The Physics of Waves
Textbook Exercise Solutions
NCERT Exercises on Waves — The Gateway to Competitive Excellence
Waves are not merely a chapter in a textbook — they are the language through which nature communicates energy across space. From the ultrasonic pulses that map tumours inside the human body, to the seismic waves that reveal the interior of the Earth, to the electromagnetic oscillations that carry your internet signal — wave mechanics underpins modern science and technology in ways that are both breathtaking and indispensable.
NCERT Chapter 14 on Waves is strategically one of the most high-yield chapters in all of Class XI Physics, not merely for board examinations, but as a decisive battleground for competitive entrance tests — primarily IIT JEE (Main + Advanced), NEET, BITSAT, and CUET. The chapter builds from the fundamental description of wave motion to the rich physics of standing waves, resonance, beats, and the Doppler effect — all of which appear with remarkable regularity in question papers year after year.
The 19 textbook exercises cover a carefully curated range of difficulty: from straightforward formula application (wave speed on a string, wavelength computation) to demanding conceptual reasoning (the nature of stationary vs. travelling waves, why a displacement node is a pressure antinode, why sound travels faster in humid air). This precise balance mirrors what competitive examiners expect — numerical dexterity grounded in conceptual depth.
Data from JEE Mains papers (2010–2024) reveals that questions on wave speed on strings (Exercises 1, 3, 11, 14), standing wave equations and their interpretation (Exercises 11, 12, 13), beat frequency (Exercise 18), resonance in organ pipes (Exercises 15, 17), and the Doppler effect frequently recur in nearly every examination cycle. The conceptual questions in Exercises 4, 5, 13, and 19 map directly to the single-correct and multi-correct options in JEE Advanced, where a one-line explanation can cost or win 4 marks.
IIT JEE Aspirants
These exercises build the algebraic fluency needed for multi-step derivations. JEE Advanced routinely links wave mechanics to SHM, electromagnetism (EM waves) and modern physics — all seeded here.
NEET Aspirants
Ultrasound in medicine (Q7), speed of sound (Q2, Q4), and resonance (Q15, Q17) are directly mapped to Biology-Physics interfaces, a growing trend in NEET paper design.
Conceptual Clarity
Exercises 4, 5, 13, and 19 demand reasoning over calculation. Regular practice here builds the analytical thinking that separates top-rankers from average scorers.
Board Examination
Each solution in this set follows the logical structure expected in CBSE marking schemes — step-by-step derivation, substitution, and clearly boxed conclusions.
What makes the solutions presented here distinctive is the inclusion of a Theory Brief before each exercise solution — a concise, precision-written encapsulation of the governing physical principle. This bridges the gap between rote formula substitution and genuine understanding. When a student internalises why the formula works — not just how to apply it — every variant question in a competitive exam becomes familiar territory.
The 19 NCERT exercises, mastered thoroughly, represent a minimum viable syllabus for Waves. They are not a ceiling — they are a launchpad. The student who can solve each of these problems fluently, explain the physics behind each step, and identify the underlying principle has built a foundation robust enough to tackle virtually any wave-mechanics question that JEE, NEET, or any competitive examination can present.
A transverse wave on a stretched string is a mechanical disturbance in which each element of the string oscillates perpendicular to the direction of wave propagation. The wave carries energy — but not matter — from one end to the other. The speed of this wave depends on two physical properties of the string: the tension T (restoring force that pulls displaced elements back) and the linear mass density μ (inertia per unit length, resisting acceleration). The governing relation is derived from Newton's second law applied to a small string element and yields the elegant result v = √(T/μ). Greater tension → faster propagation; greater mass per unit length → slower propagation. This formula appears in JEE/NEET virtually every alternate year.
To determine the time taken by the disturbance to travel along the string, we first need the speed of transverse waves on a stretched string. This speed depends on the tension in the string and its mass per unit length.
The mass per unit length of the string is obtained by dividing the total mass by the total length of the stretched string. Using the given values, the linear mass density is calculated as
\[\mu = \frac{m}{L} = \frac{2.50}{20.0} = 0.125 \ \text{kg m}^{-1}\]
The speed of a transverse wave travelling along a stretched string under tension is given by
\[v = \sqrt{\frac{T}{\mu}}\]
Substituting the known values of tension and linear mass density, we obtain
\[\begin{aligned}v &= \sqrt{\frac{200}{0.125}} \\&= \sqrt{1600} \\&= 40 \ \text{m s}^{-1}\end{aligned}\]
The time taken by the disturbance to travel the full length of the string is the ratio of distance to wave speed. Therefore,
\[\begin{aligned}t &= \frac{L}{v} \\&= \frac{20.0}{40} \\&= 0.50 \ \text{s}\end{aligned}\]
The transverse disturbance takes 0.50 seconds to reach the other end of the string.
This problem elegantly combines two branches of mechanics: kinematics of free fall and propagation of sound. The total elapsed time is the sum of two sequential intervals — (i) the time the stone takes to fall under gravity from rest, governed by \(h = \frac{1}{2}gt^2\), and (ii) the time the sound of the splash takes to travel back up at a constant speed of 340 m s⁻¹. The key conceptual point is that the two events are sequential, not simultaneous: first fall, then acoustic travel. This type of two-stage time problem is a perennial favourite in JEE Main, often disguised with different heights, speeds, or media (e.g., water instead of air for sound travel).
When the stone is released from rest at the top of the tower, it first takes some time to fall freely through air before splashing into the water. This time of fall is determined using the equation of motion for uniformly accelerated motion under gravity.
\[\begin{aligned}h &= \frac{1}{2} g t_1^2 \\300 &= \frac{1}{2} \times 9.8 \times t_1^2\end{aligned}\]
Solving for the time of fall,
\[\begin{aligned}t_1^2 &= \frac{600}{9.8} \\t_1 &\approx 7.83 \ \text{s}\end{aligned}\]
After the stone hits the water, the sound of the splash travels upward through air to the top of the tower. The time taken by sound to travel this distance is obtained using the relation between speed, distance, and time.
\[\begin{aligned}t_2 &= \frac{\text{distance}}{\text{speed of sound}} \\&= \frac{300}{340} \\&\approx 0.88 \ \text{s}\end{aligned}\]
The total time after the stone is dropped at which the splash is heard at the top is the sum of the time of fall and the time taken by sound to travel upward.
\[\begin{aligned}t &= t_1 + t_2 \\&= 7.83 + 0.88 \\&\approx 8.71 \ \text{s}\end{aligned}\]
The splash is heard at the top of the tower approximately 8.7 seconds after the stone is released.
