explain the formation of a stationary wave using a graphical method, and identify nodes and antinodes

Standing (Stationary) Waves

Objective

Explain, using a graphical method, how a standing wave is produced by the superposition of two travelling waves, identify the positions of nodes and antinodes, describe the energy distribution, and relate the theory to the three canonical laboratory demonstrations required by Cambridge AS & A Level Physics (9702) syllabus.

1. Principle of Superposition

When two waves of the same frequency, amplitude and wavelength travel in opposite directions along the same medium, the resultant displacement at any point is the algebraic sum of the two incident displacements.

\[

y_1=A\sin(kx-\omega t),\qquad

y_2=A\sin(kx+\omega t)

\]

\[

\text{Resultant: }y=y1+y2

=2A\cos(\omega t)\,\sin(kx)

\]

  • Spatial factor \(\sin(kx)\) determines the pattern of nodes and antinodes.
  • Temporal factor \(\cos(\omega t)\) makes the whole pattern oscillate in time without travelling.

2. Graphical Method of Formation

The graphical method visualises the addition of the two opposite‑travelling waves at successive instants.

  1. Choose a reference instant (e.g. t = 0) and draw the first wave \(y_1\) on an \(x\)–\(y\) graph.
  2. On the same axes draw the second wave \(y_2\) travelling in the opposite direction.
  3. At each position \(x\) add the vertical displacements of the two waves to obtain the resultant \(y\).
  4. Repeat for later instants (e.g. \(t=T/4,\;T/2\)). The nodes remain fixed while the antinodes swing between \(\pm2A\).

Sketch of two opposite‑travelling sine waves and their sum at (a) \(t=0\), (b) \(t=T/4\), (c) \(t=T/2\) – the standing‑wave pattern emerges.

3. Phase Change at Boundaries

  • Fixed (rigid) boundary – the incident wave is reflected with a phase reversal of \(\pi\) (180°). The reflected wave therefore starts out of phase with the incident wave at the boundary, producing a node.
  • Free (open) boundary – the reflected wave undergoes no phase reversal. The incident and reflected waves are in phase at the boundary, giving an antinode.

4. Nodes and Antinodes

From \(y=2A\cos(\omega t)\sin(kx)\):

  • Node – displacement is always zero.

    \[

    \sin(kx)=0\;\Longrightarrow\;kx=n\pi\;(n=0,1,2,\dots)

    \]

    \[

    \boxed{x_n=n\frac{\lambda}{2}}

    \]

    Nodes are spaced \(\lambda/2\) apart.

  • Antinode – displacement reaches the maximum magnitude \(\pm2A\).

    \[

    |\sin(kx)|=1\;\Longrightarrow\;kx=\Bigl(n+\tfrac12\Bigr)\pi

    \]

    \[

    \boxed{x_a=\Bigl(n+\tfrac12\Bigr)\frac{\lambda}{2}}

    \]

    Antinodes are also \(\lambda/2\) apart, but offset by \(\lambda/4\) from the nearest node.

5. Energy Distribution in a Standing Wave

  • At a node the medium does not move, so both kinetic and potential energy are momentarily zero.
  • At an antinode the displacement is maximal; kinetic energy is greatest when the displacement passes through zero, and potential energy is greatest at the extreme displacement. Over a full cycle the time‑averaged energy density is highest at antinodes and zero at nodes.

For a string of linear mass density \(\mu\) the instantaneous energy per unit length is

\[

E(x,t)=\tfrac12\mu\left(\frac{\partial y}{\partial t}\right)^2

+\tfrac12 T\left(\frac{\partial y}{\partial x}\right)^2,

\]

which reduces to a sinusoidal envelope that vanishes at the nodes and peaks at the antinodes.

6. Harmonic Series and Mode Numbers

Boundary conditions restrict the allowed wavelengths. The integer \(n\) (mode number) counts the number of half‑waves fitting into the length \(L\).

  • Fixed–fixed or open–open \(L=n\lambda/2\;\;(n=1,2,3,\dots)\)
  • Closed–open \(L=(2n-1)\lambda/4\;\;(n=1,2,3,\dots)\)

The corresponding frequencies are

\[

f_n=\frac{nv}{2L}\qquad\text{(fixed–fixed / open–open)},

\qquad

f_n=\frac{(2n-1)v}{4L}\qquad\text{(closed–open)},

\]

where \(v\) is the wave speed in the medium. The first three modes for a fixed–fixed string are illustrated below (placeholder for diagram).

