Describing a Wave: y(x,t), Amplitude, Wavelength & Phase

The last article gave you a wave as a picture — crests and troughs sliding along a rope. A picture is not enough to compute with. To answer where is the rope at this instant, and how fast is that bit of it moving, you need the wave written as a formula, and a wave is the first thing in physics that genuinely needs two variables at once. Its shape depends on where you look (position xx) and on when you look (time tt), so the honest object is a function of both:

y(x,t)=Asin⁡(kx−ωt+φ)y(x,t) = A\sin(kx - \omega t + \varphi)

Freeze time and it is a sine curve in space, repeating every wavelength λ\lambda. Stand at one spot and watch, and it is a sine curve in time, repeating every period TT. Same wave, two utterly different graphs — and confusing them is, by a distance, the single most expensive habit in this chapter's mark schemes. This article unpacks that one line symbol by symbol. The amplitude AA, the wave number k=2π/λk = 2\pi/\lambda, the angular frequency ω=2πf\omega = 2\pi f, and the phase constant φ\varphi each read off a different feature of the wave, and the ratio ω/k\omega/k turns out to be the wave's speed. We will learn to tell, from the sign inside the bracket alone, which way the wave travels; to compute the phase difference between any two points from how far apart they are; and — the subtlety that separates strong candidates from the rest — to keep the speed at which a rope particle whips up and down completely distinct from the speed at which the wave itself moves along. They are different numbers, often wildly different, and this article is where you learn never to confuse them.

Key takeaways
  • A wave is a function of position and time: y(x,t)=Asin⁡(kx−ωt+φ)y(x,t) = A\sin(kx - \omega t + \varphi), with AA the amplitude, kk the wave number, ω\omega the angular frequency, φ\varphi the phase constant.
  • k=2π/λk = 2\pi/\lambda (rad m⁻¹) and ω=2πf=2π/T\omega = 2\pi f = 2\pi/T (rad s⁻¹). The wave speed is v=ω/k=fλv = \omega/k = f\lambda.
  • Snapshot graph (y vs x, time frozen) shows the wavelength λ. History graph (y vs t, one point) shows the period T. Reading λ off a history graph, or T off a snapshot, is the top mark-loser.
  • The sign in the bracket sets the direction: (kx−ωt)⇒(kx - \omega t) \Rightarrow travels in +x; (kx+ωt)⇒(kx + \omega t) \Rightarrow −x.
  • Phase difference: two points a distance Δx apart differ in phase by Δφ=2π Δx/λ\Delta\varphi = 2\pi\,\Delta x/\lambda; one point at two times by Δφ=ω Δt\Delta\varphi = \omega\,\Delta t.
  • Particle speed is not wave speed. A particle's maximum speed is vp,max⁡=Aωv_{p,\max} = A\omega; the wave speed is v=ω/kv = \omega/k; their ratio is Ak=2πA/λA k = 2\pi A/\lambda, a pure number set by amplitude and wavelength.
  • Key idea: the one function y=Asin⁡(kx−ωt+φ)y = A\sin(kx - \omega t + \varphi) encodes the whole wave — every quantity you can be asked for is read straight off its four constants, provided you never mix up its space graph with its time graph, or the particle's motion with the wave's.
The core insight

Writing the wave as y(x,t)=Asin⁡(kx−ωt+φ)y(x,t) = A\sin(kx - \omega t + \varphi) lets you read amplitude, wavelength (λ=2π/k\lambda = 2\pi/k), period (T=2π/ωT = 2\pi/\omega), speed (v=ω/kv = \omega/k), direction (the sign in the bracket) and phase difference (Δφ=2π Δx/λ\Delta\varphi = 2\pi\,\Delta x/\lambda) directly off its four constants — while keeping the particle's motion (vp,max⁡=Aωv_{p,\max} = A\omega) separate from the wave's (v=ω/kv = \omega/k).

