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CIE 9702 Physics · AS · Topic 8

Superposition

Clear, syllabus-mapped CIE 9702 Physics revision notes on superposition: explanations, worked examples and exam technique, then a free targeted practice drill.

CIE 9702 PhysicsASFree revision notes
Contents: 7 sections

Syllabus points

The principle of superposition

When two or more waves meet at a point, the resultant displacement is the vector sum of the individual displacements.

Everything in this chapter is that one sentence applied to different situations. Note that it is displacements that add, not intensities or amplitudes, and that displacement has a sign, so waves can cancel.

Stationary waves

A stationary wave forms when two waves of the same frequency and amplitude travel in opposite directions and superpose. In practice this is a wave and its own reflection.

The distance between adjacent nodes is λ/2, so the wavelength is twice the node spacing. Reading the node spacing as the wavelength halves every answer that follows, and it is the most common error in the topic.

Stationary against progressive

ProgressiveStationary
EnergyTransferred along the waveStored, not transferred
AmplitudeSame for all particlesVaries from zero at a node to a maximum at an antinode
PhaseChanges continuously along the waveParticles between two nodes are all in phase; particles either side of a node are in antiphase
WaveformMoves alongDoes not move

The phase row is worth learning as written. Between two nodes every particle reaches its maximum at the same instant, so they are in phase despite having different amplitudes, and everything on the far side of a node is exactly half a cycle behind.

Harmonics on a string

A string fixed at both ends has a node at each end.

For a pipe closed at one end, there is a node at the closed end and an antinode at the open end, so the fundamental has L = λ/4 and only odd harmonics exist.

Diffraction

Diffraction is the spreading of a wave as it passes through a gap or around an obstacle.

The amount of spreading depends on the ratio of the wavelength to the gap width. The spreading is greatest when the gap is comparable to the wavelength. A gap much wider than the wavelength produces almost no spreading.

This is why sound diffracts around a doorway but light does not: the doorway is comparable to the metre-scale wavelength of sound and enormous compared with the 10⁻⁷ m wavelength of light.

Diffraction changes neither the wavelength nor the frequency nor the speed. Only the direction of travel and the amplitude change.

Two-source interference

For a stable interference pattern the sources must be coherent: they must have a constant phase difference, which requires the same frequency. In practice this is achieved by using a single source and splitting it, which is what the double slit does.

Similar amplitudes are needed for good contrast, so that the destructive minima are close to zero.

The conditions at a point:

The double slit

λ = ax / D

where a is the slit separation, x is the fringe spacing, and D is the slit-to-screen distance.

Read the symbols carefully: a is the separation of the slits and x is the separation of the fringes, and swapping them is a common slip because both are called "the spacing" in conversation.

Rearranged as x = λD / a, the equation says what happens when something is changed:

Worked example. Light of wavelength 600 nm falls on slits 0.50 mm apart. The screen is 2.0 m away. What is the fringe spacing?

x = λD / a = (600 × 10⁻⁹ × 2.0) / (0.50 × 10⁻³) = 2.4 × 10⁻³ m, or 2.4 mm.

The diffraction grating

d sin θ = nλ

where d is the grating spacing, the distance between adjacent lines, and n is the order.

If a grating is quoted as having N lines per metre, then d = 1/N. For 500 lines per mm, d = 1 / (500 × 10³) = 2.0 × 10⁻⁶ m. Missing the conversion from lines per millimetre to lines per metre is the standard error.

Because sin θ can never exceed 1, the maximum order visible is the largest integer n for which nλ/d ≤ 1. Questions ask how many orders are seen, and the answer is 2n + 1 counting both sides and the central maximum.

A grating gives sharper and brighter maxima than a double slit, because many slits contribute, which is why it is used for measuring wavelengths.

With white light the central maximum is white, because all wavelengths have zero path difference there. Every other order is spread into a spectrum, with red deviated most because it has the longest wavelength. That is the opposite of a prism, where red is deviated least, and the pair is worth remembering together.

Common mistakes

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