13.1 Periodic and Oscillatory Motion
A motion is periodic if it repeats itself, identically, after equal intervals of time. That interval is the period . The Earth going around the Sun, a clock’s hour hand, a swinging pendulum, a vibrating guitar string, even the Earth spinning on its own axis, are all periodic in this sense, even though almost nothing else about them is alike.
A narrower and more useful category is oscillatory (or vibratory) motion: periodic motion that is also to-and-fro about a fixed mean (equilibrium) position, a pendulum swinging left and right of vertical, a block on a spring sliding past and back through its rest point, an atom in a solid jiggling about its lattice site. Every oscillation is periodic, but the reverse is not true. A satellite in uniform circular motion repeats its position every orbit, so it is periodic, yet it never reverses direction or retraces its path back through a single equilibrium point, so it is not oscillatory in this specific sense.
The reciprocal of the period is the frequency, , measured in hertz (Hz), one complete repetition per second. Together, and say nothing about what is oscillating, position, pressure, voltage, the electric field in a light wave, only how quickly the repetition happens, which is exactly why the same two numbers describe a pendulum and a radio wave equally well.
13.2 Simple Harmonic Motion, and its Connection to Uniform Circular Motion
Among all periodic motions, one family is both the simplest to describe and, remarkably, the one nature keeps reproducing whenever a system is nudged slightly away from a stable equilibrium: simple harmonic motion (SHM). A particle executes SHM if its displacement from the mean position varies with time as
Here , the amplitude, is the greatest displacement on either side of the mean position (always taken positive); the full argument is the phase, which fixes exactly where in the cycle the particle is at time ; and , the phase constant (or initial phase), is just the phase’s value at , fixed by wherever and however the oscillation was started. The constant is the angular frequency, related to the period and frequency by , since cosine repeats whenever its argument advances by exactly .
13.2.1 SHM as the Shadow of Circular Motion
The clean way to see why a cosine, specifically, is the natural shape for an oscillation is to stop thinking about the oscillation directly and look instead at uniform circular motion. Let a point move at constant angular speed around a circle of radius centred at the origin , starting at at an angle to the x-axis. At time , its angular position has advanced to .
Now drop a perpendicular from onto the x-axis, and track where its foot, call it , lands. By plain trigonometry, sits at , exactly the SHM equation above. As sweeps around the circle at a perfectly steady rate, is forced to slide back and forth along the diameter between and , racing through the centre and slowing almost to a stop at the two ends, which is precisely the to-and-fro feel of a real oscillation. SHM is nothing more exotic than this: the projection of uniform circular motion onto a diameter. (Project onto the perpendicular diameter instead and you get , the same motion, just a quarter-cycle out of step, which is also why sine and cosine are interchangeable descriptions of SHM up to a shift in .)
13.3 Velocity, Acceleration and the Force Law for SHM
Differentiating the displacement once gives the velocity, and again gives the acceleration:
Speed is greatest, , exactly at the mean position, and falls to zero at the two extremes; acceleration behaves exactly oppositely, zero at the mean position and greatest, , at the extremes. The relation is worth isolating on its own, because it is really the defining property of SHM, stripped of any reference to time:
acceleration is always directly proportional to the displacement from the mean position, and always directed opposite to it, back toward the mean position. This statement runs both ways: any system whose acceleration obeys for some constant , whatever the underlying physics, is guaranteed to execute SHM with that .
13.3.1 The Force Law
Multiply through by mass and Newton’s second law converts this straight into a force law. With , writing gives the familiar
a restoring force directly proportional to displacement and always pointed back toward equilibrium, with , the force constant, setting how stiffly the system resists being displaced. This is just Hooke’s law, and it is the real content of “SHM”: whenever the restoring force on a system is exactly linear in displacement, the motion that follows is automatically sinusoidal, for reasons that have nothing to do with springs specifically.
Worked example
Reading an oscillation off its equation
A particle’s displacement is given by cm, with in seconds. Find the amplitude, period, frequency, maximum speed and maximum acceleration, and locate the particle at .
Matching against directly gives:
and at :
so the particle starts already past the mean position, 5.20 cm out of a possible 6 cm, and moving back toward the centre.
13.4 Energy in Simple Harmonic Motion
An oscillator is constantly trading kinetic energy for potential energy and back. Using from above, the kinetic energy is
and the potential energy stored against the restoring force , taking at the mean position, is the familiar spring potential energy evaluated at the instantaneous displacement,
Add them, and the time-dependence cancels completely, since :
constant, for all time, and fixed entirely by the amplitude and the force constant. In words: and each oscillate between and , but at twice the angular frequency of itself (because they depend on squares of sine and cosine), and they are exactly out of step with each other: peaks at the two extremes , where the particle is momentarily at rest, and peaks at the mean position, where speed is greatest. The two curves cross, each equal to half the total energy, at . None of this requires any outside energy input, it is simply energy shuttling between two forms, and it is exactly the conservation law you would expect from a force that does no net work over a full cycle.