Where this lives today

Every signal you send or receive is a wave function with the numbers filled in. A radio station at 100 MHz is broadcasting y=Asin⁡(kx−ωt)y = A\sin(kx - \omega t) with ω=2π×108\omega = 2\pi \times 10^8 rad s⁻¹; your phone's modem recovers the message by tracking tiny, deliberate changes in the amplitude AA, the frequency ff or the phase constant φ\varphi — amplitude, frequency and phase modulation, the three ways to write information onto a carrier wave. The phase-difference equation (4) is the beating heart of every technology that locates things by waves: GPS compares the phase of signals from several satellites, noise-cancelling headphones generate a wave exactly π\pi out of phase with the noise (Δx=λ/2\Delta x = \lambda/2) to cancel it, and phased-array radar and ultrasound steer their beams purely by adjusting the phase constant across a row of emitters. And the split this article insists on — particle motion versus wave motion — is the same split a seismologist, an audio engineer and a fibre-optic technician all live by: the medium stays home while the pattern, and the information it carries, travels.

The physical picture

A wave lives in space and time, so a single graph can only ever show you a slice of it. There are two natural slices, and telling them apart is the whole game. Freeze time — imagine a camera flash at the instant t=t0t = t_0 — and plot the displacement yy of every particle against its position xx. This snapshot graph is a photograph of the medium's shape: a sine curve laid out in space, and the distance over which it repeats is the wavelength λ\lambda. The horizontal axis is measured in metres. Now do the opposite. Fix on one particle, at position x=x0x = x_0, and plot its displacement yy against time tt as the wave rolls past. This history graph is the story of one particle's up-and-down life: again a sine curve, but the distance over which it repeats is the period TT, and the horizontal axis is measured in seconds. Both graphs are sine curves, and to a careless eye they look identical — which is exactly the trap. One repeats in space (read off λ\lambda, in metres); the other repeats in time (read off TT, in seconds). A wave function y(x,t)y(x,t) is the single object that contains both slices at once, and everything below is bookkeeping on that object.

Figure
Left: a snapshot graph, displacement against position with time frozen — the repeat distance is the wavelength lambda, measured in metres. Right: a history graph, displacement against time at one fixed point — the repeat interval is the period T, measured in seconds. Both are sine curves; reading one for the other is the classic mark-loser.
SNAPSHOT · y vs x · time frozen HISTORY · y vs t · one point x (m) y λ (metres) repeat distance in SPACE t (s) y T (seconds) repeat interval in TIME

The wave function, symbol by symbol

y(x,t)=Asin⁡(kx−ωt+φ)(1)y(x,t) = A\sin(kx - \omega t + \varphi) \qquad (1)

where: yy is the displacement of the particle at position xx at time tt; AA is the amplitude, the greatest displacement (same units as yy); kk is the wave number; ω\omega is the angular frequency; and φ\varphi is the phase constant, which sets what the wave is doing at x=0x = 0, t=0t = 0. The whole bracket, kx−ωt+φkx - \omega t + \varphi, is the phase — the stage the oscillation has reached at that place and moment, in radians. The two structural constants are fixed by the wave's repeats in space and time:

k=2πλ (rad m−1),ω=2πf=2πT (rad s−1)(2)k = \frac{2\pi}{\lambda} \ (\mathrm{rad\,m^{-1}}), \qquad \omega = 2\pi f = \frac{2\pi}{T} \ (\mathrm{rad\,s^{-1}}) \qquad (2)

where: λ\lambda is the wavelength (m), ff the frequency (Hz), TT the period (s). Read kk as "radians of phase per metre you move" and ω\omega as "radians of phase per second you wait". A full cycle is 2π2\pi radians, so travelling one wavelength or waiting one period each advances the phase by exactly 2π2\pi — which is what equations (2) say. Note the units carefully: kk is radians per metre, not "the number of waves per metre" (that would be 1/λ1/\lambda, smaller by a factor of 2π2\pi). Combine the two and the wave's speed falls out. A crest is a point of fixed phase; for the phase kx−ωtkx - \omega t to stay constant as time passes, xx must grow at the rate

v=ωk=2πf2π/λ=fλ(3)v = \frac{\omega}{k} = \frac{2\pi f}{2\pi/\lambda} = f\lambda \qquad (3)

where: vv is the wave (or phase) speed — the speed at which a crest moves along. Equation (3) is v=fλv = f\lambda, the subject of the next article, here dropping straight out of the wave function. Notice it is ω\omega divided by kk, never multiplied: a classic slip is to write v=ωkv = \omega k, which is dimensionally wrong and can be off by orders of magnitude.

