Sound as a Longitudinal Mechanical Wave

Ring a bell inside a sealed glass jar and it clangs as loud as ever. Now pump the air out of the jar and keep ringing. The clapper still strikes; you can see it hammering the metal. But the sound fades to nothing — a bell going through every motion of ringing in total silence. Robert Boyle watched exactly this in about 1660, and it is the sharpest demonstration in all of physics of what sound really is: not a thing that travels through space, but a disturbance that travels through matter. Take the matter away and there is nothing left to disturb. That single experiment fixes the entire nature of sound. It is a mechanical wave — it needs a medium, a material to carry it, exactly as ripples need water. And it is a longitudinal wave — the air does not heave up and down across the direction the sound travels, the way a plucked string does; it surges back and forth along that direction, bunching up into compressions where the pressure spikes and thinning into rarefactions where it dips. A sound wave is, at bottom, a travelling pattern of pressure, and your eardrum is a pressure sensor reading it off. This article builds that picture properly. Why sound in air or water can only be longitudinal, never transverse. Why a vacuum is silent. How the frequency you hear and the wavelength in the air are locked together by v=fλv = f\lambda, so that the note middle-A is a ripple about 78 cm78\ \mathrm{cm} long and the highest note you can hear is smaller than a grain of rice. And the subtle, exam-favourite fact that the pressure wave and the displacement wave, though they are the same sound, peak a quarter-cycle apart. Everything the rest of this chapter does — speed, loudness, echoes — stands on this one idea: sound is matter, pushed.

Key takeaways
  • Sound is a mechanical wave: it needs a material medium, and a vacuum carries no sound (the bell in the evacuated jar falls silent).
  • It is longitudinal — the medium oscillates along the direction of travel, making compressions (high pressure and density) and rarefactions (low), so sound is a travelling pressure wave.
  • Frequency and wavelength are tied by v=fλv = f\lambda; at v=343 m/sv = 343\ \mathrm{m/s} (air at 20 ∘C20\ \mathrm{^\circ C}), a 440 Hz440\ \mathrm{Hz} note has λ≈0.78 m\lambda \approx 0.78\ \mathrm{m}.
  • The audible band 20 Hz20\ \mathrm{Hz} to 20 kHz20\ \mathrm{kHz} spans wavelengths from 17 m17\ \mathrm{m} down to under 2 cm2\ \mathrm{cm} — a frequency ratio of 10001000, about ten octaves.
  • A fluid (gas or liquid) has no shear stiffness, so it can carry only a longitudinal wave through its bulk — never a transverse one.
  • The pressure wave is a quarter-cycle out of step with the displacement wave: pressure peaks where particle displacement is momentarily zero.
  • Key idea: sound is a longitudinal mechanical wave — a travelling pattern of compressions and rarefactions in a material medium — and with no medium there is nothing to compress and no sound.
The core insight

Sound is a longitudinal mechanical wave: a vibrating body pushes the surrounding medium into alternating compressions and rarefactions that travel outward as a pressure wave, obeying v=fλv = f\lambda, and because the wave is the motion of matter it cannot exist in a vacuum.

Where this lives today

That sound is a mechanical wave in a medium is not a historical curiosity — it is the working principle of a vast amount of technology. A microphone is a pressure sensor: a thin diaphragm that the compressions and rarefactions push in and out, turning the pressure wave into an electrical one; a loudspeaker runs the same idea backwards, its cone shoving the air into compressions on command. Because sound needs a medium, engineers control it by controlling the medium — double glazing traps a layer of air (or better, a partial vacuum) to starve the wave of a path, and the silence of the near-vacuum in space is why spacecraft communicate by radio, which is electromagnetic and needs no medium, not by sound. Medical ultrasound, sonar, seismology and non-destructive testing of metals all send longitudinal pressure waves into a material and read what comes back, and every one of them depends on the fact this article establishes: a sound wave is matter being pushed, and its speed, wavelength and behaviour are set by the medium it travels through. The next article asks the obvious next question — exactly how fast does that push travel, and why did Newton get it wrong.

