Progressive Waves

Wave Properties

A progressive wave transfers energy from one place to another without transferring matter. Key properties include:

PropertySymbolUnitDefinition
AmplitudeAmMaximum displacement from equilibrium
WavelengthλmDistance between two adjacent points in phase
FrequencyfHz (s−1)Number of complete oscillations per second
PeriodTsTime for one complete oscillation
Wave speedvm s−1Speed at which the wave profile moves

The Wave Equation

v = fλ     and     T = 1f

Worked Example

A sound wave in air has a frequency of 440 Hz and a wavelength of 0.773 m. Calculate the speed of sound.

v = fλ = 440 × 0.773 = 340 m s−1

Phase Difference

Phase difference describes how much one wave is ahead or behind another. It is measured in radians or degrees.

Phase difference = 2πdλ   (in radians)    or    360° × dλ

Where d is the path difference (difference in distance travelled).

  • In phase: phase difference = 0, 2π, 4π, ... (path difference = 0, λ, 2λ, ...)
  • In antiphase: phase difference = π, 3π, ... (path difference = λ/2, 3λ/2, ...)

Key Facts

  • Progressive waves transfer energy but not matter
  • The intensity of a wave is proportional to the amplitude squared: I ∝ A2
  • Frequency is determined by the source and does not change when a wave enters a new medium

Longitudinal & Transverse Waves

Comparing Wave Types

Transverse waves: The oscillation is perpendicular to the direction of wave travel. Examples: light, water surface waves, waves on a string, all EM waves.

Longitudinal waves: The oscillation is parallel to the direction of wave travel. They consist of compressions and rarefactions. Examples: sound, ultrasound, P-waves (seismic).

Transverse Wave direction of travel A λ oscillation Longitudinal Wave direction of travel C R C R C R λ C = compression, R = rarefaction

Polarisation

Polarisation restricts the oscillations of a transverse wave to a single plane. Only transverse waves can be polarised; longitudinal waves cannot.

Evidence for polarisation proves that light is a transverse wave. Applications include Polaroid filters, LCD screens, and reducing glare.

Exam Tip

If asked to prove that a wave is transverse, show that it can be polarised. Sound cannot be polarised, confirming it is longitudinal.

Superposition & Standing Waves

Principle of Superposition

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

  • Constructive interference: Waves in phase → amplitudes add → larger resultant
  • Destructive interference: Waves in antiphase → amplitudes cancel → smaller (or zero) resultant

Stationary (Standing) Waves

A stationary wave is formed when two progressive waves of the same frequency and amplitude travel in opposite directions and superpose.

N N N N N A A A A λ/2 λ N = Node (zero displacement) A = Antinode (max displacement)

Nodes: Points of zero displacement (always stationary). Antinodes: Points of maximum displacement.

The distance between adjacent nodes (or adjacent antinodes) is λ/2.

Comparing Progressive and Stationary Waves

FeatureProgressive waveStationary wave
Energy transferTransfers energyNo net energy transfer
AmplitudeSame for all particlesVaries: zero at nodes, maximum at antinodes
PhaseChanges continuously along waveAll points between two nodes are in phase
WavelengthDistance between adjacent in-phase points2 × distance between adjacent nodes

Harmonics on a String

For a string fixed at both ends, standing waves can only form at specific frequencies (harmonics). The fundamental (1st harmonic) has one antinode.

Fundamental: L = λ2    so    f1 = v2L

nth harmonic: fn = nf1

Exam Tip

When drawing standing wave patterns, count the number of antinodes to determine the harmonic. 1st harmonic = 1 antinode, 2nd = 2 antinodes, etc.

Refraction & Diffraction

Refraction and Snell's Law

Refraction occurs when a wave crosses a boundary between two media with different wave speeds. The wave changes direction (unless it enters at the normal).

n1 sin θ1 = n2 sin θ2    (Snell's Law)

The refractive index of a material is:

n = cv

Where c = speed of light in vacuum and v = speed of light in the material. A higher refractive index means slower speed.

Total Internal Reflection

When light travels from a more optically dense medium to a less dense medium (n1 > n2), it refracts away from the normal.

At the critical anglec), the refracted ray travels along the boundary. Beyond this angle, total internal reflection occurs.

sin θc = n2n1

Applications: optical fibres, endoscopes, prisms in binoculars.