Snapshot versus history — the graph that loses the most marks

Here is the discipline, and it is worth drilling until it is automatic. When you are handed a graph, look at the label on the horizontal axis before you read anything off it. If the horizontal axis is position xx (metres), you have a snapshot — a frozen photograph of the wave in space. The repeat distance along it is the wavelength λ\lambda. You may read λ\lambda, and hence k=2π/λk = 2\pi/\lambda, but you cannot read the period or frequency from it, because time is frozen. If the horizontal axis is time tt (seconds), you have a history — the motion of one particle. The repeat interval along it is the period TT. You may read TT, and hence f=1/Tf = 1/T and ω=2π/T\omega = 2\pi/T, but you cannot read the wavelength from it, because you are standing at a single point. To get the wave speed you need one of each: λ\lambda from a snapshot and TT (or ff) from a history, combined as v=λ/T=fλv = \lambda/T = f\lambda. A graph on its own gives you only half the wave. Examiners deliberately print a history graph and ask for the wavelength, or a snapshot and ask for the frequency; the correct answer is "not obtainable from this graph alone" unless the wave speed is also supplied.

Direction — reading the sign in the bracket

The relative sign of the xx and tt terms tells you which way the wave travels, with no computation at all. Track a crest, a point of constant phase. For y=Asin⁡(kx−ωt)y = A\sin(kx - \omega t), holding the phase kx−ωtkx - \omega t constant as tt increases forces xx to increase: the crest moves toward larger xx, so the wave travels in the +x direction. For y=Asin⁡(kx+ωt)y = A\sin(kx + \omega t), holding kx+ωtkx + \omega t constant as tt increases forces xx to decrease: the wave travels in the −x direction. The rule is blunt and worth memorising: opposite signs on xx and tt mean +x; the same sign means −x. (Some books write y=Asin⁡(ωt−kx)y = A\sin(\omega t - kx), which is the same +x wave with an overall sign flip that does not move the crest anywhere — the relative sign is all that matters.)

Phase and phase difference

The phase kx−ωt+φkx - \omega t + \varphi is the wave's internal clock. Two questions come up constantly: how does the phase differ between two places at one instant, and between two times at one place? Between two points separated by Δx\Delta x, at the same instant, only the kxkx term changes, so

Δφ=k Δx=2πλ Δx(4)\Delta\varphi = k\,\Delta x = \frac{2\pi}{\lambda}\,\Delta x \qquad (4)

where: Δφ\Delta\varphi is the phase difference (rad) and Δx\Delta x the separation (m). Read it as a proportion: a full wavelength of separation is a full 2π2\pi out of step (which is the same as being in step); half a wavelength is π\pi (exactly out of phase); a quarter-wavelength is π/2\pi/2, or 90°. This one equation is the engine of every interference and standing-wave problem later in the chapter, where "path difference" is exactly this Δx\Delta x. Between two instants separated by Δt\Delta t, at the same point, only the ωt\omega t term changes:

Δφ=ω Δt=2πT Δt(5)\Delta\varphi = \omega\,\Delta t = \frac{2\pi}{T}\,\Delta t \qquad (5)

so waiting a quarter-period turns the same 90° of phase. Equations (4) and (5) are the space and time faces of the one idea: phase advances by 2π2\pi per wavelength travelled and per period elapsed.

Figure
A snapshot of one wave with two particles marked a quarter-wavelength apart. Their phases differ by 2 pi times delta-x over lambda, which for a quarter-wavelength gap is pi over 2 radians — ninety degrees, a quarter of a cycle out of step.
Phase difference from separation · Δφ = 2π Δx / λ x P Q Δx = λ/4 one wavelength λ Δx = λ/4 ⇒ Δφ = 2π(λ/4)/λ Δφ = π/2 = 90° a quarter-cycle out of step