The physical picture

Every sound begins with something that vibrates — a guitar string, a drumhead, your vocal folds, the paper cone of a loudspeaker. As the surface swings forward it shoves the air molecules just ahead of it together, making a thin shell of slightly higher pressure: a compression. As it swings back it leaves a little more room, and the molecules spread out into a shell of slightly lower pressure: a rarefaction. Vibrate steadily and you launch a marching train of compressions and rarefactions, each one handed outward from molecule to molecule. That travelling pattern is the sound. The crucial word is longitudinal. Watch a single air molecule as the wave goes by and it does not travel with the sound — it jiggles a tiny distance back and forth along the same line the wave is moving, then returns, like one person in a stadium wave who only stands and sits while the wave sweeps around the ground. The molecule carries energy forward but goes nowhere itself; even for a painfully loud sound its to-and-fro is only a few micrometres, millionths of a metre. Contrast a wave on a string, where each bit of string moves across the direction of travel — that is a transverse wave. Sound in air is the other kind, and the difference is not cosmetic: it is forced by the medium, as the derivation below shows.

Figure
A longitudinal sound wave drawn as bands of crowded and spread-out air, one particle oscillating back and forth along the line of travel, with the matching pressure graph showing a compression as a pressure peak and a rarefaction as a pressure trough
Sound is a longitudinal wave — compressions and rarefactions travelling through the air compression rarefaction compression one particle: oscillates ALONG the line of travel wave high P P₀ low P pressure graph: compressions are pressure peaks, rarefactions are pressure troughs

Frequency, wavelength and the wave speed

A steady sound has a frequency ff — how many compressions pass your ear each second, in hertz — and a wavelength λ\lambda — the distance from one compression to the next. They are not independent: in the time of one full vibration, one period T=1/fT = 1/f, the wave advances by exactly one wavelength. Distance over time is speed, so

v=fλ(1)v = f\lambda \qquad (1)

where: vv is the speed of sound in the medium (a property of the medium, not of the source), ff the frequency set by the vibrating source, and λ\lambda the wavelength in that medium. Read it as a partnership: the source fixes ff, the medium fixes vv, and λ\lambda is whatever it must be to satisfy the equation. Rearranged,

λ=vf.(2)\lambda = \frac{v}{f}. \qquad (2)

Take air at 20 ∘C20\ \mathrm{^\circ C}, where the speed of sound is v=343 m/sv = 343\ \mathrm{m/s} (the next article derives that number; here we simply use it). The orchestra's tuning note, AA above middle C at f=440 Hzf = 440\ \mathrm{Hz}, has a wavelength λ=343/440=0.780 m\lambda = 343/440 = 0.780\ \mathrm{m} — about 78 cm78\ \mathrm{cm}, roughly the length of your arm. The very lowest note a human can hear, 20 Hz20\ \mathrm{Hz}, stretches to λ=343/20=17.15 m\lambda = 343/20 = 17.15\ \mathrm{m}, longer than a bus; the very highest, 20 kHz20\ \mathrm{kHz}, shrinks to λ=343/20000=0.01715 m\lambda = 343/20000 = 0.01715\ \mathrm{m}, about 1.7 cm1.7\ \mathrm{cm} — smaller than a grain of rice. That the whole world of audible sound lives between wavelengths of 17 m17\ \mathrm{m} and 2 cm2\ \mathrm{cm}, a frequency ratio of 20000/20=100020000/20 = 1000 — close to ten octaves, since 210=1024≈10002^{10} = 1024 \approx 1000 — is worth pausing on. Notice too that higher frequency always means shorter wavelength at fixed speed: ff and λ\lambda trade off inversely. Now the demonstration that pins down "mechanical." Because the wave is the compression and stretching of a medium, it cannot exist where there is no medium to compress. Seal a ringing bell in a jar and pump the air out, and the sound dies even as the clapper keeps striking — light still crosses the vacuum, so you see the bell ring, but no sound crosses it. This is not a quirk of bells; it is the deepest fact about sound.

