
Optional extension · Interactive lesson
Sound Waves & the Speed of Sound
Sound is air moving back and forth along the line of travel, and the pressure change that motion produces. The two are a quarter cycle out of step, and the speed they share belongs to the medium, not to the source.
UPI-EXT-WS.07 · Lesson 7 of 11 in this extension. Position is not a completion score.Optional extension. Use Waves & Sound only if your university includes it in Physics I. Optional work is not a required completion gate.
Build the model
Displacement and pressure, a quarter cycle apart
The key idea
A sound wave is a longitudinal disturbance in which fluid elements oscillate along the direction of propagation; the compressions and rarefactions that result travel at v = √(B/ρ), set by the medium's stiffness and density alone.
Example. At 20 °C, √(γRT/M) with γ = 1.40 and M = 28.96 g mol⁻¹ gives 343 m s⁻¹ in air. Helium, lighter and monatomic, gives 1009 m s⁻¹ — which is why a breath of it shifts vocal-tract resonances up, leaving the vocal folds' rate alone.
The complete physical model and assumptions
A sound wave is one disturbance described two ways. Fluid elements oscillate along the direction of travel by s(x, t), and because a gradient in that displacement compresses or rarefies the gas, the pressure change is Δp = −B ∂s/∂x. Differentiating a cosine gives a sine, so pressure and displacement sit a quarter cycle out of step: where the gas has moved furthest, nothing is compressed and Δp = 0. The same B that turns displacement into pressure fixes the speed, v = √(B/ρ) — stiffness over inertia, the form already met in v = √(F/μ) on a string. In a gas the compressions are far too fast for heat to escape, so the adiabatic B = γp applies and v = √(γRT/M): independent of pressure, independent of frequency, rising as √T. All of it treats a swarm of colliding molecules as a continuous medium with a local pressure and temperature, which holds because even a 20 kHz wavelength spans some 10⁵ mean free paths.
1One wave, two variables
Take a long tube of air and drive a piston back and forth at one end. Each thin slab of gas oscillates along the tube — the same axis the wave travels — and that shared axis is what makes sound longitudinal. Describe the motion by a slab's displacement from its rest position, s(x, t) = s(max) cos(kx − ωt), where x labels the slab and s is measured along x rather than across it. Slabs crowd together where neighbouring displacements converge and thin out where they diverge, so the gas alternates between compressions and rarefactions moving at speed v = ω/k. The second description is the gauge pressure Δp(x, t) = p − p₀ inside each slab. Both describe the same wave and neither is more real, but pressure is what the medium hands to a detector: an eardrum and a microphone diaphragm respond to the pressure difference across them, not to how far the air travelled. Almost every measurement of sound is therefore a measurement of Δp.
2Pressure is the displacement gradient
The bulk modulus links the two. A slab between x and x + Δx has its length changed by s(x + Δx) − s(x), so its fractional volume change is ΔV/V = ∂s/∂x, and B = −Δp/(ΔV/V) rearranges to Δp = −B ∂s/∂x. Differentiate the displacement wave: ∂s/∂x = −k s(max) sin(kx − ωt), so Δp = B k s(max) sin(kx − ωt). A cosine has become a sine. Displacement and pressure are a quarter cycle out of step in space and in time, and the reason is physical, not algebraic — where a slab has moved furthest, its neighbours have moved just as far, nothing is squeezed, and Δp = 0. With B = ρv² and ω = vk the amplitude is Δp(max) = ρ v ω s(max), which exposes how little air actually moves. The faintest audible 1 kHz tone has Δp(max) ≈ 2.9 × 10⁻⁵ Pa; with ρv = 413 kg m⁻² s⁻¹ and ω = 6.28 × 10³ s⁻¹, s(max) = 2.9 × 10⁻⁵/(413 × 6.28 × 10³) ≈ 1.1 × 10⁻¹¹ m, about a tenth of an atomic diameter.
3Speed is stiffness over inertia
Apply Newton's second law to that slab — net force from the pressure difference across its faces, mass ρA Δx — and a wave equation drops out with v² = B/ρ. The shape is the one already met on a stretched string, v = √(F/μ): a restoring stiffness above the line, an inertia below it. Nothing about the source survives, so the speed belongs to the medium. Water at 20 °C has B ≈ 2.2 GPa and ρ ≈ 998 kg m⁻³, giving v = √(2.2 × 10⁹/998) = 1.48 × 10³ m s⁻¹, over four times the speed in air. A solid needs one adjustment: in a rod narrower than a wavelength the material can bulge sideways as it is compressed, so Young modulus replaces the bulk modulus and v = √(Y/ρ). Steel with Y = 200 GPa and ρ = 7800 kg m⁻³ gives √(200 × 10⁹/7800) = 5.06 × 10³ m s⁻¹. In bulk steel the sideways bulge is blocked by the surrounding material, the effective stiffness is larger, and the longitudinal wave runs nearer 5.9 km s⁻¹.