Particle velocity is not wave speed

This is the deepest point in the article, and the one boards probe hardest. As the wave passes, each particle is doing simple harmonic motion across the wave (for a transverse wave) — the SHM of SHM Kinematics: x(t), v(t), a(t) & Phase. Its displacement swings between +A+A and −A-A, so, exactly as in SHM, its speed and acceleration peak at

vp,max⁡=Aω,amax⁡=Aω2(6)v_{p,\max} = A\omega, \qquad a_{\max} = A\omega^2 \qquad (6)

where: vp,max⁡v_{p,\max} is the greatest speed of a medium particle (m s⁻¹) — reached as it flies through its rest position — and amax⁡a_{\max} its greatest acceleration (m s⁻²), reached at the extremes of the swing. These describe the particle's motion up and down. The wave speed v=ω/kv = \omega/k is a completely separate quantity — the speed at which the crest pattern moves along. The two need not resemble each other at all; their ratio is a pure number,

vp,max⁡v=Aωω/k=Ak=2πAλ(7)\frac{v_{p,\max}}{v} = \frac{A\omega}{\omega/k} = A k = \frac{2\pi A}{\lambda} \qquad (7)

fixed entirely by how big the amplitude is compared with the wavelength. Since AA is usually far smaller than λ\lambda, the particle typically crawls up and down far more slowly than the wave races along — but crank the amplitude up and the particle can, in principle, outrun the wave. They are different animals: the medium bobs; the pattern travels. One graphical result ties them together, and you may use it as a tool. The particle's velocity equals minus the wave speed times the slope of the snapshot graph at that point, vp=−v×(slope of y vs x)v_p = -v \times (\text{slope of } y\text{ vs } x). Where the snapshot rises steeply going forward, the particle just behind is about to drop; where the snapshot is flat (a crest or trough), the slope is zero and the particle is momentarily at rest. This is justified by the geometry of a rigid shape sliding sideways — no calculus required to use it, though a slope is a calculus idea underneath.

Two derivations

Derivation ABuilding the wave function from the source's SHM and a travel delay

It is one thing to be handed y=Asin⁡(kx−ωt)y = A\sin(kx - \omega t) and another to see why a travelling wave must have that form. The goal here is to build it honestly, from nothing more than a source oscillating in simple harmonic motion and the plain fact that the disturbance takes time to travel — no wave equation, no guessing. The one idea is a time delay: a point a distance xx down the medium is simply doing what the source did, but a little later, because the disturbance had to get there first. That single insight, dressed in the SHM of SHM Kinematics, produces the whole function.

Step 1. Let the source, at x=0x = 0, oscillate in SHM: y(0,t)=Asin⁡(ωt)y(0, t) = A\sin(\omega t). (Take the phase constant to be zero for now; it just shifts the clock.)

Step 2. The disturbance travels at wave speed vv, so it reaches the point xx after a delay of x/vx/v seconds. Whatever the source was doing at time t−x/vt - x/v, the point xx is doing now, at time tt. Therefore y(x,t)=Asin⁡ ⁣(ω (t−x/v))y(x, t) = A\sin\!\big(\omega\,(t - x/v)\big) — the point simply lags the source by the travel time.

Step 3. Expand the bracket: y(x,t)=Asin⁡ ⁣(ωt−(ω/v) x)y(x, t) = A\sin\!\big(\omega t - (\omega/v)\,x\big). But ω/v=ω/(fλ)=2πf/(fλ)=2π/λ=k\omega/v = \omega/(f\lambda) = 2\pi f/(f\lambda) = 2\pi/\lambda = k, so ω/v\omega/v is exactly the wave number kk, and y(x,t)=Asin⁡(ωt−kx)y(x, t) = A\sin(\omega t - kx).

Step 4. This is a wave travelling in +x (opposite signs on xx and tt), the same physical wave as Asin⁡(kx−ωt)A\sin(kx - \omega t) up to an overall sign. Restore the phase constant to allow any starting condition and you have the general one-dimensional sinusoidal wave, y(x,t)=Asin⁡(kx−ωt+φ)y(x,t) = A\sin(kx - \omega t + \varphi) — equation (1). Every constant in it earned its place: AA from the source's amplitude, ω\omega from its frequency, kk from the travel delay, φ\varphi from where in its cycle the source began. Verified: ω/v = k for the anchor wave (40/4.0 = 10 rad m⁻¹) is recomputed in verify_hs2-describing-a-wave.py.

Go deeper · Derivation B · 1 minPhase difference from path difference
Derivation BPhase difference from path difference

Every interference problem you will ever meet — two speakers, a double slit, a thin film — reduces to one question: by how much is one wave out of step with another when they meet, given the extra distance one has travelled? The goal here is to nail the conversion from a path difference (a length, in metres) to a phase difference (an angle, in radians), because getting it is the difference between predicting a bright fringe and a dark one. The physics is only that phase advances at a steady 2π2\pi radians per wavelength.

