By the end of this chapter you'll be able to…

  • 1Distinguish transverse and longitudinal waves
  • 2Use the wave equation and find speed on strings and in gases
  • 3Apply the superposition principle and interference conditions
  • 4Analyse standing waves in strings and open/closed pipes
  • 5Explain beats and solve Doppler effect problems
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Why this chapter matters
Waves carry energy and information without carrying matter. Mechanical waves explain sound, musical instruments, and seismic waves; standing waves, beats, and the Doppler effect have applications from tuning instruments to radar and astronomy.

Before you start — revise these

A 5-minute refresher here will save you 30 minutes of confusion below.

Waves

'The wave is the fundamental entity, the primary mode of communication of energy through the universe.' — Wave Mechanics

1. Chapter Overview

WAVES are disturbances that TRANSPORT ENERGY without transporting matter. This chapter focuses on MECHANICAL WAVES (waves that require a medium — sound, springs, water waves). You will learn about TRANSVERSE and LONGITUDINAL waves, the WAVE EQUATION, SUPERPOSITION, STANDING WAVES in strings and pipes, BEATS, and the DOPPLER EFFECT.


2. Types of Waves

TypeMedium Required?Examples
MechanicalYESSound, water waves, seismic waves
ElectromagneticNOLight, radio, X-rays
Matter wavesNOElectron waves (quantum)

Mechanical Wave Classification

  • Transverse Waves: Particles vibrate PERPENDICULAR to wave direction (string waves, EM waves)
  • Longitudinal Waves: Particles vibrate PARALLEL to wave direction (sound waves, spring compression waves)

Key Terms

  • Crest: Maximum positive displacement (transverse)
  • Trough: Maximum negative displacement (transverse)
  • Compression: Region of high pressure/density (longitudinal)
  • Rarefaction: Region of low pressure/density (longitudinal)
  • Wavelength (λ): Distance between TWO successive crests/compressions
  • Amplitude (A): Maximum displacement from equilibrium

3. Wave Speed

Speed on a Stretched String

  • v = √(T/μ) where T = tension, μ = linear mass density (mass/length)
  • Independent of frequency!

Speed of Sound in a Gas

  • v = √(γP/ρ) = √(γRT/M)
  • γ = adiabatic index (1.4 for air)
  • At STP: v_air ≈ 332 m/s at 0°C, ≈ 340 m/s at 20°C

Factors Affecting Sound Speed

  • Temperature: v ∝ √T (higher T = faster sound)
  • Density: v ∝ 1/√ρ (lighter medium = faster sound)
  • Humidity: v increases with humidity (water vapour is less dense)

4. Wave Equation and Progressive Waves

Equation of a Progressive Wave

  • y(x, t) = A sin(ωt — kx + φ₀)
    • ω = 2πf (angular frequency)
    • k = 2π/λ (wave number)
    • v = ω/k = fλ (wave speed)

Particle Velocity vs Wave Velocity

  • Particle velocity: v_p = dy/dt = Aω cos(ωt — kx)
  • Wave velocity: v_w = ω/k (constant for a given medium)
  • These are DIFFERENT concepts!

Worked Problem

Q: A wave is described by y = 0.02 sin(100t — 2x) m. Find amplitude, frequency, wavelength, and wave speed. A: Comparing with y = A sin(ωt — kx): A = 0.02 m, ω = 100 rad/s, k = 2 rad/m. f = ω/2π = 100/2π = 15.92 Hz. λ = 2π/k = 2π/2 = π = 3.14 m. v = ω/k = 100/2 = 50 m/s.


5. Superposition Principle

  • Principle: When TWO or more waves overlap, the NET displacement is the SUM of individual displacements
  • y_net = y₁ + y₂ + y₃ + ...