4Adiabatic, not isothermal
Which bulk modulus belongs in √(B/ρ)? Newton assumed the compressions held ambient temperature. An isothermal ideal gas has B = p, so v = √(1.013 × 10⁵/1.204) = 290 m s⁻¹ at 20 °C — about 15 % below the measured 343 m s⁻¹, a gap that stood for a century until Laplace closed it. Compression warms a slab, and the question is whether that heat can reach the cooler rarefaction half a wavelength away before the slab expands again. Air has thermal diffusivity α ≈ 2.1 × 10⁻⁵ m² s⁻¹, so during one period of a 1 kHz tone heat diffuses roughly √(α/f) = √(2.1 × 10⁻⁸) ≈ 1.4 × 10⁻⁴ m, against a wavelength of 0.34 m. It covers about a two-thousandth of the distance required. No heat is exchanged, the correct modulus is the adiabatic B = γp, and v = √(γp/ρ) = √(1.40 × 1.013 × 10⁵/1.204) = 343 m s⁻¹ — agreement to three figures.
5What sets the speed, and what does not
Substituting p/ρ = RT/M for an ideal gas turns v = √(γp/ρ) into v = √(γRT/M), and the list of what matters shortens sharply. Pressure disappears: raise it at fixed temperature and the density rises in exact step. Sound is not slower on a mountain because the air is thin, only because it is cold. What remains is temperature, molar mass and γ. Helium at 20 °C, with M = 4.00 g mol⁻¹ and γ = 1.67, gives √(1.67 × 8.314 × 293.15/0.00400) = 1.01 × 10³ m s⁻¹, nearly three times air — breathe it and the vocal-tract resonances shift up by that factor while the folds keep vibrating at the same rate. Temperature enters under a square root, v = v₀√(T/T₀), which near room temperature is straight enough to write as v ≈ (331 + 0.60 θ) m s⁻¹ with θ in °C: 343 m s⁻¹ at 20 °C. Frequency never appears. A 20 Hz and a 20 kHz component leave together and arrive together, which is why a chord is still a chord 100 m away.
6The assumptions underneath
Every step treated the gas as a continuum carrying a local pressure, density and temperature, and every step assumed the disturbance was small. Both deserve a test. The continuum holds when a fluid element contains many molecules yet stays small against a wavelength: air at room conditions has a mean free path near 6.8 × 10⁻⁸ m, while even a 20 kHz wave has λ = 343/(2.0 × 10⁴) = 1.7 × 10⁻² m, some 2.5 × 10⁵ mean free paths. Only in rarefied gas, or at gigahertz frequencies, does that margin close and the model fail outright. Linearity is comfortable too: a very loud 1 Pa amplitude is 10⁻⁵ of atmospheric pressure, so Δp stays proportional to strain and the wave keeps its shape. Raise the amplitude to a blast wave and it does not — a compression is hotter, so locally faster, crests overtake troughs, and the front steepens into a shock. Finally, nothing here dissipates. Viscosity and conduction absorb sound roughly as f², which is why distant thunder rumbles with the crack stripped out.
Key equations
Read the units, assumptions and limits before substituting.
Pressure from displacement
Δp(x, t) = −B ∂s/∂x
A slab whose neighbours converge has ∂s/∂x < 0, so its pressure rises.
Pa; s(x, t) = s(max) cos(kx − ωt) is measured along the travel directionPressure amplitude
Δp(max) = B k s(max) = ρ v ω s(max)
Uses B = ρv² and ω = vk: the same motion at higher frequency costs more pressure.
Pa; a quarter cycle out of phase with s in both x and tSpeed in a fluid
v = √(B/ρ)
Stiffness over inertia — the same shape as v = √(F/μ) for a string.
m s⁻¹; water, B = 2.2 GPa and ρ = 998 kg m⁻³, gives 1.48 km s⁻¹Speed in an ideal gas
v = √(γp/ρ) = √(γRT/M)
Pressure cancels — raising p raises ρ in step — so only T and the gas matter.
T in K, M in kg mol⁻¹; γ = 1.40 for air gives 343 m s⁻¹ at 20 °CTemperature dependence
v = v₀√(T/T₀) ≈ (331 + 0.60 θ) m s⁻¹
The square root flattens it: near 0 °C one kelvin adds 0.61 m s⁻¹, near 40 °C only 0.57.
T in K, θ in °C; the linear form is within 0.6 m s⁻¹ of exact from −20 to 40 °CSpeed in a thin solid rod
v = √(Y/ρ)
Bulk solid is faster still, near 5.9 km s⁻¹, since sideways bulging is blocked.