Step 1. Take the wave y=Asin⁡(kx−ωt+φ)y = A\sin(kx - \omega t + \varphi) at one fixed instant tt, so the time term is frozen and only position matters. Two points PP and QQ sit at xPx_P and xQx_Q, a distance Δx=xQ−xP\Delta x = x_Q - x_P apart.

Step 2. Their phases are ϕP=kxP−ωt+φ\phi_P = kx_P - \omega t + \varphi and ϕQ=kxQ−ωt+φ\phi_Q = kx_Q - \omega t + \varphi. Subtract: the ωt\omega t and φ\varphi cancel, leaving Δφ=k(xQ−xP)=k Δx\Delta\varphi = k(x_Q - x_P) = k\,\Delta x.

Step 3. Substitute k=2π/λk = 2\pi/\lambda: Δφ=2πλ Δx\Delta\varphi = \dfrac{2\pi}{\lambda}\,\Delta x — equation (4). The phase difference is just the path difference measured in units of wavelengths, times 2π2\pi.

Step 4. Read the landmark cases. Δx=λ⇒Δφ=2π\Delta x = \lambda \Rightarrow \Delta\varphi = 2\pi: fully in step (constructive). Δx=λ/2⇒Δφ=π\Delta x = \lambda/2 \Rightarrow \Delta\varphi = \pi: fully out of step (destructive). Δx=λ/4⇒Δφ=π/2=90°\Delta x = \lambda/4 \Rightarrow \Delta\varphi = \pi/2 = 90°: a quarter-cycle apart. For the anchor wave (λ=0.6283\lambda = 0.6283 m) two points Δx=0.157\Delta x = 0.157 m apart give Δφ=(2π/0.6283)(0.157)=10×0.157=1.57\Delta\varphi = (2\pi/0.6283)(0.157) = 10 \times 0.157 = 1.57 rad =90°= 90° — a quarter-wavelength gap, exactly as the landmark predicts, since 0.157≈λ/40.157 \approx \lambda/4. Verified: Δφ = k Δx = 10 × 0.157 = 1.57 rad = 90° for the anchor wave is recomputed in verify_hs2-describing-a-wave.py.

Limiting cases

CaseResultMeaning
horizontal axis is xx (metres)snapshot — read λ\lambdatime is frozen; period is not obtainable
horizontal axis is tt (seconds)history — read TTone point; wavelength is not obtainable
bracket is (kx−ωt)(kx - \omega t)wave travels in +xopposite signs on xx and tt
bracket is (kx+ωt)(kx + \omega t)wave travels in −xsame signs on xx and tt
Δx=λ/2\Delta x = \lambda/2Δφ=π\Delta\varphi = \pi (antiphase)the destructive-interference condition
A≪λA \ll \lambda (usual case)vp,max⁡/v=2πA/λ≪1v_{p,\max}/v = 2\pi A/\lambda \ll 1the particle bobs far slower than the wave travels
slope of snapshot =0= 0 (crest)vp=0v_p = 0the particle is momentarily at rest at the extreme

Worked examples

Board level — decoding a wave function (CBSE/ICSE/A-Level pattern)

A transverse wave on a string is y=0.05sin⁡(10x−40t)y = 0.05\sin(10x - 40t), with all quantities in SI units. Find the amplitude, wave number, angular frequency, wavelength, frequency, period, wave speed and direction, and the maximum speed and acceleration of a string particle.

Step 1. Read the three constants straight off the bracket and prefactor: A=0.05A = 0.05 m (=5= 5 cm), k=10k = 10 rad m⁻¹, ω=40\omega = 40 rad s⁻¹. The sign is (kx−40t)(kx - 40t) — opposite signs — so the wave travels in +x.

Step 2. Wavelength and the time quantities: λ=2π/k=2π/10=0.6283 m\lambda = 2\pi/k = 2\pi/10 = \boxed{0.6283\ \mathrm{m}}; f=ω/2π=40/6.2832=6.366 Hzf = \omega/2\pi = 40/6.2832 = \boxed{6.366\ \mathrm{Hz}}; T=1/f=2π/ω=0.1571 sT = 1/f = 2\pi/\omega = \boxed{0.1571\ \mathrm{s}}.