Worked Example

Calculate the critical angle for glass (n = 1.50) to air (n = 1.00).

sin θc = n2 / n1 = 1.00 / 1.50 = 0.667

θc = sin−1(0.667) = 41.8°

Diffraction

Diffraction is the spreading of waves as they pass through a gap or around an obstacle.

  • Maximum diffraction occurs when the gap width is approximately equal to the wavelength
  • If the gap is much larger than the wavelength, very little diffraction occurs
  • Single slit diffraction produces a central maximum that is twice the width of the subsidiary maxima

Key Facts

  • When light enters a denser medium, it slows down and bends towards the normal
  • Frequency does not change during refraction; wavelength and speed change
  • Total internal reflection requires: denser to less dense medium AND angle of incidence > critical angle

Young's Double Slit Experiment

The Experiment

Monochromatic, coherent light passes through two narrow slits separated by distance a. An interference pattern of bright and dark fringes appears on a screen at distance D.

Coherence means the sources have a constant phase difference and the same frequency.

The Double Slit Equation

λ = axD

Where:

  • λ = wavelength
  • a = slit separation
  • x = fringe spacing (distance between adjacent bright fringes)
  • D = distance from slits to screen

Worked Example

Light of wavelength 600 nm passes through two slits 0.50 mm apart. The screen is 1.5 m away. Calculate the fringe spacing.

Rearrange: x = λD / a

x = (600 × 10−9 × 1.5) / (0.50 × 10−3)

x = 9.0 × 10−4 / 5.0 × 10−4

x = 1.8 × 10−3 m = 1.8 mm

Conditions for Maxima and Minima

At a point on the screen, whether there is a bright or dark fringe depends on the path difference between waves from the two slits.

Fringe typePath differencePhase difference
Bright (constructive)nλ (n = 0, 1, 2, ...)0, 2π, 4π, ...
Dark (destructive)(n + ½)λπ, 3π, 5π, ...

Exam Tip

The double slit equation λ = ax/D is only valid when D is much larger than a (D >> a). Always convert units: nm to m, mm to m.

Diffraction Gratings

The Diffraction Grating Equation

A diffraction grating has many equally spaced slits. It produces sharp, bright maxima at specific angles.

d sin θ = nλ

Where:

  • d = slit spacing (distance between centres of adjacent slits)
  • θ = angle of diffraction from the central maximum
  • n = order number (0, 1, 2, 3, ...)
  • λ = wavelength

If the grating has N lines per metre, then d = 1/N.

Maximum Number of Orders

The maximum order visible occurs when sin θ = 1 (i.e., θ = 90°).

nmax = dλ   (round down to nearest integer)

Worked Example

A diffraction grating has 300 lines per mm. Light of wavelength 550 nm is incident normally. (a) Calculate the angle of the 2nd order maximum. (b) Find the total number of orders visible.

(a) d = 1 / (300 × 103) = 3.33 × 10−6 m

d sin θ = nλ

sin θ = nλ / d = (2 × 550 × 10−9) / 3.33 × 10−6 = 0.330

θ = sin−1(0.330) = 19.3°

(b) nmax = d / λ = 3.33 × 10−6 / 550 × 10−9 = 6.06

Maximum order = 6. Total maxima visible = 2 × 6 + 1 = 13 (6 on each side plus central)

Gratings vs Double Slit

Compared to the double slit pattern, a diffraction grating produces:

  • Sharper, brighter maxima (more slits contributing)
  • Wider spacing between maxima
  • More precise measurements of wavelength

Applications include spectroscopy, measuring wavelengths of light, and analysing stellar spectra.

Key Facts

  • d sin θ = nλ applies to each order of diffraction
  • White light through a grating produces spectra, with violet diffracted least and red most
  • The zero-order maximum (n = 0) is always at θ = 0 (straight through)
  • More lines per mm means greater angular separation between orders

Exam Tip

Be careful with units when calculating d. If the grating has N lines per mm, then d = 1/(N × 103) metres. A common error is forgetting the mm to m conversion.

Waves Flashcards

Click to flip. Use arrow keys to navigate, space to flip.

Waves Quiz

Test your knowledge of waves.

Waves - Mock Exam Questions

Practice exam-style questions. Write your answer, then check the mark scheme.