Figure
A bell ringing inside a glass jar is loud while the jar holds air, but as a pump removes the air the sound fades to silence even though the clapper still strikes, because a vacuum has no medium to carry the compressions
The bell in a vacuum — take the air away and the sound goes with it jar full of air LOUD jar evacuated ∅ SILENT to pump clapper still strikes in both — you SEE the bell ring, but hear nothing

Pressure and displacement: the same sound, a quarter-cycle apart

There are two honest ways to draw a sound wave, and confusing them is a classic exam slip. One graph plots the displacement of the air particles — how far each has jiggled from its rest position. The other plots the pressure (or equivalently the density) — how squeezed the air is at each point. They describe the identical wave, yet their peaks do not line up. They are a quarter of a cycle out of phase. The reason is pure geometry, no calculus needed. A compression is where air has piled up — and air piles up at a place where the particles on its left have pushed to the right while the particles on its right have pushed to the left, converging from both sides. At that exact spot the particles have met and, for the instant, their own displacement is zero. So the pressure is highest precisely where the displacement is zero. Conversely, where particles are displaced most from home, they are all moving together in the same direction, neither piling up nor spreading out, so the pressure there is momentarily back to normal. Maximum pressure sits at zero displacement; maximum displacement sits at zero pressure change — the two waves are offset by a quarter wavelength, which is a quarter-cycle, or 90∘90^\circ. It is one wave described two ways, and knowing which one a graph shows is often the whole of a JEE or NEET question.

Derivation AWhy sound in a fluid can only be longitudinal

The goal is to explain, from the mechanical properties of matter, why sound in air or water is always longitudinal and never transverse — a fact students usually just memorise. The strategy is to ask what kind of stiffness a wave needs in order to exist, and then to notice that a fluid has one kind and lacks the other. A wave is a disturbance that a medium resists and springs back from; the type of resistance decides the type of wave.

Step 1. Identify the two ways a material can resist deformation. It can resist being compressed — squeezed into a smaller volume — and this stiffness is the bulk modulus; every ordinary material has it. It can also resist being sheared — layers sliding sideways past one another — and this stiffness is the shear modulus.

Step 2. Note what a transverse wave demands. In a transverse wave the medium is displaced sideways relative to the direction of travel, so neighbouring layers slide past each other. Restoring that sideways slide, and springing back, requires shear stiffness. A transverse mechanical wave can travel only through a medium with a non-zero shear modulus.

Step 3. Note what a longitudinal wave demands. In a longitudinal wave the medium is alternately squeezed and stretched along the direction of travel. Restoring that requires compressive stiffness — a bulk modulus — and nothing else.

Step 4. Apply it to a fluid. A gas or a liquid flows freely: it offers essentially no resistance to shear (its shear modulus is zero — that is what "fluid" means), but it stoutly resists compression (its bulk modulus is large). So a fluid cannot carry a transverse wave through its bulk, but it readily carries a longitudinal one. Sound in air and water is therefore longitudinal, full stop. A solid, having both stiffnesses, can carry both kinds — which is why an earthquake sends a fast longitudinal P-wave and a slower transverse S-wave through rock, and the S-wave, needing shear, dies in the liquid outer core. Verified: this derivation is qualitative and introduces no new numbers; the wavelengths it refers to are checked in verify_hs2-nature-of-sound.py.

Go deeper · Derivation B · 1 minThe pressure wave lags the displacement wave by a quarter-cycle
Derivation BThe pressure wave lags the displacement wave by a quarter-cycle

Here we justify the exact quarter-cycle offset between the pressure and displacement pictures of one sound wave, using only where the air piles up — no calculus. The goal is to convince you that the pressure maxima fall at the displacement zeros, so that you never again line the two graphs up on top of each other. The strategy is to track, at a frozen instant, where particles are converging and where they are merely displaced.

Step 1. Draw the displacement pattern at one instant: some particles pushed right, some pushed left, in a smooth wave. Mark a point CC where particles just to its left are displaced right (toward CC) and particles just to its right are displaced left (toward CC). Air is streaming into CC from both sides.

Step 2. Read off the pressure at CC. Air crowding in from both sides makes CC a compression — maximum pressure. But the particle at CC sits between a right-pusher and a left-pusher that cancel, so its own displacement is essentially zero. Hence: maximum pressure occurs at zero displacement.

Step 3. Now find a point DD of maximum displacement, where every nearby particle is shifted the same way, say all to the right. Since neighbours move together, none is crowding onto another: the air is neither compressed nor rarefied at DD, so the pressure there is back to its ambient value. Hence: maximum displacement occurs at zero pressure change.