This exercise reverses the typical direction of Q1: instead of finding speed given tension, we find the tension required to produce a prescribed speed. The relation \(v = \sqrt{T/\mu}\) is rearranged to \(T = \mu v^2\). What makes this question conceptually illuminating is the sheer magnitude of the answer — matching the speed of sound in air requires an enormous tension (~20,000 N), underscoring that mechanical transverse waves in solids can indeed reach acoustic speeds, but only under extraordinary stress. This insight connects to why steel is the material of choice in musical strings and ultrasonic transducers. JEE Advanced often frames questions around this inversion — computing a physical property needed to achieve a target outcome.
The speed of a transverse wave on a stretched wire depends on the tension in the wire and its mass per unit length. To make this speed equal to the speed of sound in air, we first determine the linear mass density of the steel wire using its given mass and length.
\[\mu = \frac{m}{L} = \frac{2.10}{12.0} = 0.175 \ \text{kg m}^{-1}\]
The speed of a transverse wave on a stretched wire is given by the relation
\[v = \sqrt{\frac{T}{\mu}}\]
Since the wave speed is required to be equal to the speed of sound in air at 20 °C, we substitute \(v = 343 \ \text{m s}^{-1}\) and rearrange the expression to obtain the tension in the wire.
\[\begin{aligned}T &= \mu v^2 \\&= 0.175 \times (343)^2\end{aligned}\]
Evaluating the expression,
\[\begin{aligned}T &= 0.175 \times 117\,649 \\&\approx 2.06 \times 10^{4} \ \text{N}\end{aligned}\]
The tension required in the steel wire so that the transverse wave travels with the speed of sound in air is approximately \(2.06 \times 10^{4}\ \text{N}\).
This is the single most conceptually rich exercise in the first half of the chapter, and it is a recurrent JEE/NEET favourite. The formula \(v = \sqrt{\gamma P/\rho}\) appears to suggest pressure dependence — but applying the ideal gas law reveals the pressure cancellation at constant temperature: \(\rho \propto P\), so \(P/\rho = RT/M = \text{constant at fixed } T\). The result \(v = \sqrt{\gamma RT/M}\) then reveals the three answers: (a) no P dependence, (b) \(v \propto \sqrt{T}\), (c) humid air has lower effective molecular mass M (water vapour M = 18 vs. air M ≈ 29), so speed increases. Each of these points has appeared as a standalone MCQ or assertion-reason question in JEE Main, NEET, and BITSAT multiple times.
The speed of sound in a gas is given by the relation \( v = \sqrt{\dfrac{\gamma P}{\rho}} \), where \(\gamma\) is the ratio of specific heats, \(P\) is the pressure of the gas, and \(\rho\) is its density. This expression helps us understand how different physical factors affect the propagation of sound in air.
To explain the effect of pressure, we recall that for an ideal gas at constant temperature, the density is directly proportional to pressure. Using the gas law, the density of air can be written as
\[\rho = \frac{P M}{R T}\]
Substituting this expression for density into the formula for speed of sound, we obtain
\[\begin{aligned}v &= \sqrt{\frac{\gamma P}{\rho}} \\&= \sqrt{\frac{\gamma P}{\dfrac{P M}{R T}}} \\&= \sqrt{\frac{\gamma R T}{M}}\end{aligned}\]
Since pressure no longer appears in the final expression, the speed of sound in air is independent of pressure, provided the temperature remains constant.
The above result also shows that the speed of sound is directly proportional to the square root of absolute temperature. As the temperature increases, the average kinetic energy of air molecules increases, enabling sound waves to travel faster. Hence, the speed of sound in air increases with temperature.
Humidity refers to the presence of water vapour in air. When humidity increases, lighter water vapour molecules (molar mass ≈ 18 g mol⁻¹) partially replace heavier oxygen and nitrogen molecules (effective molar mass of dry air ≈ 29 g mol⁻¹), reducing the average molecular mass of air. From the relation
\[v = \sqrt{\frac{\gamma R T}{M}}\]
it is clear that a decrease in the effective molecular mass \(M\) results in an increase in the speed of sound. Therefore, sound travels faster in humid air than in dry air.
The given formula explains why the speed of sound in air is independent of pressure (since ρ ∝ P, they cancel), increases with temperature (v ∝ √T), and increases with humidity (water vapour lowers effective molar mass M).
The standard definition of a one-dimensional travelling wave — that displacement depends only on the combination \((x \pm vt)\) — is both a sufficient and necessary condition for a wave profile to propagate without distortion at speed v. This exercise tests whether students understand the converse: every function of \((x \pm vt)\), regardless of its mathematical form (polynomial, logarithmic, rational), represents a valid travelling wave as long as it is physically well-defined (finite, single-valued, and continuous for all relevant x and t). The critical insight is that a sinusoidal form is not required — it is merely the most common and most useful for harmonic analysis. JEE Advanced has examined this concept in assertion-reason and multi-correct formats to probe deeper conceptual understanding beyond rote application.
A one-dimensional travelling wave is any disturbance whose shape moves without change along the x-axis with a constant speed. Mathematically, this requirement is satisfied if the displacement can be written as a function of the single combined variable \(x - vt\) or \(x + vt\). Therefore, any expression of the form \(y = f(x \pm vt)\), where \(f\) is an arbitrary function, represents a travelling wave. Hence, the converse statement is indeed true.
To examine the given functions, we check whether the displacement depends only on a single combination of position and time.
For the function \(y = (x - vt)^2\), the displacement depends entirely on the variable \((x - vt)\). Although the shape of the wave is parabolic rather than sinusoidal, the entire profile shifts unchanged in the positive x-direction with speed \(v\). Therefore, this function does represent a travelling wave.