Step 3. Wave speed — ω\omega divided by kk: v=ω/k=40/10=4.0 m s−1v = \omega/k = 40/10 = \boxed{4.0\ \mathrm{m\,s^{-1}}}. Cross-check with v=fλ=6.366×0.6283=4.0v = f\lambda = 6.366 \times 0.6283 = 4.0 m s⁻¹. Agreed.

Step 4. Particle motion, a different pair of numbers: vp,max⁡=Aω=0.05×40=2.0 m s−1v_{p,\max} = A\omega = 0.05 \times 40 = \boxed{2.0\ \mathrm{m\,s^{-1}}} and amax⁡=Aω2=0.05×1600=80 m s−2a_{\max} = A\omega^2 = 0.05 \times 1600 = \boxed{80\ \mathrm{m\,s^{-2}}}. Note the particle's top speed (2.0 m s⁻¹) is half the wave speed (4.0 m s⁻¹) — as it must be, since vp,max⁡/v=Ak=0.05×10=0.5v_{p,\max}/v = Ak = 0.05 \times 10 = 0.5.

Competitive level — phase difference and the two speeds (JEE-Main/NEET pattern)

For the same wave y=0.05sin⁡(10x−40t)y = 0.05\sin(10x - 40t) (SI): (a) find the phase difference between two points 0.157 m apart at one instant; (b) confirm the ratio of a particle's maximum speed to the wave speed; (c) state where in its cycle a particle is moving fastest.

Step 1. Part (a): use Δφ=k Δx=10×0.157=1.57 rad=90°\Delta\varphi = k\,\Delta x = 10 \times 0.157 = \boxed{1.57\ \mathrm{rad} = 90°}. Since 0.157≈λ/4=0.6283/4=0.15710.157 \approx \lambda/4 = 0.6283/4 = 0.1571 m, the two points are a quarter-wavelength apart, so a 90° phase difference is exactly right — a useful landmark to sanity-check against.

Step 2. Part (b): vp,max⁡/v=Ak=0.05×10=0.5v_{p,\max}/v = A k = 0.05 \times 10 = \boxed{0.5}. So the particle's fastest motion (2.0 m s⁻¹) is half the wave speed (4.0 m s⁻¹). This ratio is a pure number set by 2πA/λ2\pi A/\lambda; it says nothing mystical — just that this amplitude is small compared with this wavelength.

Step 3. Part (c): a particle in SHM moves fastest as it passes through its rest position (y=0y = 0), where all its energy is kinetic, and is instantaneously at rest at the crest and trough (y=±Ay = \pm A), where the snapshot slope is zero. The maximum-speed value there is the vp,max⁡=2.0v_{p,\max} = 2.0 m s⁻¹ of part (b). Timing note: about 90 seconds. The examiner's trap is to slip a unit — leaving Δx in centimetres, or reading the wave speed as ωk=400\omega k = 400 instead of ω/k=4\omega/k = 4. Write v=ω/kv = \omega/k every time, and check that a quarter-wavelength gives 90° before trusting your phase answer.

Exam traps

Reading the wrong quantity off a graph. A yy-vs-xx snapshot gives the wavelength; a yy-vs-tt history gives the period. Check the horizontal-axis label first. If asked for the wave speed from a single graph, the honest answer is "need the other quantity too" — you cannot get vv from one graph alone.

v=ωkv = \omega k instead of ω/k\omega/k. The wave speed is angular frequency divided by wave number. Multiplying gives a number with the wrong units and often a wildly wrong size (here 400 instead of 4). Memorise the division.

kk as "waves per metre". The wave number is 2π/λ2\pi/\lambda in radians per metre, not 1/λ1/\lambda. The two differ by a factor of 2π≈6.282\pi \approx 6.28 — a favourite distractor.

Setting particle speed equal to wave speed. vp,max⁡=Aωv_{p,\max} = A\omega (the particle bobbing) and v=ω/kv = \omega/k (the wave travelling) are different quantities. Their ratio is 2πA/λ2\pi A/\lambda, rarely one. Keep them in separate boxes.

Calculator in degree mode, or dropping φ\varphi. The phase is in radians; degree mode corrupts every displacement value. And if the wave is given with a phase constant, carry it — it fixes the wave's state at the origin and cannot be silently dropped.