Step 4. Put the two together. Pressure peaks where displacement is zero, and displacement peaks where pressure is ambient — the two waves are shifted by a quarter wavelength, that is a quarter-period or 90∘90^\circ. They are the same wave seen through two different instruments: a microphone reads the pressure wave, a particle tracker would read the displacement wave, and the two never peak at the same place. Verified: the quarter-cycle offset is a geometric statement with no new numbers; the frequencies and wavelengths named alongside it are checked in verify_hs2-nature-of-sound.py.

Limiting cases

caseresultmeaning
no medium (vacuum)no sound at allnothing to compress: the bell in the evacuated jar is silent
fluid medium (gas, liquid)longitudinal wave onlyzero shear stiffness forbids a transverse wave in the bulk
solid mediumboth longitudinal and transversea solid has shear stiffness too (seismic P- and S-waves)
f=440 Hzf = 440\ \mathrm{Hz}, airλ=0.78 m\lambda = 0.78\ \mathrm{m}a middle-A ripple is about an arm's length
f=20 Hz→20 kHzf = 20\ \mathrm{Hz} \to 20\ \mathrm{kHz}λ=17.15 m→1.7 cm\lambda = 17.15\ \mathrm{m} \to 1.7\ \mathrm{cm}the audible band, a factor of 10001000 in ff and in λ\lambda
pressure versus displacementpeaks a quarter-cycle apartone wave, two graphs; a microphone reads pressure

Worked examples

Board level — the wavelength of a musical note (CBSE and IGCSE pattern)

The A above middle C has frequency 440 Hz440\ \mathrm{Hz}. Taking the speed of sound in air as 343 m/s343\ \mathrm{m/s} (air at 20 ∘C20\ \mathrm{^\circ C}), find its wavelength. What happens to the wavelength if the same note is played on a day when the air is colder and the speed of sound is lower?

Step 1. Choose the right form of the wave relation. Frequency is given, wavelength is wanted, so use equation (2), λ=v/f\lambda = v/f.

Step 2. Substitute: λ=343/440=0.780 m\lambda = 343/440 = \boxed{0.780\ \mathrm{m}}, about 78 cm78\ \mathrm{cm}. Sense-check: a mid-range musical note should have a wavelength of order a metre, and it does.

Step 3. The temperature part. The frequency is set by the vibrating source (the string or reed) and does not change with the weather. The speed falls in colder air, so by λ=v/f\lambda = v/f the wavelength gets shorter — same pitch, slightly smaller ripple. This cleanly separates what the source owns (ff) from what the medium owns (vv and hence λ\lambda).

Competitive level — the whole audible band (JEE-Main and NEET pattern)

A healthy young person hears frequencies from 20 Hz20\ \mathrm{Hz} to 20 kHz20\ \mathrm{kHz}. Taking v=343 m/sv = 343\ \mathrm{m/s}, find the range of wavelengths, the ratio of highest to lowest frequency, and roughly how many octaves that spans. Which end of the band has the longer wavelength?

Step 1. Longest wavelength comes from the lowest frequency: λmax⁡=343/20=17.15 m\lambda_{\max} = 343/20 = \boxed{17.15\ \mathrm{m}}. So the deepest audible tone is a ripple longer than a bus.

Step 2. Shortest wavelength from the highest frequency: λmin⁡=343/20000=0.01715 m=1.7 cm\lambda_{\min} = 343/20000 = 0.01715\ \mathrm{m} = \boxed{1.7\ \mathrm{cm}}, smaller than a grain of rice. The low end has the long wavelength — high frequency means short wavelength, always, at fixed vv.

Step 3. Frequency ratio: 20000/20=100020000/20 = \boxed{1000}. An octave is a doubling of frequency, so the number of octaves is the number of doublings needed to reach 1000×1000\times: since 210=1024≈10002^{10} = 1024 \approx 1000, that is about 10 octaves\boxed{10\ \text{octaves}}.

Step 4. A closing subtlety worth a mark: if a graph of this sound is shown, ask whether it plots pressure or displacement. The two are the same wave a quarter-cycle apart — pressure peaks where displacement is zero — and examiners test whether you know which is which. Timing note: about 90 seconds. Do the two divisions 343/20343/20 and 343/20000343/20000 first, then the ratio; the octave estimate is just "how many doublings reach a thousand," and 210≈10002^{10} \approx 1000 is worth memorising. Do not reach for a calculator on the octave count — recognise the power of two.