Interference

  • Constructive: Waves in PHASE (path difference = nλ) → amplitude DOUBLES
  • Destructive: Waves OPPOSITE phase (path difference = (2n+1)λ/2) → amplitude ZERO
  • Resultant amplitude: R = √(A₁² + A₂² + 2A₁A₂cosφ)

6. Reflection of Waves

Reflection at a Boundary

BoundaryString PulsePhase Change
Rigid (fixed end)Invertedπ radians (180°)
Free endNot invertedNo phase change
Sound from rigid wallCompression as compression?Depends on density

Standing (Stationary) Waves

  • Formed when two IDENTICAL waves travel in OPPOSITE directions
  • y(x,t) = 2A sin(kx) cos(ωt)
  • Nodes: Points of ZERO displacement (2A sin(kx) = 0)
  • Antinodes: Points of MAXIMUM displacement (2A sin(kx) = ±2A)

Standing Waves in a String (Fixed at Both Ends)

  • Allowed wavelengths: λ_n = 2L/n (n = 1, 2, 3...)
  • Frequencies: f_n = nv/2L = n√(T/μ)/2L
  • n = 1: Fundamental (first harmonic)
  • n = 2: First overtone (second harmonic)
  • n = 3: Second overtone (third harmonic)

Standing Waves in a Pipe

Pipe TypeOpen EndsClosed End
Open at both endsf_n = nv/2LALL harmonics present
Closed at one endf_n = nv/4LONLY ODD harmonics

7. Beats

  • Formation: When TWO waves of SLIGHTLY DIFFERENT frequencies travel together
  • Beat frequency: f_beat = |f₁ — f₂|
  • The amplitude (loudness) varies periodically
  • Applications: Tuning musical instruments, detecting frequency differences

Worked Problem

Q: Two tuning forks of frequencies 256 Hz and 260 Hz sound together. Find beat frequency. A: f_beat = |260 — 256| = 4 Hz. You hear 4 loudness maxima per second.


8. Doppler Effect

  • Definition: APPARENT change in frequency due to RELATIVE MOTION between source and observer
  • Formula: f' = f(v + v₀)/(v — v_s)
    • v = speed of sound in the medium
    • v₀ = velocity of observer (positive TOWARD source)
    • v_s = velocity of source (positive AWAY from observer)

Special Cases

SituationApparent Frequency
Source moving toward stationary observerf' = fv/(v — v_s) — INCREASED
Source moving away from stationary observerf' = fv/(v + v_s) — DECREASED
Observer moving toward stationary sourcef' = f(v + v₀)/v — INCREASED
Observer moving away from stationary sourcef' = f(v — v₀)/v — DECREASED

Applications

  • Radar speed guns (police tracking)
  • Medical ultrasound (blood flow measurement)
  • Astronomy: REDSHIFT (stars moving away from Earth)
  • Weather radar (Doppler radar)

9. Common Mistakes

  1. Particle velocity ≠ wave velocity: Particles oscillate; the WAVE propagates. A cork on water bobs up and down while the wave moves horizontally
  2. Nodes are NOT points of minimum amplitude: They are points of PERMANENTLY ZERO amplitude
  3. Beat frequency is |f₁ — f₂|, NOT (f₁ + f₂)/2: The average frequency is what you hear; the beat is the VARIATION
  4. Doppler effect depends on RELATIVE velocity: Moving source vs. moving observer give DIFFERENT formulas
  5. Closed pipe has ONLY odd harmonics: This gives the characteristic 'mellow' sound of a clarinet

10. CBSE Exam Focus

  1. Progressive wave equation — derivation and numericals (3/5-mark)
  2. Standing waves in strings — harmonics (5-mark)
  3. Standing waves in open and closed organ pipes (5-mark)
  4. Beats — formation, beat frequency (3-mark)
  5. Doppler effect — derivation and numericals (5-mark)
  6. Speed of sound — factors affecting it

11. Key Formulas

  • v = fλ = ω/k
  • v_string = √(T/μ)
  • v_sound = √(γP/ρ) = √(γRT/M)
  • y(x,t) = A sin(ωt — kx + φ₀)
  • Standing wave: y = 2A sin(kx) cos(ωt)
  • f_n (string) = nv/2L
  • f_n (open pipe) = nv/2L
  • f_n (closed pipe) = nv/4L (n odd)
  • f_beat = |f₁ — f₂|
  • f' = f(v ± v₀)/(v ∓ v_s) (Doppler)

12. Self-Test (5+ Q&A)

Q1: A string of length 1 m has linear density 0.01 kg/m and tension 100 N. Find fundamental frequency. A: v = √(T/μ) = √(100/0.01) = 100 m/s. f₁ = v/2L = 100/2 = 50 Hz.