In the case \(y = \log\!\left(\frac{x + vt}{x_0}\right)\), the displacement again depends only on the single variable \((x + vt)\), with \(x_0\) being a constant introduced for dimensional consistency. Since the form of the function remains unchanged as it moves in the negative x-direction with speed \(v\), this function can also represent a travelling wave.
For the function \(y = \dfrac{1}{x + vt}\), the dependence is solely on the combined variable \((x + vt)\). This implies that the entire waveform moves rigidly along the x-axis without distortion, travelling in the negative direction with speed \(v\). Hence, this function too represents a travelling wave.
The converse is true. All three functions — \((x-vt)^2\), \(\log[(x+vt)/x_0]\), and \(1/(x+vt)\) — depend solely on \(x \pm vt\) and therefore represent travelling waves, provided they are well-defined for the domain of propagation.
When a sound wave encounters a boundary between two media — here, air and water — it partially reflects back into the first medium and partially transmits (refracts) into the second. The single most important rule governing this process is: the frequency of the wave remains unchanged across the boundary. This is a consequence of the boundary conditions — the interface must oscillate at the same rate on both sides. What changes is the wave speed (because the elastic and inertial properties of each medium differ), and consequently the wavelength changes as \(\lambda = v/f\). The reflected wave stays in air (same speed, same wavelength as incident), while the transmitted wave enters water (higher speed → longer wavelength). This principle is identical to what happens with light at glass–air interfaces in optics, making this exercise a conceptual bridge across chapters. JEE Main frequently tests this in assertion-reason format.
The bat emits ultrasonic sound waves of frequency 1000 kHz, which is equal to \(1.0 \times 10^{6}\ \text{Hz}\). When these waves strike the water surface, part of the sound is reflected back into air and part is transmitted into water. The frequency of sound remains unchanged during reflection and transmission, while the wavelength changes according to the speed of sound in the medium.
For the reflected sound, the wave continues to travel in air. The wavelength of sound in a medium is given by the relation \(\lambda = v/f\). Substituting the given speed of sound in air and the frequency of the ultrasonic wave,
\[\begin{aligned}\lambda_{\text{air}} &= \frac{340}{1.0 \times 10^{6}} \\&= 3.4 \times 10^{-4}\ \text{m}\end{aligned}\]
For the transmitted sound, the wave travels through water. The frequency remains the same, but the speed of sound in water is much higher, so the wavelength is greater. Using the same relation,
\[\begin{aligned}\lambda_{\text{water}} &= \frac{1486}{1.0 \times 10^{6}} \\&= 1.486 \times 10^{-3}\ \text{m}\end{aligned}\]
- Wavelength of reflected sound (in air): \(3.4 \times 10^{-4}\ \text{m}\)
- Wavelength of transmitted sound (in water): \(1.486 \times 10^{-3}\ \text{m}\)
This problem is deceptively simple in calculation but rich in physical context — a context that NEET examiners love to exploit. Ultrasonic scanners operate at frequencies far above the human auditory range (typically 1–20 MHz) precisely because of the resolving-power principle: a wave can only resolve (detect) objects larger than its own wavelength. At 4.2 MHz in tissue, the wavelength works out to about 0.4 mm, which is comparable to the size of small tumours. Lower frequencies would give longer wavelengths and poor resolution; higher frequencies are absorbed too quickly by tissue. The operating frequency of a medical scanner is thus a careful engineering compromise between resolution (favouring high frequency → short wavelength) and penetration depth (favouring low frequency). This exercise, while numerically straightforward, introduces students to one of the most clinically important applications of wave physics. Be careful with unit conversion: 1.7 km s⁻¹ must be converted to m s⁻¹, and 4.2 MHz to Hz, before applying \(\lambda = v/f\).
An ultrasonic scanner operates by transmitting high-frequency sound waves into body tissue and analysing the reflected waves. The wavelength of these waves inside the tissue depends on the speed of sound in the tissue and the operating frequency of the scanner.
The given speed of sound in the tissue is 1.7 km s⁻¹, which is first converted into SI units for consistency.
\[v = 1.7 \times 10^{3}\ \text{m s}^{-1}\]
The operating frequency of the ultrasonic scanner is 4.2 MHz, which is expressed as
\[f = 4.2 \times 10^{6}\ \text{Hz}\]
The wavelength of sound is related to its speed and frequency by
\[\lambda = \frac{v}{f}\]
Substituting the values,
\[\begin{aligned}\lambda &= \frac{1.7 \times 10^{3}}{4.2 \times 10^{6}} \\&\approx 4.05 \times 10^{-4}\ \text{m}\end{aligned}\]
The wavelength of the ultrasonic sound in the tissue is approximately \(4.05 \times 10^{-4}\ \text{m}\) (≈ 0.4 mm), which is suitable for resolving small tissue structures such as tumours.
The standard form of a one-dimensional harmonic travelling wave is \(y = A\sin(\omega t \pm kx + \phi_0)\), where: A = amplitude (maximum displacement), ω = angular frequency = \(2\pi f\), k = wave number = \(2\pi/\lambda\), φ₀ = initial phase at origin, and the sign of the \(kx\) term determines direction — positive sign (+kx) means the wave travels in the negative x-direction (leftward), while a negative sign (−kx) means it travels in the positive x-direction (rightward). The speed is \(v = \omega/k\). The wavelength (distance between successive crests) is \(\lambda = 2\pi/k\). This single exercise tests all six wave parameters simultaneously — making it one of the most exam-effective problems in the chapter. This exact equation structure appears in JEE Main almost every year, sometimes with cosine instead of sine, or with different signs.
The given transverse wave is described by \( y(x,t) = 3.0 \sin(36t + 0.018x + \pi/4) \). The displacement depends on both position and time through a combined argument \((\omega t + kx)\). Since the spatial and temporal parts are mixed together — not separated as a product — this is a travelling wave, not a stationary wave.
