The Wave Model is the foundation for the entire C-block of IB Physics HL. Once you can confidently use $v = f\lambda$, distinguish transverse from longitudinal waves, and read both displacement-time and displacement-position graphs, the rest of waves (Topic C.3 wave phenomena, C.4 standing waves, C.5 Doppler) becomes a matter of applying the same core ideas in new contexts.
This cheatsheet condenses the full Topic C.2 syllabus — wave quantities, the wave equation, mechanical vs electromagnetic waves, sound, the EM spectrum, and graph interpretation — into one page you can revise from. The classic IB traps (frequency at a boundary, particle vs wave speed, polarisation) are flagged in red. Scroll to the bottom for the printable PDF and the full Photon Academy notes library.
§1 — Wave Properties & Quantities C.2 SL + HL
Core wave equation
Here $v$ is wave speed (m s$^{-1}$), $f$ is frequency (Hz), $\lambda$ is wavelength (m), and $T = 1/f$ is the period (s).
Key quantities
| Quantity | Definition |
|---|---|
| Amplitude $A$ | Maximum displacement from equilibrium. |
| Period $T$ | Time for one complete oscillation. |
| Frequency $f$ | Number of cycles per second; $f = 1/T$. |
| Wavelength $\lambda$ | Distance between two adjacent in-phase points. |
| Wave speed $v$ | Speed at which the wave pattern (energy) travels. |
§2 — Transverse vs Longitudinal Waves C.2 SL + HL
Transverse waves
- Particle motion is perpendicular to the direction of energy transfer.
- Can be polarised.
- Show crests and troughs.
- Examples: light, all EM waves, waves on a string, water surface waves.
Longitudinal waves
- Particle motion is parallel to the direction of energy transfer.
- Cannot be polarised.
- Show compressions and rarefactions.
- Examples: sound, seismic P-waves, slinky compressions.
Compressions & rarefactions
- Compression: particles closer than normal (high pressure).
- Rarefaction: particles further apart (low pressure).
- Distance between adjacent compressions $= \lambda$.
- On a displacement–position graph: C $=$ zero displacement with negative gradient; R $=$ zero displacement with positive gradient.
§3 — Sound Waves C.2 SL + HL
Nature of sound
- Sound is mechanical and longitudinal.
- Requires a material medium — cannot travel in vacuum.
- Propagates as pressure variations.
- Speed in air at 20 °C $\approx 340\ \mathrm{m\,s^{-1}}$.
- Faster in liquids and solids than in gases.
- $f$ determines pitch; $A$ determines loudness.
- Audible range $\approx 20\ \mathrm{Hz} - 20\ \mathrm{kHz}$.
Approximate sound speeds
| Medium | Speed of sound |
|---|---|
| Air (20 °C) | $\approx 340\ \mathrm{m\,s^{-1}}$ |
| Water | $\approx 1500\ \mathrm{m\,s^{-1}}$ |
| Steel | $\approx 5000\ \mathrm{m\,s^{-1}}$ |
Sound is faster in solids and liquids than in gases because the stronger intermolecular forces transmit the pressure disturbance more quickly.
§4 — Electromagnetic Waves & the EM Spectrum C.2 SL + HL
Nature of EM waves
- Transverse: oscillating $\vec{E}$ and $\vec{B}$ fields, perpendicular to each other and to the direction of propagation.
- Do not need a medium — travel through vacuum.
- All EM waves travel at $c = 3.00\times 10^8\ \mathrm{m\,s^{-1}}$ in vacuum.
- Obey $c = f\lambda$ in vacuum.
- Slow down (and wavelength shortens) in a medium, but frequency is unchanged.
