
Optional extension · Interactive lesson
Phase, Superposition & Coherence
Two waves arriving at one point do not average and do not compete: their displacements add. Everything interesting follows from a single number, the phase difference, and from whether that number holds still long enough to be seen.
UPII-PREFLIGHT-W.02 · Lesson 2 of 6 in this extension. Position is not a completion score.Optional extension. Use this unnumbered support sequence where your university’s syllabus or prerequisite needs require it. It is not an additional numbered unit. Optional work is not a required completion gate.
Build the model
Displacements add; the phase difference decides what the sum looks like.
The key idea
Superposition is the rule that two waves crossing at a point add their displacements, and the phase difference — how far out of step they are, in radians — decides whether that sum is larger or smaller than either wave alone.
Example. Two loudspeakers in step emit sound of λ = 0.50 m; a listener 0.25 m farther from one of them receives Δφ = 2π(0.25/0.50) = π rad, the crests of one wave arriving with the troughs of the other, and hears almost nothing.
The complete physical model and assumptions
Phase is where a point sits in its cycle, and a travelling wave carries it as φ = kx − ωt + φ₀. When two waves reach the same place the medium cannot displace twice, so the displacements add instant by instant. That is superposition, and it is not a new law: the wave equation is first power in y throughout, so any sum of solutions is a solution. Add two sinusoids of the same frequency and the algebra collapses to one statement — with the two amplitudes fixed, the resultant depends on nothing else about the waves but the phase difference between them, through AR = √(A₁² + A₂² + 2A₁A₂ cos Δφ). Geometry supplies most of that phase difference, since an extra path Δr costs 2πΔr/λ radians, and the sources supply the rest. All of interference is in those two lines. Where the model stops is coherence: Δφ has to be the same on every cycle the detector averages over. Real sources radiate in wave trains of finite length and reset their phase at random every coherence time, so the cos Δφ term averages to zero and the intensities simply add. That is why two torch bulbs never make fringes, and why a single wave has to be split and recombined within its own coherence length.
1Phase is a position in the cycle
For a sinusoidal wave travelling in the +x direction, y(x, t) = A sin(kx − ωt + φ₀), and the whole bracket φ(x, t) = kx − ωt + φ₀ is the phase: an angle in radians saying where that point of the medium sits in its cycle, with 2π rad for one complete cycle. The absolute value of φ depends on where you put the origin of x and t, so it is a bookkeeping choice. Differences are physical. At one instant, two points a distance Δx apart on the same wave differ in phase by Δφ = kΔx = 2πΔx/λ, so points one wavelength apart are in step by definition. At one point, two instants Δt apart differ by Δφ = ωΔt. Now keep the sign straight, because it is easy to talk yourself into the wrong one. A wave that has travelled farther arrives later, and with this convention its phase is the larger one: y = A sin(k(r + Δr) − ωt) = A sin(kr − ωt + kΔr), which is the same motion delayed by Δr/v. Later in time, larger in kx − ωt. Write the phase the other way round, as ωt − kx, and every one of those signs flips, so pick one convention and stay inside it.
2Path difference is where Δφ usually comes from
Two waves that leave in step and travel different distances arrive out of step purely because one had farther to go. An extra path of one wavelength puts the wave back exactly where it started in its cycle, so an extra path Δr is worth Δφ = 2πΔr/λ. Only the part beyond whole cycles matters. Take λ = 640 nm and Δr = 1.60 μm: the ratio is 1.60/0.640 = 2.50 wavelengths, so Δφ = 5π rad, which is π rad plus two full turns, and the waves arrive exactly out of step. If the sources are not themselves in step, add their phase offset: Δφ = 2πΔr/λ + Δφ₀. Two identical antennas fed by cables differing by half a period are already π rad apart before geometry contributes anything at all.