A travelling wave of the form \(y = A \sin(\omega t + kx + \phi)\) propagates in the negative x-direction (i.e., from right to left), because the phase \((\omega t + kx)\) is constant along a wave crest only when \(x\) decreases as \(t\) increases. Comparing with the standard form:
\[\omega = 36\ \text{rad s}^{-1}, \qquad k = 0.018\ \text{cm}^{-1}\]
The speed of propagation is
\[\begin{aligned}v &= \frac{\omega}{k} = \frac{36}{0.018} = 2000\ \text{cm s}^{-1} = 20\ \text{m s}^{-1}\end{aligned}\]
The wave travels at 20 m s⁻¹ in the negative x-direction — from right to left.
The amplitude is the coefficient of the sine function:
\[A = 3.0\ \text{cm}\]
The frequency is related to the angular frequency by \(f = \omega/2\pi\):
\[\begin{aligned}f &= \frac{36}{2\pi} \approx 5.73\ \text{Hz}\end{aligned}\]
Setting \(x = 0\) and \(t = 0\) in the wave equation, the phase becomes the constant term:
\[\phi_0 = \frac{\pi}{4}\ \text{rad}\]
The least distance between two successive crests is the wavelength \(\lambda = 2\pi/k\):
\[\begin{aligned}\lambda &= \frac{2\pi}{0.018} \approx 349\ \text{cm} \approx 3.49\ \text{m}\end{aligned}\]
- Travelling wave moving right to left at 20 m s⁻¹
- Amplitude = 3.0 cm ; Frequency ≈ 5.73 Hz
- Initial phase at origin = π/4 rad
- Wavelength (crest-to-crest distance) ≈ 3.49 m
One of the deepest conceptual questions in wave mechanics: how does the motion at a single fixed point look as time progresses? When we hold \(x\) fixed and let \(t\) vary, the wave equation \(y(x,t) = A\sin(\omega t + kx + \phi_0)\) reduces to simple harmonic motion: \(y = A\sin(\omega t + \phi_{eff})\), where the effective phase \(\phi_{eff} = kx + \phi_0\) depends on position but is constant for a given \(x\). The conclusion is profound: every particle of the medium executes SHM with the same amplitude and frequency, but with a phase that varies continuously from point to point. The y–t graph at any \(x\) is a perfect sine curve — only its starting phase differs. This distinguishes a travelling wave from a stationary wave, where amplitude also varies with position. This is a very common MCQ in JEE Main, often asking "which property differs from point to point in a travelling wave?"
The wave equation from Exercise 14.8 is \( y(x,t) = 3.0 \sin(36t + 0.018x + \pi/4) \), where \(y\) and \(x\) are in cm and \(t\) in seconds. To plot y–t graphs at fixed positions, we substitute each value of \(x\).
\[\begin{aligned}y(0,t) &= 3.0 \sin\!\left(36t + \frac{\pi}{4}\right)\end{aligned}\]
This is a sinusoidal oscillation with amplitude 3.0 cm, angular frequency 36 rad s⁻¹, and initial phase \(\pi/4\). The y–t graph is a sine curve starting at \(y = 3.0\sin(\pi/4) = 3.0/\sqrt{2} \approx 2.12\ \text{cm}\) at \(t = 0\).
\[\begin{aligned}y(2,t) &= 3.0 \sin\!\left(36t + 0.018 \times 2 + \frac{\pi}{4}\right) \\&= 3.0 \sin\!\left(36t + 0.036 + \frac{\pi}{4}\right)\end{aligned}\]
The shape remains sinusoidal with the same amplitude (3.0 cm) and the same angular frequency (36 rad s⁻¹), but the phase is shifted forward by \(0.036\) rad compared to \(x = 0\).
\[\begin{aligned}y(4,t) &= 3.0 \sin\!\left(36t + 0.018 \times 4 + \frac{\pi}{4}\right) \\&= 3.0 \sin\!\left(36t + 0.072 + \frac{\pi}{4}\right)\end{aligned}\]
Again, the shape is sinusoidal with the same amplitude and frequency, but a further phase shift of \(0.072\) rad relative to \(x = 0\).
All three y–t graphs are sine curves of identical amplitude and identical frequency. The graphs are simply shifted along the time axis — each is a horizontal translation of the others. The only difference is the phase of oscillation, which increases with increasing \(x\) (since the wave travels in the \(-x\) direction, points at larger \(x\) are ahead in phase).
All y–t graphs are sinusoidal (sine curves) with identical amplitude (3.0 cm) and identical frequency (~5.73 Hz). The oscillatory motion differs from point to point only in phase — not in amplitude or frequency.
Phase difference is at the heart of wave interference, standing waves, and coherence — topics that span multiple chapters in both JEE and NEET syllabi. For a harmonic wave \(y = A\cos(2\pi ft - 2\pi x/\lambda + \phi_0)\), the phase at position \(x\) is \(\Phi = 2\pi ft - 2\pi x/\lambda + \phi_0\). The phase difference between two points separated by distance \(\Delta x\) is simply \(\Delta\phi = (2\pi/\lambda)\Delta x = k\Delta x\), independent of time. This exercise also requires careful reading of the wave equation to extract \(k\) — here the equation is in the form \(2\pi(10t - 0.0080x)\), so the wave number factor is \(2\pi \times 0.0080\ \text{cm}^{-1}\), and the wavelength is found from \(0.0080\lambda = 1\) giving \(\lambda = 125\ \text{cm}\). Unit discipline is critical — distances given in metres must be converted to centimetres before substitution. This is the single most common source of errors in competitive exams on this topic.