Exam traps

"Sound travels through space." It does not. Sound is mechanical and needs a medium; a vacuum is silent. The bell-in-a-jar experiment is the standard exam illustration, and the film cliché of hearing an explosion in space is the standard wrong answer. State it flatly: no medium, no sound.

Calling sound transverse. In a fluid the particles oscillate along the direction of travel, so sound in air and water is longitudinal only. The familiar sine curve is a graph of pressure or displacement against position — it is not a picture of the medium moving sideways. Reserve "transverse" for strings, water-surface ripples and light.

Confusing the pressure and displacement graphs. They are one wave shown two ways, and they peak a quarter-cycle apart: pressure (and density) is greatest exactly where particle displacement is momentarily zero. If a question gives a displacement graph and asks for the pressure, shift by a quarter wavelength — do not copy the same curve.

Thinking loud sound moves a lot of air. Loudness is about pressure amplitude, not bulk airflow. Individual molecules jiggle only micrometres even for a loud sound; the wave transports energy, not matter. "The wind from a shout" is not how sound works.

Getting v=fλv = f\lambda backwards, or forgetting whose is whose. The source sets ff; the medium sets vv; λ=v/f\lambda = v/f follows. When the medium changes (temperature, or air to water) the speed changes and so does the wavelength, but the frequency — fixed by the source — stays put. Many "what changes when sound passes from air into water" questions hinge on exactly this.

Board scope. Every board here — CBSE, ICSE, JEE-Main, NEET, IGCSE and A-Level (CIE 9702) — expects the qualitative longitudinal picture, the need for a medium, and v=fλv = f\lambda. IGCSE and 9702 own that qualitative core and stop there. The finer point that pressure and displacement peak a quarter-cycle apart is JEE and NEET level; it is not required for IGCSE.

Origins · 1 minClaude-Louis Navier and how this was discovered
CN
Claude-Louis Navier
1785–1836 · Paris

Claude-Louis Navier was a French engineer and mathematician, best known for the fluid-flow equations that carry his name, but his deeper relevance to sound lies in his 1821 continuum theory of an elastic solid. Building a material up from the forces between its molecules, Navier derived how an elastic medium stores and returns the energy of a deformation — precisely the stiffness that lets a disturbance propagate as a wave, and lets one region of matter push the next. A sound wave is exactly that: a compression handed molecule to molecule through an elastic medium, which is why, with no medium, there is nothing to compress and no wave at all. Navier did not perform the bell-in-a-vacuum demonstration — that is Boyle's — but he supplied the physics of why a medium is indispensable: the elasticity of matter is the spring on which every mechanical wave rides.

History
1638
— Galileo Galilei, in Two New Sciences, ties the pitch of a sound to the frequency of the vibration that makes it.
1660
— Robert Boyle's air-pump experiments show a bell in an evacuated jar falling silent while it still visibly rings: sound needs a material medium.
1687
— Isaac Newton, in the Principia, computes the first theoretical speed of sound in air, a result that comes out about 15 percent too low.
1821
— Claude-Louis Navier builds the continuum theory of an elastic medium from the forces between its molecules, the physics of why a disturbance propagates.
1877
— Lord Rayleigh's Theory of Sound systematises acoustics as the study of waves in elastic media, longitudinal in fluids and both kinds in solids.

Going further

Texts. NCERT Physics Class 11, Ch. 15 ("Waves"), the sections on the nature and production of sound · H. C. Verma, Concepts of Physics Vol. 1, "Sound Waves" · Cambridge IGCSE 0625 (sound: longitudinal waves, need for a medium, v=fλv = f\lambda) · CIE A-Level 9702 (progressive and longitudinal waves).

Provenance. Standard results. Recompute: λ(440)=343/440=0.780 m≈78 cm\lambda(440) = 343/440 = 0.780\ \mathrm{m} \approx 78\ \mathrm{cm}; λ(20)=343/20=17.15 m\lambda(20) = 343/20 = 17.15\ \mathrm{m}; λ(20 000)=343/20000=0.01715 m≈1.7 cm\lambda(20\,000) = 343/20000 = 0.01715\ \mathrm{m} \approx 1.7\ \mathrm{cm}; the frequency ratio 20000/20=100020000/20 = 1000 and the octave count from 210=1024≈10002^{10} = 1024 \approx 1000. All are checked in verify_hs2-nature-of-sound.py.