3Superposition is linearity, not a separate law
The wave equation ∂²y/∂x² = (1/v²) ∂²y/∂t² contains y only to the first power. Differentiation is linear, so if y₁ and y₂ each satisfy it, so does y₁ + y₂: the medium's response to both waves is the sum of its responses to each. Three consequences are worth naming. The displacement at a point is the algebraic sum, signs included, so a crest meeting a trough of equal size gives zero displacement there. Two pulses emerge from a crossing with their original shapes and speeds, because neither ever changed the other. And the rule has a limit: it holds while the restoring force stays proportional to the displacement. Drive the amplitude high enough — a shock wave in air, an intense beam in glass — and the medium's response bends, harmonics appear, and waves begin to affect one another.
4Adding two sinusoids: the phasor triangle
Take equal amplitudes first, and let wave 2 be the one that travelled farther, so its phase is θ + Δφ. A sin θ + A sin(θ + Δφ) = 2A cos(Δφ/2) sin(θ + Δφ/2): still a sinusoid of the same frequency, with amplitude 2A|cos(Δφ/2)| and a phase halfway between the two. The amplitude runs from 2A at Δφ = 0 down to 0 at Δφ = π. Unequal amplitudes are easiest as phasors — draw each wave as an arrow of length A whose angle is its phase, and add the arrows nose to tail. The triangle has sides A₁ and A₂ with an included angle of π − Δφ, so the cosine rule gives AR = √(A₁² + A₂² + 2A₁A₂ cos Δφ). With A₁ = 3.0 mm, A₂ = 2.0 mm and Δφ = 60°: AR = √(9.0 + 4.0 + 6.0) = 4.4 mm. Notice that only cos Δφ appears, so the sign of Δφ never matters to the amplitude — swap which wave is behind and the resultant is unchanged. Complete cancellation now needs A₁ = A₂ as well as Δφ = π; otherwise the best the waves manage is |A₁ − A₂|.
5Interference moves energy, it does not create or destroy it
Intensity goes as amplitude squared, so the cross term in AR² is the whole story: I = I₁ + I₂ + 2√(I₁I₂) cos Δφ. For two equal coherent waves this is I = 4I₀ cos²(Δφ/2). In step, the intensity is 4I₀, four times one wave and not twice, which is the first surprise. Out of step it is exactly zero, which is the second. Neither breaks conservation of energy, because the pattern has to be added up as a whole: the mean of cos² over a cycle is ½, so the average intensity across the fringes is 2I₀, exactly the I₁ + I₂ the two sources emit between them. Interference redistributes energy out of the dark fringes and into the bright ones. A detector at a dark fringe is not watching energy be destroyed; it is standing where none arrives.
6Coherence: the phase difference has to hold still
Every result above assumed Δφ is a fixed number. Real atoms radiate in wave trains lasting a coherence time τc ≈ 1/Δν, where Δν is the source bandwidth, and each new train starts at a random phase. A detector averaging over many trains sees ⟨cos Δφ⟩ = 0, the cross term vanishes, and the intensities simply add — no fringes. The path difference must therefore stay inside the coherence length Lc = cτc = λ²/Δλ. For white light near 550 nm with Δλ ≈ 300 nm, Lc ≈ 1.0 μm, a couple of wavelengths. Filter it to Δλ = 1.0 nm and Lc grows to 0.30 mm; a laboratory HeNe laser with Δν = 1.5 GHz reaches 0.20 m. In between sits partial coherence, written I = I₁ + I₂ + 2√(I₁I₂)|γ| cos Δφ, whose fringe visibility V = (Iₘₐₓ − Iₘᵢₙ)/(Iₘₐₓ + Iₘᵢₙ) equals |γ| when the two intensities match. This is why interference experiments split one beam in two rather than using two lamps.
Key equations
Read the units, assumptions and limits before substituting.
Phase of a travelling wave
φ(x, t) = kx − ωt + φ₀
Names where a point sits in its cycle; one whole cycle is 2π rad.
k = 2π/λ in rad m⁻¹, ω = 2πf in rad s⁻¹, φ₀ the source phase in radPhase difference from path difference
Δφ = 2π Δr/λ + Δφ₀
Converts a geometric length into radians: one extra λ costs 2π.
