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Theme C — Wave Behaviour

C.2.2 Transverse and Longitudinal Waves — IB Physics HL Revision Notes & Topical Questions

5 min read 11 parts Lesson 13 of 37 1 quiz

📚 IB Physics HL Hub / Topical Revision
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Curriculum Equation Key قوانين الرقم الهيدروجيني والاتزان الأيوني - pH & Acid-Base Equilibrium FormulasFast Exam Solution
pH = -log[H⁺] | pOH = -log[OH⁻] | pH + pOH = 14 | [H⁺][OH⁻] = 10⁻¹⁴
Word Equation & Conditions: الرقم الهيدروجيني = -لوغاريتم تركيز أيون الهيدروجين | pH + pOH = 14
Location & Specifications: الاتزان الأيوني، كيمياء 3 ثانوي، التحصيلي، و AP Chemistry.
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Lesson summary

C.2.2 Transverse and Longitudinal Waves — IB PHYSICS SL notes: Distinguish transverse from longitudinal waves, interpret their graphs and explain polarization of transverse waves.Classification — compare the direction in which particles or fields oscillate with the direction in w…

  • Particles stay put
  • Energy transfer
  • Compression
  • Rarefaction
  • Wavelength
  • Slinky picture

Part 1 of 9Direction of oscillation versus travel

Direction of oscillation versus travel
Classification
  • Classification compare the direction in which particles or fields oscillate with the direction in which energy travels
Particles stay put
  • Particles stay put in mechanical waves particles oscillate about fixed points and do not travel along the wave
  • All particles have the same motion but are displaced slightly in time, creating the illusion of one moving pattern.

Part 2 of 9Transverse waves

Transverse wave
  • Transverse wave a wave in which the oscillations are perpendicular to the direction of motion and energy transfer
  • Each particle vibrates up and down.
Pattern
  • Pattern crests (peaks) and troughs
Examples
  • Examples electromagnetic waves such as radio, visible light and UV,
    • and mechanical waves such as vibrations on a guitar string, a rope or approximately water ripples
Vacuum
  • Vacuum electromagnetic transverse waves need no particles, so UV from the Sun reaches us across space

Part 3 of 9Longitudinal waves

Longitudinal wave
  • Longitudinal wave a wave in which the oscillations are parallel to the direction of motion and energy transfer
  • Each particle vibrates back and forth along the line of travel.
Examples
  • Examples sound, ultrasound, compression waves in a spring and P-waves in the Earth
Medium
  • Medium they are mechanical waves and need particles, so they cannot travel through a vacuum
  • Nothing can be heard in outer space.
Energy transfer
  • Energy transfer vibrating particles pass energy to neighbours, which produces a compression further along

Part 4 of 9Compressions and rarefactions

Compression
  • Compression a region where particles are squeezed closer together, so pressure is above average
Rarefaction
  • Rarefaction a region where particles are further apart, so pressure is below average
Wavelength
  • Wavelength the distance between two successive compressions or two successive rarefactions
Slinky picture
  • Slinky picture each coil moves back and forth along the slinky while the compressions travel along it at the wave speed
  • At the centre of a compression the coil has zero displacement.
  • Coils on either side are displaced towards the centre.

Part 5 of 9Graphs of longitudinal waves

Plot
  • Plot displacement against distance, with positive displacement meaning a shift in the direction of travel
Warning
  • Warning the sine-shaped graph is not a picture of the medium; it only plots displacement against position
Compression centre
  • Compression centre the curve crosses zero going from positive to negative
Rarefaction centre
  • Rarefaction centre the curve crosses zero going from negative to positive
Pressure
  • Pressure it is a quarter of a cycle out of phase with displacement
  • Pressure is maximum at a compression centre, where the displacement is zero.

Part 6 of 9Polarization

Plane-polarized wave
  • Plane-polarized wave a transverse wave whose oscillations lie in a single plane
Unpolarized light
  • Unpolarized light light from the Sun or a lamp is a mixture of all planes perpendicular to the direction of travel
Polarizing filter
  • Polarizing filter it has a transmission axis and passes only the component of oscillation along it
Malus's law
  • I = I0 cos2θ for an ideal filter
  • I0 is the intensity of plane-polarized light incident on the filter.
  • θ is the angle between its plane of polarization and the filter axis.
  • Crossed filters (θ = 90°) transmit nothing.
Unpolarized light
  • Unpolarized light the first filter halves the intensity and makes the light polarized, then Malus's law applies
Evidence
  • Evidence only transverse waves can be polarized, which shows light is transverse and sound in air can never be polarized

Part 7 of 9Everyday cases

Glare
  • Glare light reflected from water or road is partially polarized, so polarizing sunglasses reduce it
Rotation
  • Rotation some crystals and solutions rotate the plane of polarization, which is used to study sugar concentration and stress in transparent plastics
Seismic waves
  • P-waves are longitudinal and travel through solid and liquid, while S-waves are transverse and cannot travel through liquid
  • This is how the liquid outer core of the Earth was inferred.

Part 8 of 9Transverse and longitudinal waves compared

FeatureTransverseLongitudinal
Particle motionPerpendicular to travelParallel to travel
PatternCrests and troughsCompressions and rarefactions
PolarizationPossibleImpossible
MediumMechanical ones need a medium resisting shear; electromagnetic ones need noneSolids, liquids and gases
Wave equationv = fλv = fλ

Part 9 of 9More from the specification

More from the specification
Transverse waves
  • Transverse waves oscillations are perpendicular to the direction of energy travel, as in light and water waves.
Longitudinal waves
  • Longitudinal waves oscillations are parallel to travel, forming compressions and rarefactions, as in sound.
Wave quantities
  • Wave quantities amplitude is the maximum displacement, period is the time for one cycle, and frequency is its reciprocal in hertz.
Wave equation
  • Wave equation speed equals frequency times wavelength, with wavelength measured in metres.
Electromagnetic spectrum
  • Electromagnetic spectrum transverse waves from radio to gamma that share a speed in vacuum but differ in frequency range.
Frequency
  • Revolutions per second, f = 1/T.
    What the symbols mean: T = period, the time for one complete wave (s) · f = frequency (Hz)
Period
  • Time for one revolution.
Amplitude
  • Maximum displacement from equilibrium.
Spectrum
  • Range of colours in white light.
Equilibrium
  • State with zero net force.
Equilibrium position
  • Position where the net force is zero.
Electromagnetic spectrum
  • Continuous family of waves from radio waves to gamma rays
Matter wave
  • The wave associated with a moving particle such as an electron.

Key terms

TermMeaning
Transverse waveOscillation perpendicular to the direction of energy transfer.
Longitudinal waveOscillation parallel to the direction of energy transfer.
CompressionRegion of higher-than-average particle density and pressure.
RarefactionRegion of lower-than-average density and pressure.
Polarized waveTransverse wave oscillating in one plane only.
Malus's lawI = I₀cos²θ for transmission through an ideal polarizer.

Avoid these mistakes

1
Saying sound waves are transverse — air particles oscillate parallel to the travel direction.
2
Thinking longitudinal waves cannot be drawn as sine graphs — they can, but the graph plots displacement against position.
3
Using Malus's law for unpolarized light without first halving the intensity.
4
Believing polarization applies to any wave — only transverse waves can be polarized.
5
Placing the pressure maximum at the point of maximum displacement — it is at zero displacement.

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