Waves, Sound, and Physical Optics
What this unit covers
The topics below follow the published Physics 2 course framework for Unit 6. This unit is worth 12–15% of the exam, so budget your time against that rather than against how long the unit takes to teach.
Lessons in this unit
- Wave Properties & the Wave Equation12 min · 3 objectivesDistinguish transverse from longitudinal waves and define wave quantities · Relate wave speed, frequency, and wavelength through v = fλ · Predict how wavelength changes when frequency changes at constant speed
- Sound Waves & the Doppler Effect13 min · 3 objectivesDescribe sound as a longitudinal pressure wave and relate its properties to what we hear · Apply v = fλ to sound in air · Explain the Doppler effect for a source moving relative to an observer
- Superposition & Interference14 min · 3 objectivesApply the principle of superposition to overlapping waves · Use path difference to distinguish constructive from destructive interference · Relate the double-slit condition to bright and dark fringes
- Diffraction & the Wave Nature of Light13 min · 3 objectivesDescribe diffraction and the condition under which it is pronounced · Explain how diffraction gratings and single slits spread light · Identify interference and diffraction as evidence that light is a wave
Formulas in Unit 6
Every term in Unit 6
All 24 terms we publish for Waves, Sound, and Physical Optics, with definitions. Reading them through is the fastest way to find the ones you cannot define — then drill those in cram mode until you can produce them without the prompt.
- Double-slit interference
- d sin θ = mλ for bright fringes. Wider slit separation gives closer fringes, and longer wavelength gives wider spacing.
- Polarization
- Restricting the oscillation of a transverse wave to one plane. Proves light is transverse, since sound cannot be polarized.
- Wave equation
- v = fλ. In a given medium the speed is fixed, so raising frequency shortens wavelength.
- Transverse vs longitudinal waves
- Transverse oscillate perpendicular to travel (light, string waves); longitudinal oscillate parallel (sound). Only transverse waves can be polarized.
- Wave speed depends on the medium
- Set by the medium's properties, not the source. Changing frequency does not change speed in a given medium.
- Superposition and interference
- Overlapping waves add displacement. Constructive interference occurs when a path difference is a whole number of wavelengths, destructive at half-integer multiples.
- Standing waves on a string
- Fixed at both ends, wavelengths are 2L/n. The fundamental has one antinode; harmonics are integer multiples of the fundamental frequency.
- Standing waves in pipes
- A pipe open at both ends supports all harmonics; a pipe closed at one end supports only odd harmonics, with its fundamental an octave lower for the same length.
- Beats
- Two close frequencies produce a beat frequency equal to their difference — the effect used to tune instruments.
- Doppler effect
- Motion between source and observer shifts observed frequency: higher when approaching, lower when receding. The source frequency itself is unchanged.
- Intensity and the inverse square law
- Intensity falls as 1/r² for a point source spreading in three dimensions, so doubling the distance quarters the intensity.
- Single-slit diffraction
- a sin θ = mλ locates the DARK fringes — the opposite convention to double-slit, which is a frequent source of error.
- Diffraction and wavelength
- Spreading is significant when the aperture is comparable to the wavelength, which is why sound diffracts around a doorway and light does not.
- Thin film interference
- Reflections from the two surfaces interfere. A phase inversion occurs on reflection from a higher-index medium, and it decides which thickness gives constructive interference.
- What changes when a wave enters a new medium
- Speed and wavelength change; frequency does not, because it is set by the source.
- Reflection and phase inversion
- A wave on a string reflects inverted from a fixed end and upright from a free end. The same rule governs thin-film interference.
- Resonance
- Driving a system at a natural frequency builds large amplitude, which is how instruments amplify and how structures fail.
- Harmonics on a string
- f_n = nv/2L. The fundamental has the longest wavelength; overtones are integer multiples of it.
- Why a closed pipe sounds an octave lower
- It supports only odd harmonics and its fundamental wavelength is 4L rather than 2L, so its fundamental frequency is half that of an open pipe of the same length.
- Path difference and interference
- Constructive when the path difference is a whole number of wavelengths, destructive at half-integer multiples — provided neither wave is phase-inverted.
- Coherence
- Interference patterns require a constant phase relationship, which is why a laser or a single source split in two is used rather than two separate lamps.
- Effect of slit separation on fringe spacing
- Fringe spacing is λL/d, so wider separation gives narrower fringes and longer wavelength gives wider ones.
- Diffraction grating vs double slit
- A grating has many slits, producing much sharper and more widely separated maxima at the same angles given by d sin θ = mλ.
- Thin film thickness for constructive reflection
- Depends on whether a phase inversion occurs at each surface; with one inversion, 2t = (m + ½)λ/n gives constructive reflection.
What examiners penalize here
- When a wave passes from one medium to another, its *frequency stays the same* (set by the source), while its speed and wavelength both change. This fact underlies refraction: light slows in glass, so its wavelength shortens while its color (frequency) is unchanged.
- Doppler shorthand: approaching → higher pitch (compressed waves), receding → lower pitch (stretched waves). The dramatic drop you hear as a vehicle passes is the switch from approaching to receding at the instant it goes by.
- Convert everything to meters before using d sinθ = mλ: millimeters are 10⁻³ and nanometers are 10⁻⁹. A power-of-ten error here is the most common way to lose the double-slit point.
- Sort the evidence: interference and diffraction demonstrate light’s *wave* nature; the photoelectric effect and Compton scattering demonstrate its *particle* nature. Light is both — the exam expects you to name which experiment reveals which side.
Practice Physics 2
Our practice bank is drawn from across the whole course rather than filtered to one unit, which is closer to how the exam asks anyway — it will not tell you which unit a question is testing.
Questions about this unit
How much of the AP Physics 2: Algebra-Based exam is Unit 6?
Unit 6, Waves, Sound, and Physical Optics, is worth 12–15% of the Physics 2 multiple-choice section according to the published course framework. Across all 7 units that makes it a substantial share — heavier than an even split would give it.
What topics are covered in Physics 2 Unit 6?
Waves, Sound, and Physical Optics covers Wave properties, Sound, Interference and Diffraction. We publish 24 terms with definitions for this unit, all of them on this page.
How should I study Physics 2 Unit 6?
Read the 4 lessons below first — about 50 minutes — then drill the 24 terms in cram mode until you can produce each definition from memory rather than just recognize it. Recognition is what makes a unit feel finished when it is not. Finish with practice questions and read the explanation for every one you get right by elimination as well as the ones you miss.
All 7 units of AP Physics 2: Algebra-Based
Unit names, topics and exam weights follow the published College Board course framework for AP Physics 2: Algebra-Based. AP® is a trademark registered by the College Board, which does not endorse this site.