Board scope — IGCSE. The wave function y(x,t)y(x,t) is not on the IGCSE 0625 syllabus; IGCSE stops at the wave model and v=fλv = f\lambda. If you are an IGCSE candidate, read this article for understanding, but you will only be examined on v=fλv = f\lambda and the shapes of waves, not on Asin⁡(kx−ωt+φ)A\sin(kx - \omega t + \varphi) or phase difference.

Origins · 1 minJean le Rond d'Alembert and how this was discovered
JL
Jean le Rond d'Alembert
1717–1783 · France

Found abandoned as a newborn on the steps of the Paris church of Saint-Jean-le-Rond — from which he took his name — d'Alembert rose to become one of the towering intellects of the Enlightenment, co-editor with Diderot of the great Encyclopédie and a mathematician of the first rank. In 1747 he wrote down the equation governing a vibrating string and solved it in complete generality, showing that its solution is a sum of two shapes, f(x−vt)+g(x+vt)f(x - vt) + g(x + vt) — one travelling right, one left, each rigidly carrying its form along. That was the first clear statement that a wave is a function of the combination x∓vtx \mp vt, and it is precisely why the sign inside your sin⁡(kx−ωt)\sin(kx - \omega t) decides the direction of travel. Every wave function in this article is a sinusoidal special case of d'Alembert's general travelling shape.

History
1747
— Jean le Rond d'Alembert derives the wave equation for a vibrating string and gives its general solution as f(x−vt)+g(x+vt)f(x - vt) + g(x + vt) — the first statement that a wave is a function of x∓vtx \mp vt.
1748
— Leonhard Euler extends the solution, insisting that any shape whatever, not just a neat formula, is a legitimate wave.
1753
— Daniel Bernoulli argues that every vibration of a string is a sum of simple sinusoidal modes — the seed of Fourier analysis.
1759
— Joseph-Louis Lagrange joins the "vibrating-string controversy" over what counts as an allowable function of x−vtx - vt.
1822
— Joseph Fourier proves that essentially any repeating shape can be built from sinusoids, vindicating Bernoulli's modes.

Going further

Texts. NCERT Physics Class 11, Ch. 15 "Waves", §§15.3–15.4 (the wave function, wavelength, wave number, phase) · H. C. Verma, Concepts of Physics Vol. 1, "Wave Motion and Waves on a String" · Halliday, Resnick & Walker, "Waves — I", the travelling-wave sections · Cambridge A-Level 9702 topic 7, "Waves" (graphical treatment of phase difference).

Provenance. Standard results. Recompute in `verify_hs2-describing-a-wave.py` for the anchor wave y=0.05sin⁡(10x−40t)y = 0.05\sin(10x - 40t): A=0.05A = 0.05 m; λ=2π/10=0.6283\lambda = 2\pi/10 = 0.6283 m; f=40/2π=6.366f = 40/2\pi = 6.366 Hz; T=2π/40=0.1571T = 2\pi/40 = 0.1571 s; v=ω/k=40/10=4.0v = \omega/k = 40/10 = 4.0 m s⁻¹, cross-checked as fλ=4.0f\lambda = 4.0; vp,max⁡=Aω=2.0v_{p,\max} = A\omega = 2.0 m s⁻¹; amax⁡=Aω2=80a_{\max} = A\omega^2 = 80 m s⁻²; the ratio vp,max⁡/v=Ak=0.5v_{p,\max}/v = Ak = 0.5; the delay identity ω/v=k=10\omega/v = k = 10; and the phase difference Δφ=k Δx=10×0.157=1.57\Delta\varphi = k\,\Delta x = 10 \times 0.157 = 1.57 rad =90°= 90° for Δx=0.157≈λ/4\Delta x = 0.157 \approx \lambda/4 m.

Prerequisites. Wave Motion: Transverse & Longitudinal — the crest/trough picture this article puts to an equation · SHM Kinematics: x(t), v(t), a(t) & Phase — the single-particle motion the wave is built from, and the source of vp,max⁡=Aωv_{p,\max} = A\omega. Leads to. Wave Speed: v = fλ — the medium's grip on v=ω/kv = \omega/k · the wave-equation numericals archetype, which drills reading and building y(x,t)y(x,t).

Go deeper (UG). Where the form y=f(x−vt)y = f(x - vt) comes from, and why ∂2y/∂t2=v2 ∂2y/∂x2\partial^2 y/\partial t^2 = v^2\,\partial^2 y/\partial x^2 has exactly d'Alembert's two-shape solution, is developed in The One-Dimensional Wave Equation in the university mechanics track. It is enrichment; nothing here depends on it.