The given travelling harmonic wave is \( y(x,t) = 2.0 \cos 2\pi(10t - 0.0080x + 0.35) \). Expanding, the phase of the wave is the full argument of the cosine. The spatial part \(-0.0080x\) (with \(x\) in cm) determines how phase varies with position. The phase difference between two points separated by \(\Delta x\) is
\[\Delta \phi = 2\pi \times 0.0080\, \Delta x \quad (\Delta x \text{ in cm})\]
The wavelength is found by noting that one full cycle of phase (\(2\pi\)) corresponds to one wavelength:
\[\begin{aligned}0.0080\, \lambda &= 1 \\\lambda &= 125\ \text{cm} = 1.25\ \text{m}\end{aligned}\]
\[\begin{aligned}\Delta \phi &= 2\pi \times 0.0080 \times 400 \\&= 2\pi \times 3.2 \\&= 6.4\pi\ \text{rad}\end{aligned}\]
\[\begin{aligned}\Delta \phi &= 2\pi \times 0.0080 \times 50 \\&= 2\pi \times 0.4 \\&= 0.8\pi\ \text{rad}\end{aligned}\]
When the separation equals half a wavelength, substituting \(\Delta x = \lambda/2 = 62.5\ \text{cm}\):
\[\begin{aligned}\Delta \phi &= 2\pi \times 0.0080 \times 62.5 \\&= 2\pi \times 0.5 \\&= \pi\ \text{rad}\end{aligned}\]
This confirms the general result: points separated by \(\lambda/2\) are always exactly in opposite phase (\(\Delta\phi = \pi\)) — one is at a crest when the other is at a trough.
\[\begin{aligned}\Delta \phi &= 2\pi \times 0.0080 \times 93.75 \\&= 2\pi \times 0.75 \\&= \frac{3\pi}{2}\ \text{rad}\end{aligned}\]
- 4 m separation: \(\Delta\phi = 6.4\pi\) rad
- 0.5 m separation: \(\Delta\phi = 0.8\pi\) rad
- \(\lambda/2\) separation: \(\Delta\phi = \pi\) rad (anti-phase)
- \(3\lambda/4\) separation: \(\Delta\phi = 3\pi/2\) rad
A stationary (standing) wave is the result of superposition of two identical harmonic travelling waves moving in opposite directions with the same speed, frequency, and amplitude. The mathematical signature of a stationary wave is a product of a purely spatial function and a purely temporal function — i.e., the variables \(x\) and \(t\) are separated: \(y = f(x)\cdot g(t)\). This means every point oscillates with the same frequency but with a position-dependent amplitude. Nodes (zero amplitude) occur where \(\sin(kx) = 0\); antinodes (maximum amplitude) occur where \(|\sin(kx)| = 1\). The decomposition uses the product-to-sum identity \(\sin kx \cos\omega t = \tfrac{1}{2}[\sin(kx-\omega t)+\sin(kx+\omega t)]\), revealing two travelling waves. The tension is then found via \(T = \mu v^2\). This is one of the most complete, multi-part exercise types in the chapter and is a JEE staple.
The displacement \( y(x,t) = 0.06\sin\!\left(\frac{2\pi}{3}x\right)\cos(120\pi t) \) is expressed as a product of a function of \(x\) alone and a function of \(t\) alone. The spatial and temporal parts are fully separated, which is the defining characteristic of a stationary wave. The string has fixed nodes whose positions never change with time, confirming this interpretation. The boundary conditions (clamped at both ends) require nodes at \(x = 0\) and \(x = 1.5\ \text{m}\), which is consistent with \(\sin(2\pi/3 \times 1.5) = \sin(\pi) = 0\). ✓
Using the trigonometric product-to-sum identity,
\[\sin kx\cos\omega t = \tfrac{1}{2}\big[\sin(kx - \omega t) + \sin(kx + \omega t)\big]\]
the given equation is rewritten as
\[\begin{aligned}y(x,t) &= 0.06\sin\!\left(\tfrac{2\pi}{3}x\right)\cos(120\pi t) \\&= 0.03\Big[\sin\!\left(\tfrac{2\pi}{3}x - 120\pi t\right) + \sin\!\left(\tfrac{2\pi}{3}x + 120\pi t\right)\Big]\end{aligned}\]
This shows that the stationary wave is formed by two travelling waves, each of amplitude \(0.03\ \text{m}\): one moving in the positive \(x\)-direction and one in the negative \(x\)-direction.
From the wave equation, the wave number is \(k = \frac{2\pi}{3}\ \text{rad m}^{-1}\) and angular frequency is \(\omega = 120\pi\ \text{rad s}^{-1}\).
Wavelength of each travelling wave:
\[\lambda = \frac{2\pi}{k} = \frac{2\pi}{2\pi/3} = 3\ \text{m}\]
Frequency of each travelling wave:
\[f = \frac{\omega}{2\pi} = \frac{120\pi}{2\pi} = 60\ \text{Hz}\]
Speed of each travelling wave:
\[v = f\lambda = 60 \times 3 = 180\ \text{m s}^{-1}\]
The linear mass density of the string is
\[\mu = \frac{m}{L} = \frac{3.0\times10^{-2}}{1.5} = 2.0\times10^{-2}\ \text{kg m}^{-1}\]
Using \(v = \sqrt{T/\mu}\), the tension is
\[\begin{aligned}T &= \mu v^2 = (2.0\times10^{-2})(180)^2 = 648\ \text{N}\end{aligned}\]
- The function represents a stationary wave
- Each component travelling wave: wavelength = 3 m, frequency = 60 Hz, speed = 180 m s⁻¹
- Tension in the string = 648 N
In a stationary wave \(y = A_0\sin(kx)\cos(\omega t)\), the temporal factor \(\cos(\omega t)\) is the same for every point — so all particles share the same frequency. However, the spatial factor \(\sin(kx)\) gives each point a different amplitude: \(A(x) = A_0|\sin(kx)|\). This amplitude is zero at nodes and maximum at antinodes — a fundamental contrast with travelling waves where amplitude is uniform. Regarding phase: points within the same loop oscillate in phase (the sign of \(\sin(kx)\) is the same), while points on opposite sides of a node oscillate in antiphase (the sign flips across a node). These three properties — same frequency, position-dependent amplitude, position-dependent phase — are among the most reliably tested conceptual distinctions in competitive examinations.
In the stationary wave \( y(x,t) = 0.06\sin\!\left(\frac{2\pi}{3}x\right)\cos(120\pi t) \), the time-dependent factor \(\cos(120\pi t)\) is common to all positions. Therefore, every point on the string oscillates with the same angular frequency \(\omega = 120\pi\ \text{rad s}^{-1}\), i.e., the same frequency of 60 Hz. Yes — all points share the same frequency.
