C.3 Wave phenomena
IB Physics HLΒ· Theme C: Wave Behaviour, C.3 Wave phenomenaΒ· 20 min read
1. Standing Wavesβ β ββββ± 5 min
Standing Wave
A stationary wave pattern formed by the superposition of two identical waves travelling at the same speed in opposite directions. Nodes and antinodes remain in fixed positions, with no net propagation of energy.
Example:
An incident wave reflected off a fixed string end interferes with the original wave to form a standing wave.
Standing wave harmonics depend on boundary conditions: fixed boundaries produce nodes, open boundaries produce antinodes. Key harmonic formulas are:
String of length fixed at both ends / pipe open at both ends: ,
Pipe of length closed at one end: , (only odd harmonics)
A 1.2 m long pipe closed at one end has a fundamental frequency of 70 Hz. Calculate the speed of sound in air.
- 1
The fundamental frequency is the first harmonic, so for a closed pipe:
- 2
- 3
Use the universal wave equation :
- 4
2. Single-slit Diffractionβ β β βββ± 5 min
Diffraction describes the spreading of waves when they pass through an aperture. A single narrow slit produces a diffraction pattern with a wide, bright central maximum, and smaller dimmer maxima on either side. Minima occur where destructive interference cancels the wave.
Single-slit Diffraction Minima
The condition for the first minimum (edge of the central maximum) is , where is slit width, is the angular position of the minimum, and is wavelength. For small angles where is distance from the central maximum on the screen, and is distance from slit to screen.
550 nm monochromatic light is incident on a 0.1 mm wide single slit. The distance from the slit to the screen is 2.5 m. Calculate the width of the central maximum.
- 1
Convert all values to SI units:
- 2
- 3
Use small angle approximation to find the angle of the first minimum:
- 4
- 5
The width of the central maximum is twice the distance from the centre to the first minimum ():
- 6
3. Two-source Interferenceβ β β βββ± 5 min
Two coherent wave sources produce a stable interference pattern of bright (constructive) and dark (destructive) fringes on a distant screen. The fringe separation depends on wavelength, slit separation, and distance to the screen.
Two-source Interference Conditions
For coherent sources separated by distance : constructive interference (bright fringe) when path difference = , ; destructive interference (dark fringe) when path difference = . Fringe separation (distance between adjacent bright fringes) is .
Two slits separated by 0.2 mm are illuminated with 600 nm light. The screen is 3.0 m from the slits. Find the separation between adjacent bright fringes.
- 1
Convert to SI units:
- 2
- 3
Substitute into the fringe separation formula:
- 4
4. Rayleigh Criterion for Resolutionβ β β β ββ± 5 min
Resolution is the ability of an imaging system to distinguish two adjacent point sources as separate objects. If the diffraction patterns of the two sources overlap too much, they appear as a single blurred source.
Rayleigh Criterion
Two point sources are just resolvable when the central maximum of the diffraction pattern of one source coincides with the first minimum of the diffraction pattern of the second source. For a circular aperture, the minimum angular separation (in radians) is , where is the aperture diameter.
The human eye has an aperture diameter of 2 mm in bright light. Estimate the minimum angular separation that can be resolved for 550 nm visible light.
- 1
Convert values to SI units:
- 2
- 3
Apply the Rayleigh criterion for a circular aperture:
- 4
5. Common Pitfalls
Wrong move:
Using the 1.22 factor for single slit resolution
Why:
The 1.22 factor is only required for circular apertures, not rectangular single slits
Correct move:
Use without the 1.22 factor for non-circular apertures
Wrong move:
Forgetting to double the distance to get the full width of the central maximum in single slit diffraction
Why:
The formula gives the distance from the central maximum to the first minimum, not between the two outer minima
Correct move:
Multiply the distance from centre to first minimum by 2 to get the full central width
Wrong move:
Using the open pipe wavelength formula for closed pipes
Why:
Closed pipes have a node at the closed end and antinode at the open end, so only odd harmonics exist
Correct move:
For closed pipes, use where
Wrong move:
Mixing up (slit width) and (slit separation) between single and double slit formulas
Why:
Students often swap the variables, leading to incorrect calculations
Correct move:
Single slit width = , two-slit separation = ; always confirm which variable you need for the formula
Wrong move:
Claiming standing waves transfer energy along the medium
Why:
Standing waves are stationary, so no net energy propagation occurs
Correct move:
Energy is stored between nodes and does not travel along the standing wave
6. Quick Reference Cheatsheet
Concept | Key Formula | Notes |
|---|---|---|
Standing wave (string/open pipe) | , | Fixed ends = nodes |
Standing wave (closed pipe) | , | Only odd harmonics |
Single slit 1st minimum | Central width = | |
Two-slit fringe separation | = slit separation | |
Rayleigh (circular aperture) | Omit 1.22 for single slit |
7. Frequently Asked
Is the Rayleigh criterion formula given in the data booklet?
Yes, but you must remember that the 1.22 factor only applies to circular apertures (eyes, telescopes, cameras) and not rectangular single slits.
When this came up on past exams
AI-estimated based on syllabus patterns β cross-check with official past papers for accuracy. Use only as revision-focus signals.
- 2025 Β· Paper 1
Rayleigh criterion calculation
- 2024 Β· Paper 2
Standing waves in closed pipes
- 2023 Β· Paper 1
Single slit diffraction width
- 2022 Β· Paper 2
Two-source interference problem
Going deeper
What's Next
This sub-topic builds core wave behaviour concepts that are the foundation for further topics including the Doppler effect and thin film interference, which extend the superposition, path difference and diffraction principles you learned here. Understanding the Rayleigh criterion for resolution is also key for astronomy and imaging technologies that appear in IB Physics HL option topics. Mastering standing waves, interference and diffraction here will make these more advanced follow-on topics much more intuitive and easier to solve problems for.