Q2: Two waves y₁ = 0.05 sin(200t — 5x) and y₂ = 0.05 sin(200t + 5x) interfere. Find the standing wave equation and node positions. A: y = 2×0.05 sin(5x) cos(200t) = 0.1 sin(5x) cos(200t). Nodes where sin(5x) = 0 → x = nπ/5.

Q3: A source moving at 30 m/s emits 500 Hz sound. Find apparent frequency for a stationary observer when source approaches. (v = 340 m/s) A: f' = fv/(v — v_s) = 500×340/(340 — 30) = 170000/310 = 548.4 Hz.

Q4: Find the third harmonic of a 50 cm long open organ pipe (v = 340 m/s). A: f₃ = 3v/2L = 3×340/(2×0.5) = 1020 Hz.

Q5: What are beats and how are they formed? A: Beats are periodic variations in loudness produced by superposition of two waves of slightly different frequencies. Beat frequency = |f₁ — f₂|.


13. Conclusion

Waves are FUNDAMENTAL to physics — they transport energy and information across distances. Mechanical waves in strings and pipes lead to musical instruments. Standing waves explain why a guitar string produces specific notes. Beats help in tuning. The Doppler effect has APPLICATIONS ranging from radar to astronomy. While this chapter focuses on mechanical waves, the concepts of wavelength, frequency, superposition, and interference EXTEND to light (wave optics) and quantum mechanics.

Key formulas & results

Everything you need to memorise, in one card. Screenshot this for revision.

Wave speed
v = f lambda = omega/k; v_string = sqrt(T/mu); v_sound = sqrt(gamma RT/M)
String speed depends on tension and linear density; sound speed on temperature.
Progressive wave
y(x,t) = A sin(omega t - kx + phi)
omega = 2 pi f, k = 2 pi/lambda.
Standing waves
f_n(string/open pipe) = nv/2L; f_n(closed pipe) = nv/4L (n odd)
Closed pipes give only odd harmonics.
Beats and Doppler effect
f_beat = |f1 - f2|; f' = f(v +/- v0)/(v -/+ v_s)
Apparent frequency depends on relative motion of source and observer.
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Common mistakes & fixes

These are the exact errors that cost students marks in board exams. Read them once, save yourself the trouble.

WATCH OUT
Confusing particle velocity with wave velocity
Particles oscillate about a fixed point; the wave (and its energy) propagates. A floating cork bobs up and down while the wave moves on.
WATCH OUT
Calling nodes points of minimum amplitude
Nodes are points of permanently zero amplitude in a standing wave.
WATCH OUT
Using (f1 + f2)/2 for beat frequency
Beat frequency is the difference |f1 - f2|; the average is the pitch you hear.
WATCH OUT
Using one Doppler formula for all cases
Moving source and moving observer give different expressions; apply the correct sign convention for relative motion.

Practice problems

Try each one yourself before tapping "Show solution". Active recall > rereading.

Q1MEDIUM· String
A 1 m string (mu = 0.01 kg/m, T = 100 N) is fixed at both ends. Find the fundamental frequency.
Show solution
v = sqrt(T/mu) = sqrt(100/0.01) = 100 m/s. f1 = v/2L = 100/2 = 50 Hz.
Q2HARD· Standing Wave
Waves y1 = 0.05 sin(200t - 5x) and y2 = 0.05 sin(200t + 5x) superpose. Find the standing wave and node positions.
Show solution
y = 0.1 sin(5x) cos(200t). Nodes where sin(5x) = 0, i.e. x = n pi/5 (n = 0, 1, 2, ...).
Q3MEDIUM· Doppler
A source moving at 30 m/s emits 500 Hz toward a stationary observer (v = 340 m/s). Find the apparent frequency.
Show solution
f' = fv/(v - v_s) = 500 x 340/(340 - 30) = 170000/310 = 548.4 Hz.
Q4MEDIUM· Pipe
Find the third harmonic of a 50 cm open organ pipe (v = 340 m/s).
Show solution
f3 = 3v/2L = 3 x 340/(2 x 0.5) = 1020 Hz.
Q5EASY· Beats
Two tuning forks of 256 Hz and 260 Hz sound together. Find the beat frequency.
Show solution
f_beat = |260 - 256| = 4 Hz, so 4 loudness maxima are heard per second.