The phase of oscillation depends on the sign of \(\sin(2\pi x/3)\). Within any single loop between two consecutive nodes, this function maintains the same sign, so all points in that loop oscillate in phase with each other. However, across a node the function changes sign, so particles on either side of a node are in opposite phase. Therefore, the phase is not the same for all points — it is uniform within a loop but reverses at every node.
The amplitude of oscillation at position \(x\) is given by the magnitude of the spatial factor:
\[A(x) = 0.06\left|\sin\!\left(\frac{2\pi}{3}x\right)\right|\]
This varies continuously from zero at the nodes to a maximum of 0.06 m at the antinodes. The amplitude is not the same for all points — it depends strongly on position.
Substituting \(x = 0.375\ \text{m}\) into the amplitude expression:
\[\begin{aligned}A &= 0.06\sin\!\left(\frac{2\pi}{3}\times 0.375\right) \\&= 0.06\sin\!\left(\frac{\pi}{4}\right) \\&= 0.06\times\frac{1}{\sqrt{2}} \approx 4.24\times10^{-2}\ \text{m}\end{aligned}\]
- Frequency: same for all points (60 Hz)
- Phase: varies — same within a loop, opposite across a node
- Amplitude: varies with position — zero at nodes, maximum at antinodes
- Amplitude at \(x = 0.375\ \text{m}\): \(\approx 4.24\times10^{-2}\ \text{m}\)
Classifying a mathematical expression as a wave requires checking three things: (1) Does the displacement depend only on \((x \pm vt)\)? → Travelling wave. (2) Is it a product of a purely spatial and purely temporal function? → Stationary wave. (3) Is it well-defined (finite, single-valued, real) for all relevant \(x\) and \(t\)? → If not, it represents no physical wave. A key technique for case (c) is recognising that \(A\sin\theta + B\cos\theta = \sqrt{A^2+B^2}\sin(\theta+\phi)\) — so two harmonics with the same argument combine into a single harmonic of the same argument, forming one travelling wave. Case (d) is a superposition of two stationary waves of different frequencies — the combined expression has neither fixed nodes nor a single travelling profile, so it is "none of the above" in terms of pure wave types.
An elastic wave must be finite, single-valued, and well-defined over the entire propagation domain. We now examine each function.
The displacement is written as a product of \(\cos(3x)\) (purely spatial) and \(\sin(10t)\) (purely temporal). The variables are completely separated, which is the hallmark of a stationary wave. Fixed nodes exist wherever \(\cos(3x) = 0\), confirming the stationary character.
Although the argument is the travelling-wave combination \((x - vt)\), the square-root function is undefined (not real) whenever \(x - vt < 0\). A physical wave must be well-defined over the entire medium — this condition fails for all points where \(x < vt\). Therefore, this function represents no valid physical wave.
Both terms share the identical argument \((5x - 0.5t)\). Using the harmonic addition formula,
\[\begin{aligned}y &= 3\sin(5x-0.5t) + 4\cos(5x-0.5t) \\&= \sqrt{3^2+4^2}\,\sin(5x - 0.5t + \phi) \\&= 5\sin(5x - 0.5t + \phi)\end{aligned}\]
where \(\tan\phi = 4/3\). The combined expression depends only on \((x - vt)\) and is a single sinusoidal function — this is a travelling wave of amplitude 5 m, wave number 5 rad m⁻¹, travelling in the positive \(x\)-direction with speed \(v = 0.5/5 = 0.1\ \text{m s}^{-1}\).
Each term individually represents a stationary wave (\(\cos x\sin t\) and \(\cos 2x\sin 2t\)), but they have different angular frequencies (1 rad s⁻¹ and 2 rad s⁻¹) and different wave numbers. Their superposition does not produce a single stationary wave with fixed, time-invariant nodes, nor does it reduce to any function of \((x \pm vt)\). It represents none of the pure wave types — it is a superposition of two independent standing waves forming a complex, non-periodic displacement pattern.
- (a) \(2\cos(3x)\sin(10t)\) → Stationary wave
- (b) \(2\sqrt{x-vt}\) → None (undefined for \(x < vt\))
- (c) \(3\sin(5x-0.5t)+4\cos(5x-0.5t)\) → Travelling wave (amplitude 5 m)
- (d) \(\cos x\sin t + \cos 2x\sin 2t\) → None (superposition of two different stationary waves)
When a string is fixed at both ends and set into vibration, only specific frequencies — called natural frequencies or harmonics — are sustained. The lowest such frequency is the fundamental mode (first harmonic), where exactly half a wavelength fits along the string: \(L = \lambda/2\), so \(\lambda = 2L\). Higher harmonics follow as \(L = n\lambda/2\) for integer \(n\). Once the wavelength is known and the frequency is given, the wave speed follows from \(v = f\lambda\). The tension is then extracted from \(T = \mu v^2\). A subtle but important step here is that the length of the wire is not given directly — it must be computed from the given mass \(m\) and linear mass density \(\mu\) using \(L = m/\mu\). Missing this step is a common error in competitive exams. This problem is a complete worked template for all string-resonance questions.
The wire is stretched between two rigid supports and vibrates in its fundamental mode. We first determine the length of the wire from the given mass and linear mass density.
\[\begin{aligned}L &= \frac{m}{\mu} = \frac{3.5\times10^{-2}}{4.0\times10^{-2}} = 0.875\ \text{m}\end{aligned}\]
In the fundamental mode, the length of the string equals half the wavelength of the stationary wave:
\[\lambda = 2L = 2\times 0.875 = 1.75\ \text{m}\]
The speed of the transverse wave is
\[\begin{aligned}v &= f\lambda = 45\times 1.75 = 78.75\ \text{m s}^{-1}\end{aligned}\]
Using the relation \(v = \sqrt{T/\mu}\), the tension is
\[\begin{aligned}T &= \mu v^2 = (4.0\times10^{-2})(78.75)^2 \approx 248\ \text{N} \approx 2.48\times10^{2}\ \text{N}\end{aligned}\]
- Speed of transverse wave: 78.75 m s⁻¹ ≈ 78.8 m s⁻¹
- Tension in the string: \(2.48\times10^{2}\ \text{N}\)
A tube open at one end and closed at the other (like a resonance column with a piston) supports only odd harmonics. Resonance occurs when the tube length satisfies \(L = (2n-1)\lambda/4\) for integers \(n = 1, 2, 3,\ldots\). For two successive resonances at lengths \(L_1\) and \(L_2\), the difference is \(L_2 - L_1 = \lambda/2\), giving \(\lambda = 2(L_2 - L_1)\). This elegant result eliminates the need to know which harmonic is excited — a crucial advantage in the resonance column experiment where end corrections can shift the absolute positions but not the difference. The speed of sound is then \(v = f\lambda\). This exact experimental method is used in school laboratories and the associated calculation appears in almost every NEET paper and frequently in JEE Main.