7. Laboratory Demonstrations (Syllabus 8.1)

ExperimentMedium & Boundary ConditionsWavelength ConditionTypical ObservationSafety / Practical Tips
Stretched string (fixed–fixed)String fixed at both ends → nodes at each end\(L=n\lambda/2\;(n=1,2,3,\dots)\)Alternating nodes and antinodes; resonant frequencies \(f_n=n v/2L\)Secure clamps firmly; keep fingers away from the vibrating region; use a driver with adjustable amplitude to avoid excessive tension.
Air column – open–open tubeBoth ends open → antinodes at each end\(L=n\lambda/2\;(n=1,2,3,\dots)\)Resonant standing sound waves; distinct “harmonic” tones heard with a speaker or tuning fork.Do not over‑inflate the tube; keep the speaker at a safe distance to avoid hearing damage at high amplitudes.
Air column – open–closed tubeClosed end → node; open end → antinode\(L=(2n-1)\lambda/4\;(n=1,2,3,\dots)\)Only odd harmonics appear; resonance when the length matches a quarter‑wave series.Use a rubber stopper that fits tightly; never place the open end near a heat source.
Microwave cavity (parallel plates)Electromagnetic wave between two reflecting plates → electric‑field nodes at the plates\(d=n\lambda/2\) where \(d\) is plate separationStanding‑wave pattern detected with a probe; intensity minima correspond to nodes.Never look directly at the microwave source; use appropriate shielding and follow the laboratory’s microwave safety protocol.

8. Practical Technique – Determining Wavelength from Nodes/Antinodes

Count‑and‑Measure Method

1. Identify and count the number of nodes (or half‑waves) between two fixed reference points (e.g. the ends of a string or the closed end of a pipe).

2. If \(N\) half‑waves are observed over a length \(L\), then

\[

\lambda=\frac{2L}{N}.

\]

3. Use the measured wavelength with the known wave speed \(v\) to obtain the frequency \(f=v/\lambda\).

This directly satisfies the AO3 requirement “determine wavelength from node/antinode positions”.

9. Worked Example – Fundamental Frequency of a Fixed–Fixed String

Given:

  • Length \(L=0.75\;\text{m}\)
  • Tension \(T=80\;\text{N}\)
  • Linear mass density \(\mu=0.002\;\text{kg m}^{-1}\)

Wave speed on the string:

\[

v=\sqrt{\frac{T}{\mu}}=\sqrt{\frac{80}{0.002}}=200\;\text{m s}^{-1}.

\]

Fundamental wavelength (first mode, \(n=1\)):

\[

\lambda_1=2L=1.50\;\text{m}.

\]

Fundamental frequency:

\[

f1=\frac{v}{\lambda1}= \frac{200}{1.50}=133.3\;\text{Hz}.

\]

Students can verify the result experimentally by adjusting the driver frequency until the first standing‑wave pattern (one antinode between the two nodes) is observed.

10. Summary Table

FeatureMathematical ConditionPosition along the mediumPhysical Meaning
Node\(\sin(kx)=0\)\(x_n=n\frac{\lambda}{2}\)Zero displacement at all times (waves 180° out of phase).
Antinode\(|\sin(kx)|=1\)\(x_a=\bigl(n+\tfrac12\bigr)\frac{\lambda}{2}\)Maximum displacement \(\pm2A\) (waves in phase).
Energy density\(E(x,t)=\tfrac12\mu\dot y^{2}+\tfrac12T y'^{2}\)Zero at nodes, maximum at antinodesShows localisation of kinetic + potential energy.
Fundamental mode\(n=1\)One half‑wave in the length \(L\)Lowest possible frequency \(f_1=v/2L\).

11. Key Points to Remember

  • A standing wave results from the superposition of two identical waves travelling in opposite directions.
  • The graphical method makes clear why nodes stay fixed while antinodes oscillate.
  • Phase reversal at a fixed boundary creates a node; no reversal at a free boundary creates an antinode.
  • Nodes are spaced \(\lambda/2\) apart; antinodes are also \(\lambda/2\) apart but offset by \(\lambda/4\).
  • Energy is stored only at antinodes; nodes carry no energy.
  • Boundary conditions dictate the allowed wavelengths and therefore the harmonic series.
  • In the laboratory, count nodes (or half‑waves) to obtain \(\lambda\), then use \(v=f\lambda\) to find the resonant frequency.
  • Observe safety guidelines for each demonstration: secure mechanical setups, protect hearing, and handle microwave sources with shielding.
  • Understanding standing waves in strings, air columns and electromagnetic cavities demonstrates the universality of the superposition principle across physics.