Why does the wave need two variables, x and t — is one not enough?

Because a wave changes both with where you look and with when you look, and no single-variable graph can capture both. Freeze time and you get the wave's shape in space (a snapshot, giving λ); stand still and watch and you get one particle's motion in time (a history, giving T). Each is a genuine slice of the wave but only a slice. The function y(x,t)y(x,t) holds both at once: fix tt in it and you recover the snapshot, fix xx and you recover the history. That is exactly why a wave is the first object in your physics course that honestly requires a function of two variables — a still photograph and a movie of one spot are both incomplete descriptions of the same moving thing.

How can I instantly tell which way a wave is travelling?

Look at the signs of the xx term and the tt term inside the bracket. If they are opposite — as in sin⁡(kx−ωt)\sin(kx - \omega t) — the wave moves in the +x direction; if they are the same — as in sin⁡(kx+ωt)\sin(kx + \omega t) — it moves in −x. The reason is that a crest is a point of constant phase, and for the phase to stay fixed as time ticks on, xx must move the way that keeps the bracket unchanged. Do not be thrown by seeing it written sin⁡(ωt−kx)\sin(\omega t - kx): an overall sign on the whole bracket changes nothing about the direction, because it does not move the crest. Only the relative sign of xx and tt matters.

Is the wave number k the same as "the number of waves"?

No, and the name is genuinely misleading. The wave number is k=2π/λk = 2\pi/\lambda, measured in radians per metre — it is the amount of phase (in radians) the wave gets through per metre you move along it. The plain "number of waves per metre" would be 1/λ1/\lambda, which is smaller by a factor of 2π≈6.282\pi \approx 6.28. Spectroscopists do use a quantity called wavenumber defined as 1/λ1/\lambda (in cm⁻¹), which adds to the confusion, but in mechanics and in every formula on this page, kk carries the 2π2\pi. If you ever find v=ω/kv = \omega/k giving a badly wrong answer, check whether you slipped 1/λ1/\lambda in for kk.

Can a particle of the medium ever move faster than the wave itself?

Yes, in principle — and this surprises people. The particle's top speed is vp,max⁡=Aωv_{p,\max} = A\omega; the wave speed is v=ω/kv = \omega/k; their ratio is Ak=2πA/λA k = 2\pi A/\lambda. That ratio exceeds one whenever the amplitude AA is larger than about λ/(2π)\lambda/(2\pi) — a very tall, short wave. For ordinary waves the amplitude is tiny compared with the wavelength, so the particle bobs far more slowly than the wave races along (in the worked example, half as fast). But the two speeds are genuinely independent quantities, and there is no law that a medium particle cannot momentarily move faster than the pattern crossing it. They simply measure different things: one the medium bobbing in place, the other the shape travelling.

What exactly does the phase constant φ do?

It sets the clock — it fixes what the wave is doing at the origin, x=0x = 0, at the start, t=0t = 0. With φ=0\varphi = 0 the wave has y=0y = 0 at the origin at t=0t = 0 and is just starting upward; with φ=π/2\varphi = \pi/2 it starts at a crest (y=Ay = A); other values start it anywhere in between. Changing φ\varphi does not alter the amplitude, wavelength, frequency, speed or direction — it only slides the whole wave along, advancing or retarding its cycle. That is why you can often set φ=0\varphi = 0 by choosing a convenient origin, but you must keep it whenever the problem fixes the wave's state at a particular place and time, or compares two waves that start out of step.

Why is the particle velocity minus the wave speed times the slope?

Picture the snapshot as a rigid shape sliding to the right at speed vv without changing form. A moment later, the whole curve has shifted right by a tiny amount. At a fixed point xx, the new displacement is what used to sit slightly to the left — so if the curve slopes upward to the right there (positive slope), the point is about to take on the lower value that was behind it, and moves down. The steeper the slope, the faster that change; the faster the wave slides, the faster too. Put together, the particle's velocity is −v-v times the snapshot's slope: steep-and-rising means diving downward, flat (at a crest) means momentarily still. It is a picture, not a calculation — but it lets you read a particle's direction of motion straight off a snapshot graph.

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