The tube is open at one end and closed at the other by a movable piston. The two resonant lengths are \(L_1 = 25.5\ \text{cm}\) and \(L_2 = 79.3\ \text{cm}\). For a pipe closed at one end, the difference between two successive resonant lengths equals half the wavelength.
\[\begin{aligned}\Delta L &= L_2 - L_1 = 79.3 - 25.5 = 53.8\ \text{cm}\end{aligned}\]
Therefore, the wavelength of sound in air is
\[\begin{aligned}\lambda &= 2\Delta L = 2\times 53.8 = 107.6\ \text{cm} = 1.076\ \text{m}\end{aligned}\]
The speed of sound in air at the experimental temperature is obtained using \(v = f\lambda\):
\[\begin{aligned}v &= 340\times 1.076 \approx 3.66\times10^{2}\ \text{m s}^{-1}\end{aligned}\]
The speed of sound in air at the temperature of the experiment is approximately \(3.66\times10^{2}\ \text{m s}^{-1}\).
When a rod is clamped at its centre and set into longitudinal vibration, the clamping point becomes a displacement node (the rod cannot move there) while both free ends become displacement antinodes. In the fundamental mode, one full half-wavelength spans the entire rod: the node is at the centre and antinodes are at both ends. This is identical to the vibration pattern of an open organ pipe, and the fundamental frequency condition is \(L = \lambda/2\), giving \(\lambda = 2L\). The speed of longitudinal sound in the steel is then \(v = f\lambda\). This problem reinforces that the same resonance condition \(L = \lambda/2\) applies to any system with two free ends — whether it be an open pipe, a free rod, or a bar struck at its end. The result (~5060 m s⁻¹) is a well-known benchmark for the speed of sound in steel.
The steel rod has a total length of \(L = 100\ \text{cm} = 1.0\ \text{m}\) and is clamped at its middle. When clamped at the centre, longitudinal vibrations produce a node at the clamp and antinodes at both free ends. In the fundamental mode, the length of the rod equals half the wavelength:
\[\lambda = 2L = 2\times 1.0 = 2.0\ \text{m}\]
The fundamental frequency is \(f = 2.53\ \text{kHz} = 2.53\times10^{3}\ \text{Hz}\). The speed of sound in steel is
\[\begin{aligned}v &= f\lambda = (2.53\times10^{3})\times 2.0 = 5.06\times10^{3}\ \text{m s}^{-1}\end{aligned}\]
The speed of sound in steel is approximately \(5.06\times10^{3}\ \text{m s}^{-1}\).
Two key rules govern organ pipe resonance:
Closed pipe (one end closed, one open): only odd harmonics are supported. Resonant frequencies are \(f_n = (2n-1)v/4L\) for \(n = 1, 2, 3,\ldots\) — giving \(f_1, 3f_1, 5f_1,\ldots\)
Open pipe (both ends open): all harmonics are supported. Resonant frequencies are \(f_n = nv/2L\) for \(n = 1, 2, 3,\ldots\) — giving \(f_1, 2f_1, 3f_1,\ldots\)
The fundamental of a closed pipe (\(v/4L\)) is exactly half that of an open pipe (\(v/2L\)) of the same length. A given source frequency will resonate with a pipe only if it exactly matches one of the pipe's natural frequencies. This exercise is a clean test of whether students can correctly identify which mode is excited — and recognise when no resonance is possible.
The pipe has length \(L = 20\ \text{cm} = 0.20\ \text{m}\).
The fundamental frequency (first harmonic) of a closed pipe is
\[\begin{aligned}f_1 &= \frac{v}{4L} = \frac{340}{4\times0.20} = \frac{340}{0.80} = 425\ \text{Hz}\end{aligned}\]
The source frequency is 430 Hz, which is very close to 425 Hz. Let us check if 430 Hz matches a higher harmonic more exactly. The resonant frequencies of the closed pipe are \(425\ \text{Hz},\ 1275\ \text{Hz},\ 2125\ \text{Hz},\ldots\) None exactly matches 430 Hz, but 425 Hz is close enough to consider the fundamental as resonantly excited — the small deviation (5 Hz) arises due to the neglected end correction. For the purposes of this problem, 430 Hz excites the fundamental mode (first harmonic) of the closed pipe.
The fundamental frequency of an open pipe of the same length is
\[\begin{aligned}f_1 &= \frac{v}{2L} = \frac{340}{2\times0.20} = \frac{340}{0.40} = 850\ \text{Hz}\end{aligned}\]
The resonant frequencies of the open pipe are \(850\ \text{Hz},\ 1700\ \text{Hz},\ 2550\ \text{Hz},\ldots\) The source frequency 430 Hz does not match any of these. Therefore, the 430 Hz source will not produce resonance when the pipe is open at both ends.
- Closed pipe: 430 Hz excites the fundamental mode (1st harmonic)
- Open pipe: no resonance — 430 Hz matches no harmonic of the open pipe
When two sound waves of slightly different frequencies \(f_1\) and \(f_2\) are superimposed, the resulting amplitude oscillates at a rate equal to the difference in frequencies: beat frequency \(= |f_1 - f_2|\). This gives the magnitude of the frequency difference, but not the sign — we cannot yet tell which string is higher. The resolution comes from a secondary observation: how the beat frequency changes when the tension in one string is altered. Since frequency is proportional to \(\sqrt{T}\), reducing the tension of string A lowers its frequency. If the new beat frequency decreases, it means A's frequency is moving closer to B's — so B must be on the side towards which A is moving, i.e., B is below A. If instead the beat frequency increased, B would be above A. This logical deduction eliminates one of the two possibilities and pinpoints the unique answer. This reasoning pattern — using a deliberate perturbation to identify the direction of frequency difference — appears regularly in JEE and NEET.
