivered to the external load is maximum when R = r, giving Pmax = ε2/(4r).

Concept check: Kirchhoff's laws are conservation laws

Kirchhoff's first law is conservation of charge: charge cannot accumulate at a junction in a steady circuit. Kirchhoff's second law is conservation of energy: the total energy supplied per unit charge around a complete loop equals the total energy transferred per unit charge.

Internal resistance represents energy transferred inside a source. When current increases, the lost volts Ir increase, so terminal p.d. falls. A potential divider is useful because the output p.d. is a fraction of the supply determined by the resistance ratio; changing a sensor resistance changes that fraction.

10.8 Terminal p.d. and Internal Resistance

e.m.f. is energy transferred per unit charge around the whole circuit. Terminal p.d. is energy per unit charge across the external load only. V = εIr, so V falls as current rises. A graph of V against I has intercept ε and gradient −r.

10.9 Null Methods

A potentiometer compares p.d.s. At the balance (null) length the galvanometer reads zero, so no current is drawn from the unknown — the comparison is made at infinite resistance. Thermistors and LDRs in a potential divider make the output p.d. depend on temperature or light.

11Particle Physics

Nuclear atom, radioactivity, beta decay, quarks, leptons, antiparticles and the Standard Model basics required for AS.

11.1 Nuclear Atom

Tiny dense positive nucleus (protons + neutrons) surrounded by electrons. Evidence: Rutherford α-scattering (most pass through; few deflected; very few bounce back).

11.2 Notation

AZX: A = nucleon number, Z = proton number.

Isotopes: same Z, different A.

11.3 Fundamental Particles

Fundamental particles have no known internal structure. In the AS course, the required matter particles are quarks and leptons.

Every particle has an antiparticle with the same mass and opposite charge, e.g. electron / positron, proton / antiproton.

For 9702 AS, focus on matter and antimatter particles, quarks, leptons and hadrons. Detailed force-carrier particles and the Higgs boson are not required.

11.4 Radioactive Emissions

TypeIdentityChargeMass (u)Penetration
α42He nucleus+2e≈ 4Few cm air, stopped by paper
β-Fast electron-e≈ 0~1 m air, few mm Al
β+Positron+e≈ 0Annihilates with electron → 2γ
γEM photon00Reduced by Pb/concrete

11.5 Beta Decay

β- decay: a neutron changes into a proton, electron and electron antineutrino.

10n11p + 0-1e + 00νe
du + e- + νe

β+ decay: a proton changes into a neutron, positron and electron neutrino.

11p10n + 0+1e + 00νe
ud + e+ + νe

11.6 Quark Model

Six quark flavours: u, d, s, c, t, b. Charges: u, c, t have +2/3e; d, s, b have -1/3e.

Quarks are affected by the strong force and cannot be isolated individually.

Baryons = 3 quarks, e.g. proton = uud, neutron = udd. Mesons = quark + antiquark.

11.7 Leptons and Nuclear Forces

Leptons come in six types: e, μ, τ, νe, νμ, ντ. Charged leptons have charge -e; neutrinos are neutral and interact only through the weak interaction (and gravity).

Strong force acts on quarks and hadrons, not leptons; it is short-ranged but very strong. Weak force acts on both quarks and leptons and is responsible for beta decay.

The strong interaction binds quarks into hadrons and holds hadrons close together inside nuclei; its range is about 10-15 m. The weak interaction has a still shorter range, about 10-17 m, and can change quark flavour during beta decay.

11.8 Useful Constants

1 u = 1.66 × 10-27 kg ≈ proton mass; e = 1.60 × 10-19 C; 1 eV = 1.60 × 10-19 J.

Concept check: conservation rules organise particle physics

In every nuclear or particle equation, conserve nucleon number, charge, lepton number and energy. An emitted beta particle alone cannot account for the observed energy and momentum distribution, which is why a neutrino or antineutrino is included.

Do not confuse a nucleus with an atom: an atom includes electrons, whereas nuclear notation counts protons and neutrons only. Radioactive emission is random for one nucleus; the predictable behaviour of a sample appears only when very many nuclei are considered.

11.9 Discrete α Energies and Continuous β Spectra

α-particles from a given decay have discrete kinetic energies (two-body decay to a definite daughter). β-particles share energy with an (anti)neutrino, so their spectrum is continuous up to a maximum. β produces an electron antineutrino; β+ produces an electron neutrino.

11.10 Writing Decay Equations

Nucleon number and charge are conserved. Example: 238U → 234Th + 4He. Use the unified atomic mass unit u when masses are given.