5-minute revision

The whole chapter, distilled. Read this the night before the exam.

  • Transverse waves vibrate perpendicular, longitudinal parallel to propagation.
  • v = f lambda; v_string = sqrt(T/mu); v_sound = sqrt(gamma RT/M); sound speed rises with temperature.
  • Progressive wave: y = A sin(omega t - kx); particle velocity differs from wave velocity.
  • Superposition: constructive (path difference n lambda), destructive ((2n+1)lambda/2).
  • Standing waves: nodes (zero) and antinodes (maximum); string/open pipe f_n = nv/2L.
  • Closed pipe: f_n = nv/4L, only odd harmonics.
  • Beats: f_beat = |f1 - f2|; Doppler: f' = f(v +/- v0)/(v -/+ v_s).

CBSE marks blueprint

Where the marks come from in this chapter — so you can plan your prep.

Typical chapter weightage: 7-9 marks across the chapter

Question typeMarks eachTypical countWhat it tests
Standing waves (strings/pipes)3-51Harmonics and resonance frequencies
Doppler effect3-51Apparent frequency for moving source/observer
Wave equation / beats2-31Progressive waves and beat frequency
Prep strategy
  • Practise reading A, omega, k from the wave equation
  • Learn harmonic series for strings and both pipe types
  • Master the Doppler sign convention with all four cases
  • Remember beat frequency is the difference of frequencies

Where this shows up in the real world

This chapter isn't just an exam topic — it lives in the world around you.

Musical instruments

Standing waves in strings and air columns produce the notes of guitars, flutes, and organs.

Medical and radar imaging

Doppler ultrasound measures blood flow and radar guns measure vehicle speeds.

Astronomy

Doppler redshift reveals the motion of stars and the expansion of the universe.

Exam strategy

Battle-tested tips from teachers and toppers for this chapter.

  1. Extract A, omega, k, v from the given wave equation first
  2. Draw the harmonic pattern for string/pipe problems
  3. Set the Doppler sign convention before substituting
  4. Use f_beat = |f1 - f2| for tuning problems

Going beyond the textbook

For olympiad aspirants and curious learners — topics that build on this chapter.

  • Derive the Doppler formula for a moving medium (wind) and combined source-observer motion.
  • Analyse end-correction in organ pipes and the superposition of multiple harmonics.

Where else this chapter is tested

CBSE board isn't the only one — other exams test this chapter too.

CBSE Class 11 Physics examHigh
JEE Main and Advanced (Waves)Very High
NEET PhysicsHigh

Questions students ask

The real ones — pulled from the Q&A community and tutor sessions.

A pipe closed at one end must have a node (zero displacement) at the closed end and an antinode at the open end. The boundary conditions allow only wavelengths where the pipe length equals an odd number of quarter-wavelengths (L = lambda/4, 3 lambda/4, ...). This gives frequencies f_n = nv/4L for odd n only, which is why a closed pipe sounds an octave lower and 'mellower' than an open pipe of the same length.

When a light or sound source moves away from an observer, the waves are stretched, lowering the observed frequency. For light from distant galaxies moving away from us, this shifts the spectral lines toward the red (longer wavelength) end -- the cosmological redshift. Measuring this shift lets astronomers determine how fast galaxies recede, which is key evidence for the expanding universe.
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Last reviewed on 29 May 2026. Written and reviewed by subject-matter experts — read about our process.
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