Let the original frequency of string A be \(f_A = 324\ \text{Hz}\) and that of string B be \(f_B\). The initial beat frequency is 6 Hz, so
\[|f_A - f_B| = |324 - f_B| = 6\]
This gives two possible values:
\[f_B = 330\ \text{Hz} \quad \text{or} \quad f_B = 318\ \text{Hz}\]
Now, the tension in string A is slightly reduced. Since \(f \propto \sqrt{T}\), reducing the tension lowers the frequency of string A — its new frequency is less than 324 Hz. The observed beat frequency decreases from 6 Hz to 3 Hz. This means the frequency of A is approaching that of B — i.e., A and B are getting closer in frequency. Since A's frequency is falling, B's frequency must be below the original 324 Hz.
Therefore, the only consistent value is
\[f_B = 318\ \text{Hz}\]
Verification: after reducing tension, if \(f_A\) falls to, say, 321 Hz, then \(|321 - 318| = 3\ \text{Hz}\). ✓ This matches the observed new beat frequency.
The frequency of sitar string B is 318 Hz.
This final exercise is qualitatively the richest in the entire chapter — and arguably the most JEE Advanced-aligned, as it tests the breadth and depth of conceptual understanding across five distinct ideas: the phase relationship between displacement and pressure in sound waves, biological ultrasound (echolocation), acoustic timbre, the role of shear rigidity in transverse wave propagation, and the phenomenon of wave dispersion. Each sub-part has appeared as a standalone assertion-reason question or conceptual MCQ in JEE Advanced, NEET, and BITSAT. The student who can articulate precise, physically grounded answers to all five parts has truly mastered the conceptual landscape of this chapter.
In a sound wave, particles oscillate along the direction of propagation. At a displacement node, the particles are permanently at rest at their mean positions — they do not move. However, neighbouring particles on both sides alternately crowd towards and away from the node. This results in maximum compression and rarefaction occurring right at the node — making it a region of maximum pressure variation, i.e., a pressure antinode. Conversely, at a displacement antinode, particles have maximum displacement — they move the most. Their oscillation spreads them out symmetrically, and the pressure fluctuations at this location cancel out, resulting in minimum pressure variation — a pressure node. This 90° phase difference between displacement and pressure is mathematically expressed as: if displacement goes as \(\sin(kx)\cos(\omega t)\), then pressure variation goes as \(\cos(kx)\sin(\omega t)\).
Bats emit short, high-frequency ultrasonic pulses (typically 20–200 kHz) from their larynx or nose. When these pulses encounter an object — a moth, a tree branch, a wall — they are partially reflected as echoes back to the bat's highly sensitive ears. By measuring the time delay between emission and reception, the bat calculates the distance to the object (using \(d = v_{sound}\times\Delta t/2\)). The direction is determined by comparing the relative intensity and timing of echoes received by each ear. The size and nature of the object are inferred from the amplitude spectrum, frequency shift (Doppler effect from moving prey), and the pattern of echo reflections. This biological sonar system — known as echolocation — is extraordinarily precise: bats can detect wires as thin as 0.1 mm in complete darkness.
Two musical notes can share the same fundamental frequency (hence the same pitch) and yet sound entirely different because of their timbre (tone quality). When a violin or sitar string vibrates, it does not produce a single pure frequency — it simultaneously produces the fundamental and a set of overtones (higher harmonics: \(2f_1, 3f_1, 4f_1,\ldots\)). The violin and sitar differ in their physical construction — the shape and material of the resonating body, the nature of the string, the method of excitation (bow vs. plectrum). These physical differences mean that the relative amplitudes (intensities) of the harmonics are different for each instrument. The resulting complex waveforms, though having the same fundamental period, have different shapes — and the human auditory system, acting like a Fourier analyser, perceives these different harmonic spectra as distinct timbres.
A transverse wave requires the medium to exert a restoring force when sheared — i.e., when adjacent layers are displaced perpendicular to the wave direction. This restoring force is characterised by the shear modulus of the medium. Solids possess a non-zero shear modulus because their atoms are bound in a fixed lattice — they resist being slid past each other. Therefore, solids can sustain transverse waves. Gases (and liquids) have essentially zero shear modulus — their molecules can flow freely past each other and offer no resistance to shear deformation. Hence, no restoring force is generated for transverse displacements, and transverse waves cannot propagate. Gases can only sustain longitudinal (compressional) waves, where the restoring force arises from the bulk modulus (resistance to compression).
A dispersive medium is one in which the speed of wave propagation depends on the frequency (or wavelength) of the wave: \(v = v(f)\). A pulse — any non-sinusoidal disturbance — is mathematically equivalent to a superposition of many different frequency components (a Fourier series or integral). In a non-dispersive medium (like a string or air for sound), all frequency components travel at the same speed, so the pulse shape is preserved indefinitely. In a dispersive medium, however, each frequency component travels at a different speed. The components therefore arrive at different times at a given point — some race ahead, others fall behind. The pulse, initially compact, gradually spreads out and its shape changes as it travels. This phenomenon is called dispersion. It is responsible for the separation of white light into its spectrum through a prism, for the distortion of digital signals in optical fibres, and for the spreading of ocean wave packets.
- (a) At a displacement node, maximum compression/rarefaction occurs → pressure antinode. At a displacement antinode, pressure variations cancel → pressure node.
- (b) Bats use echolocation: time delay → distance; intensity/arrival time difference → direction; Doppler shift and echo pattern → size and nature.
- (c) Same fundamental frequency but different harmonic spectra (timbre) — the relative intensities of overtones differ between instruments.
- (d) Transverse waves require non-zero shear modulus. Solids have it; gases do not — hence only longitudinal waves in gases.
- (e) In a dispersive medium, different frequency components travel at different speeds, causing the pulse to spread and distort over time.