Prerequisites. Periodic Motion and the Definition of SHM — each air particle in a sound wave executes simple harmonic motion about its rest position. Leads to. Speed of Sound: Newton–Laplace and Factors — how fast the compressions travel, and why Newton's first estimate was 15%15\% low · Characteristics of Sound: Pitch, Loudness and Quality — turning frequency and pressure amplitude into what we actually hear.

Go deeper (UG). How a longitudinal disturbance propagates through an elastic solid, and the split into fast P-waves and slow S-waves, is developed in Elastic Waves in Solids in the university mechanics track — Navier's continuum theory made quantitative. Enrichment only; nothing here depends on it.

What is the difference between a longitudinal and a transverse wave?

In a transverse wave the medium is displaced at right angles to the direction the wave travels — a wave on a string moves along the string, but each bit of string moves up and down across it. In a longitudinal wave the medium is displaced along the direction of travel: the particles surge forward and back in the same line the wave runs, bunching into compressions and thinning into rarefactions. Sound in air and water is longitudinal. Waves on strings, ripples on water and light are transverse. The physical reason sound in a fluid must be longitudinal is that a fluid has no shear stiffness — it cannot spring back from a sideways slide — but it strongly resists compression, so only the compressional (longitudinal) wave survives.

Why can't sound travel through a vacuum, when light can?

Because they are utterly different kinds of wave. Sound is a mechanical wave: it is the compression and stretching of a material medium, so with no matter there is nothing to compress and no wave. Light is an electromagnetic wave — an oscillation of electric and magnetic fields — which needs no medium and crosses empty space happily. That is exactly why, in the bell-in-a-jar experiment, you go on seeing the bell ring (light crosses the vacuum) while you stop hearing it (sound cannot). It is also why astronauts, and characters in honest science-fiction, are silent in space and must talk by radio.

If molecules only jiggle a few micrometres, how does sound cross a room?

Each molecule barely moves — it oscillates a few millionths of a metre about its home position and stays there. What crosses the room is not the molecules but the pattern: each jiggling molecule nudges its neighbour, which nudges the next, so the compression is handed along the line at the speed of sound while every individual particle stays put. Think of a stadium wave — it sweeps right around the ground, but no spectator travels; each only stands and sits. Sound carries energy and information across the room, not air. This is why a shout does not create a draught: the wave moves, the matter does not.

What exactly is a compression and a rarefaction?

A compression is a thin region where the air (or other medium) has been momentarily squeezed together, so its pressure and density are slightly above normal. A rarefaction is the opposite: a region where the air has spread out a little, so pressure and density dip slightly below normal. A sound wave is a train of these, compression–rarefaction–compression–rarefaction, marching outward from the source. The distance from one compression to the next is one wavelength. Your eardrum feels the passing pressure highs and lows as the push and pull of the sound, and a microphone records exactly that pressure trace. The "loudness" of the sound is how far above and below normal those pressure swings go.

Why do the pressure graph and the displacement graph of a sound look shifted?

Because they measure different things about the same wave, and the two peak a quarter-cycle apart. Pressure is highest where air has piled up — and air piles up where particles are converging from both sides, which is exactly where the particle at that point has zero net displacement. So the pressure maxima sit at the displacement zeros, and the displacement maxima (where all nearby particles move together, crowding no one) sit at ordinary pressure. Shift either graph by a quarter wavelength and you get the other. In an exam, always check whether a given graph is labelled pressure/density or displacement before reading off maxima — treating one as the other is a standard trap.

Does the speed of sound depend on how loud or how high-pitched the sound is?

No — to a very good approximation the speed of sound in a given medium at a given temperature is a single number, the same for a whisper and a shout, for a deep note and a shrill one. Loudness is the amplitude of the pressure swing and pitch is the frequency; neither changes the speed. What the speed does depend on is the medium and its state: sound goes at about 343 m/s343\ \mathrm{m/s} in air at 20 ∘C20\ \mathrm{^\circ C}, faster in warmer air, and much faster in water or steel. Because vv is fixed by the medium while ff is fixed by the source, changing the pitch changes the wavelength (through λ=v/f\lambda = v/f) but not the speed. The next article works out that speed from the stiffness and density of the air.

Before this

Where this leads