Rod narrower than λ; steel, Y = 200 GPa and ρ = 7800 kg m⁻³, gives 5.06 km s⁻¹Interactive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. Push f up with s(max) held fixed and the top curve keeps its height while the bottom one grows — Δp(max) = ρvω s(max) — then warm the air instead and the whole pattern stretches, because v, and so λ, belongs to the medium. Wherever the dashed quarter-wavelength line lands, s is zero and Δp is at its peak.
Live results
- SPEED v
- 343.0 m s⁻¹
- WAVELENGTH λ
- 0.686 m
- IMPEDANCE ρv
- 413 Pa s m⁻¹
- PRESSURE Δp(max)
- 12.97 Pa
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. Frequency f: 500 Hz; Air temperature θ: 20 °C; Displacement s(max): 10.0 μm
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
Two swaps recur. The first puts the compressions where the displacement is largest; Δp = −B ∂s/∂x makes them a quarter cycle apart, so a displacement antinode is a pressure node — the reason an open pipe end is a pressure node rather than a pressure antinode. The second reads v = √(B/ρ) as "denser means faster". Density sits in the denominator: steel outruns air by a factor of 15 because it is 1.4 × 10⁶ times stiffer while only 6.5 × 10³ times denser.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
A tuning fork sounds at 512 Hz in a room at 25 °C. Find the speed of sound there and the wavelength of the note.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 3 steps revealed.
- Speed belongs to the medium, so start from temperature: v ≈ (331 + 0.60θ) m s⁻¹ with θ = 25 °C gives v = 331 + 0.60 × 25 = 331 + 15 = 346 m s⁻¹.
- Check it against the exact form: v = 331 × √(298.15/273.15) = 331 × 1.0448 = 346 m s⁻¹ — the linear rule is good to well under a metre per second here.
- Only now bring in the source: λ = v/f = 346 ÷ 512 = 0.676 m.
Answer. v = 346 m s⁻¹; λ = 0.676 m
MediumExample 2
A 1.00 kHz tone in air at 20 °C (ρ = 1.20 kg m⁻³, v = 343 m s⁻¹) has pressure amplitude Δp(max) = 28 Pa — a painfully loud 120 dB. Find the displacement amplitude, and say where in the cycle the pressure is zero.
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.
- Δp(max) = ρvω s(max), so s(max) = Δp(max)/(ρvω).
- Acoustic impedance first: ρv = 1.20 × 343 = 412 kg m⁻² s⁻¹. Then ω = 2πf = 2π × 1.00 × 10³ = 6.28 × 10³ s⁻¹.
- s(max) = 28 ÷ (412 × 6.28 × 10³) = 28 ÷ (2.59 × 10⁶) = 1.1 × 10⁻⁵ m.
- Set that against λ = 343 ÷ 1000 = 0.343 m: even at 120 dB the air shifts 11 μm, about 3 × 10⁻⁵ of a wavelength.
- Δp = −B ∂s/∂x, and the gradient of a cosine vanishes at its peak, so Δp = 0 exactly where the displacement is largest — a quarter cycle from the pressure maxima.
Answer. s(max) = 1.1 × 10⁻⁵ m (11 μm); the pressure vanishes at the displacement antinodes, a quarter cycle from the pressure maxima
HardExample 3
Sound travels at 319 m s⁻¹ through argon at 20 °C. Argon's molar mass is 39.95 g mol⁻¹. Find γ for argon, and say what that value reveals about the molecule.
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.
- Rearrange v = √(γRT/M): square it to v² = γRT/M, so γ = v²M/(RT).
- SI units first: M = 39.95 g mol⁻¹ = 3.995 × 10⁻² kg mol⁻¹, and T = 20 + 273.15 = 293.15 K.
- Numerator: v²M = (319)² × 3.995 × 10⁻² = 1.0176 × 10⁵ × 3.995 × 10⁻² = 4065 J mol⁻¹.
- Denominator: RT = 8.314 × 293.15 = 2437 J mol⁻¹.
- γ = 4065 ÷ 2437 = 1.67, which is 5/3 — the monatomic value. Argon stores energy in three translational degrees of freedom and nothing else; air's diatomic molecules also rotate, which adds two more and drops γ to 1.40.
Answer. γ = 1.67, i.e. 5/3 — argon is monatomic, with no rotational modes to absorb energy
Quick check
Select an answer and explain it before checking.
Review & continue
A sound wave is a longitudinal disturbance in which fluid elements oscillate along the direction of propagation; the compressions and rarefactions that result travel at v = √(B/ρ), set by the medium's stiffness and density 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.