Δr the extra path in m, λ the wavelength in m, Δφ and Δφ₀ in radLinear superposition
y(x, t) = y₁(x, t) + y₂(x, t)
Add displacements, never intensities, while the medium stays linear.
displacements in m, added at the same x and the same tTwo-wave resultant, any amplitudes
AR = √(A₁² + A₂² + 2A₁A₂ cos Δφ)
The cosine rule on the phasor triangle; the cross term is the interference.
A₁, A₂ and AR in m; Δφ in rad; equal frequencies onlyTwo-wave resultant, equal amplitudes
AR = 2A |cos(Δφ/2)|
Locates the fringes at a glance: zeros at Δφ = π, 3π, 5π, …
A in m, Δφ in rad; AR runs from 2A down to exactly 0Coherence length
Lc = c/Δν = λ²/Δλ
The largest path difference that still shows fringes.
Δν the source bandwidth in Hz, Δλ the linewidth in m, Lc in mInteractive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. Hold the amplitude ratio at 1 and drag the path difference from 0 to 0.50 λ: the sum starts at twice either wave and has vanished by the end. Now keep it at 0.50 λ and dial the source phase to 180° — the cancellation turns back into reinforcement, so path difference alone never settles it.
Live results
- PATH PHASE 2πΔr/λ
- 90 °
- TOTAL PHASE Δφ
- 90 °
- RESULTANT AR
- 1.41 × A₁
- INTENSITY ÷ (I₁ + I₂)
- 1.00
Results follow this lesson’s model and assumptions. Displayed values are rounded.
Predict → change one variable → check
Plan a change before running it. Every other input stays at the saved baseline.
Saved baseline. Path difference Δr: 0.25 λ; Amplitude ratio A₂/A₁: 1.00 × A₁; Source phase offset Δφ₀: 0 °
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
The wreck is adding the wrong quantity. A detector reads intensity, so students reach for I₁ + I₂, conclude that two waves of intensity I₀ deliver 2I₀ everywhere, and then read a dark fringe as energy destroyed. Superposition is a statement about displacement: add the two y values first, get AR from the cosine rule, and square only at the end. Adding intensities is not a blunder in itself — it is exactly right for incoherent sources, where the cross term 2√(I₁I₂) cos Δφ averages away over the detector's integration time. So the question is never which formula looks familiar; it is which kind of source you have. One amplifier feeding two speakers, or one beam split and recombined inside its coherence length: add displacements. Two independent lamps, or two arms set farther apart than the coherence length: add intensities. The two routes disagree by a factor of two at a bright fringe, so the choice has to be made deliberately.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
Two dippers in a ripple tank move in step, sending out waves of wavelength 24 cm that each arrive at point P with amplitude 5.0 mm. P lies 1.44 m from one dipper and 1.98 m from the other. Find the path difference, the phase difference, and the amplitude of the water's motion at P.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- Path difference: Δr = 1.98 m − 1.44 m = 0.54 m.
- In wavelengths: Δr/λ = 0.54 m ÷ 0.24 m = 2.25, so the wave from the far dipper is two and a quarter cycles behind.
- Phase difference: Δφ = 2π × 2.25 = 4.5π rad. Only the part beyond whole cycles counts, and 4.5π − 4π = 0.5π rad, a quarter of a cycle.
- Equal amplitudes, so AR = 2A|cos(Δφ/2)| = 2(5.0 mm) × |cos 2.25π| = 10 mm × 0.7071 = 7.07 mm.
- Sense check: a quarter-cycle lag is between the two extremes, and 7.1 mm does sit between 0 and 10 mm, high up because cos falls slowly at first.
Answer. Δr = 0.54 m = 2.25λ, Δφ = 4.5π rad (a quarter cycle out of step), and the water at P oscillates with amplitude 7.1 mm.