The EM spectrum (low $f$ → high $f$)
| Region | Typical wavelength |
|---|---|
| Radio | $\lambda \sim 1\ \mathrm{m} - 1\ \mathrm{km}$ |
| Microwave | $\lambda \sim 1\ \mathrm{cm}$ |
| Infrared | $\lambda \sim 10\ \mathrm{\mu m}$ |
| Visible | $\lambda \sim 400 - 700\ \mathrm{nm}$ |
| Ultraviolet | $\lambda \sim 100\ \mathrm{nm}$ |
| X-ray | $\lambda \sim 0.1\ \mathrm{nm}$ |
| Gamma | $\lambda < 0.01\ \mathrm{nm}$ |
§5 — Mechanical vs Electromagnetic Waves C.2 SL + HL
| Property | Mechanical | Electromagnetic |
|---|---|---|
| Medium needed? | Yes | No |
| Wave type | Transverse OR longitudinal | Transverse only |
| Speed in vacuum | Does not propagate | $c = 3.00 \times 10^8\ \mathrm{m\,s^{-1}}$ |
| Speed depends on | Medium (density, elasticity) | Medium ($v < c$ in matter) |
| Polarisable? | Only if transverse | Yes (all EM waves) |
| Examples | Sound (L), strings (T), water (T) | Light, radio, X-rays, gamma |
§6 — Graph Interpretation C.2 SL + HL
Displacement–position graph ($y$ vs $x$)
- Snapshot of the whole wave at one instant $t$.
- Horizontal axis in metres $\Rightarrow$ read off wavelength $\lambda$.
- Vertical axis $\Rightarrow$ read off amplitude $A$.
- If the wave moves to the right, each point will next move in the direction of the point behind it.
Displacement–time graph ($y$ vs $t$)
- Motion of one particle over time.
- Horizontal axis in seconds $\Rightarrow$ read off period $T$.
- Vertical axis $\Rightarrow$ read off amplitude $A$.
- $f = 1/T$, then use $v = f\lambda$ if a wavelength is given.
§7 — Exam Attack Plan All sections
When you see this in the question — reach for that:
| Question trigger | Reach for |
|---|---|
| "Find $\lambda$, $f$ or $v$" | $v = f\lambda$ in the relevant medium. |
| "Wave enters a denser medium" | $v$ ↓, $\lambda$ ↓, $f$ unchanged. |
| "Can the wave be polarised?" | Yes only if transverse. |
| "Sound in a vacuum?" | No — sound is mechanical and needs a medium. |
| "Doubling the amplitude — what happens to intensity?" | $I \propto A^2 \Rightarrow$ × 4. |
| "Speed of light in a vacuum" | $c = 3.00 \times 10^8\ \mathrm{m\,s^{-1}}$. |
| $y$–$x$ graph reading | Read $\lambda$ from horizontal axis. |
| $y$–$t$ graph reading | Read $T$ from horizontal axis, then $f = 1/T$. |
| "Order of EM spectrum" | Radio < microwave < infrared < visible < UV < X-ray < gamma. |
| "Particle speed vs wave speed" | Particles oscillate, do not travel with the wave. |
Worked Example — IB-Style Wave Model Problem
Question (HL Paper 2 style — 6 marks)
A loudspeaker emits a sound of frequency 850 Hz into air at 20 °C, where the speed of sound is 340 m s$^{-1}$. The sound wave then enters water, where the speed of sound is 1500 m s$^{-1}$. (a) Calculate the wavelength of the sound in air. (b) State and explain what happens to the frequency as the wave enters the water. (c) Calculate the wavelength of the sound in water.
Solution
- Wavelength in air: rearrange $v = f\lambda$ to give $\lambda = v/f$. (M1)
- $\lambda_\text{air} = 340 / 850 = 0.400\ \mathrm{m}$. (A1)
- Frequency is set by the source (the loudspeaker) and is unchanged at the boundary. Only $v$ and $\lambda$ change. (R1)
- Wavelength in water with the same frequency: $\lambda_\text{water} = v_\text{water}/f$. (M1)
- $\lambda_\text{water} = 1500 / 850 = 1.76\ \mathrm{m}$ (3 s.f.). (A1)
- State: the wavelength increases because sound is faster in water and the frequency is fixed. (A1)
Examiner's note: The most common mistake is writing "$f$ also increases because the wave is faster". Frequency is set by the source — it never changes at a boundary in IB Physics. State this explicitly to score the R1 mark; otherwise the (b) part is lost.
Common Student Questions
What changes when a wave enters a denser medium?
Why can only transverse waves be polarised?
What is the difference between wave speed and particle speed?
How do I tell a displacement-position graph from a displacement-time graph?
Does intensity depend on amplitude or frequency?
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