MediumExample 2
Two speakers on a bench both emit 1.70 kHz; take the speed of sound as 340 m s⁻¹. At a microphone, speaker 1 alone gives pressure amplitude 48 mPa and speaker 2 alone gives 30 mPa. Speaker 2 stands 3.50 cm farther from the microphone, and a delay line drives it a further 90° behind speaker 1. Find the resultant pressure amplitude at the microphone.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- Wavelength: λ = v/f = 340 m s⁻¹ ÷ 1700 Hz = 0.200 m.
- Path contribution: Δφₚₐₜₕ = 2π(0.0350 m ÷ 0.200 m) = 0.350π rad = 63.0°.
- Both effects put wave 2 behind wave 1, so they add: Δφ = 63.0° + 90.0° = 153.0°, and cos Δφ = −0.8910.
- Cosine rule on the phasors: AR² = 48² + 30² + 2(48)(30)(−0.8910) = 2304 + 900 − 2566 = 638 mPa².
- So AR = √638 mPa² = 25.3 mPa.
- Sense check: 153° is most of the way to antiphase, so the pair should be quieter than speaker 1 alone — and 25 mPa is below even the 30 mPa of the weaker speaker.
Answer. AR = 25 mPa, quieter than either speaker alone, because Δφ = 153° leaves the two waves close to antiphase.
HardExample 3
A mercury lamp is filtered to a mean wavelength of 546.1 nm with linewidth Δλ = 1.2 nm and feeds a two-beam interferometer. (a) Find the coherence length and the number of fringes countable before the pattern washes out. (b) The two arms are then set to differ by 0.60 mm; say what the screen shows. (c) With the arms matched, the beams have equal intensity but the measured degree of coherence is |γ| = 0.35. Find the fringe visibility and Iₘₐₓ/Iₘᵢₙ.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- (a) Lc = λ²/Δλ = (546.1 × 10⁻⁹ m)² ÷ (1.2 × 10⁻⁹ m) = (2.982 × 10⁻¹³ m²) ÷ (1.2 × 10⁻⁹ m) = 2.49 × 10⁻⁴ m, that is 0.25 mm.
- Fringe m sits at path difference mλ, so contrast dies near m = Lc/λ = λ/Δλ = 546.1 ÷ 1.2 = 455 fringes either side of the centre.
- (b) 0.60 mm is 0.60/0.2485 = 2.4 coherence lengths, so each wave train recombines with a train that left the lamp at an unrelated moment. ⟨cos Δφ⟩ = 0, the cross term dies, and the intensities add: the screen is uniformly lit, with no fringes.
- (c) For equal intensities I = 2I₀(1 + |γ| cos Δφ), so Iₘₐₓ = 2I₀(1 + 0.35) and Iₘᵢₙ = 2I₀(1 − 0.35).
- Visibility V = (Iₘₐₓ − Iₘᵢₙ)/(Iₘₐₓ + Iₘᵢₙ) = |γ| = 0.35, and Iₘₐₓ/Iₘᵢₙ = 1.35 ÷ 0.65 = 2.1.
- Sense check: a laboratory HeNe laser with Δν = 1.5 GHz has Lc = c/Δν = 0.20 m, some 800 times this lamp's, which is why the filtered lamp needs its arms matched to a fraction of a millimetre and the laser does not.
Answer. Lc = 0.25 mm, about 455 fringes; at a 0.60 mm path difference (2.4 Lc) the fringes are gone and the field is uniform; with |γ| = 0.35, V = 0.35 and Iₘₐₓ/Iₘᵢₙ = 2.1.
Quick check
Select an answer and explain it before checking.
Review & continue
Superposition is the rule that two waves crossing at a point add their displacements, and the phase difference — how far out of step they are, in radians — decides whether that sum is larger or smaller than either wave alone.
- Explain the relationship without looking at the equation.
- Check a sign, a unit and a model assumption in your working.
- Return to the lab or worked example if a step is still unclear.
Optional supporting lessons
These chapter resources can help with earlier ideas; they are not additional required Physics II completion tasks.