Worked example
Splitting the energy at a given displacement
A 0.5 kg block on a spring of force constant 20 N/m oscillates with amplitude 10 cm. Find the total energy, and the kinetic and potential energy when the block is 5 cm from the mean position.
Total energy, from the amplitude alone:
Potential energy at m:
and kinetic energy is whatever is left of the total:
As a check, with gives m²/s², so J independently, confirming the split.
13.5 Some Systems Executing SHM: the Spring-Block Oscillator and the Simple Pendulum
SHM is not a special trick a spring performs, it is what any system with a linear restoring force does. Two standard examples from the chapter make the point from opposite directions: one where the force law is exactly linear, and one where it only approximately is.
13.5.1 The Spring-Block Oscillator
A block of mass on a spring of force constant , sliding on a frictionless surface, feels exactly , so , which is with . The period follows immediately:
Notice what is not in this formula: the amplitude. Pull the block out 2 cm or 12 cm, within the spring’s linear range, and it takes exactly the same time to complete one cycle either way, because never involved in the first place. This amplitude-independence of the period is called isochronism, and it is exactly what the phase-space view in the simulation below makes visible: dragging the amplitude slider inflates the ellipse traced by , but never stretches or compresses it along the time axis, so the dot completes one lap in the same time regardless of the ellipse’s size.
Worked example
Same spring, two amplitudes, same period
A 0.5 kg block sits on a spring with N/m, the same values the simulation defaults to. Compare the period when it is released from 5 cm versus from 12 cm.
for both amplitudes: never entered the calculation of , so it cannot affect . Only the ellipse’s size, and the maximum speed at its widest point, change between the two cases.
13.5.2 The Simple Pendulum
A bob of mass hangs from a light, inextensible string of length , displaced through angle from the vertical. Along the arc, the only unbalanced force is the tangential component of gravity, (the string tension handles the radial part), so with arc-length displacement , Newton’s second law along the arc reads
This is not yet SHM, is not proportional to . But for small (in radians), , which turns the force into , linear in at last, giving and
Notice this entire derivation leaned on one approximation, , valid only while stays small, roughly under 10°, where the two differ by less than half a percent. Swing the pendulum through a larger arc and falls measurably below , so the real restoring force is weaker than the ideal linear force this formula assumes, especially near the extremes of the swing. The practical effect is that the period creeps up with amplitude for large swings, isochronism breaks down, for precisely the reason the spring-block’s isochronism depended on being exactly linear: the pendulum’s force law is only ever approximately linear, and only at small amplitude. The interactive simulation’s amplitude slider is built around the clean spring case precisely so this assumption is visible by contrast, an ideal spring never develops this drift, however large the amplitude, as long as it stays in its linear range.
Worked example
Period of a one-metre pendulum
Estimate the period of small oscillations of a simple pendulum 1.0 m long, taking m/s².
which is why a pendulum built to tick out whole seconds (half a swing per tick) ends up close to a metre long, essentially the reasoning behind every pendulum clock.
13.6 Damped Oscillations and Forced Oscillations, Resonance
Every real oscillator loses some energy, to air resistance, internal friction, or some other drag. Model that loss as a damping force proportional to velocity, , acting alongside the restoring force, and the amplitude no longer stays fixed, it decays exponentially with time:
with a slightly lower angular frequency than the undamped value. Larger means faster decay; the mechanical energy, tracking the square of the amplitude, falls off as . A swing left alone, or a plucked guitar string fading out, are both damped oscillators.
Push a damped oscillator with an external periodic force at some driving frequency and, once the initial transient dies away, it settles into steady oscillation at itself, not at its own natural frequency , with an amplitude that depends on how close is to and how strong the damping is. As approaches , the driving force pumps energy in step with the system’s own rhythm on every cycle, and the amplitude grows sharply, a phenomenon called resonance, limited in practice only by however much damping is present. Soldiers breaking step while crossing a bridge, rather than marching in time, exist as a rule precisely because a matched rhythm can pump a bridge’s own oscillation to dangerous amplitude; a sustained note at just the right pitch can do the same to a wine glass, shattering it, and a child’s swing climbs highest when each push lands in step with the swing’s own natural frequency rather than at some arbitrary rhythm.
— From the NCERT exercises
Two of the chapter’s own exercise questions, with original worked solutions.
NCERT Exercise 13.9
A spring with force constant 1200 N/m is mounted on a horizontal frictionless surface, with a 3 kg block attached to its free end. The block is pulled sideways to a distance of 2.0 cm from its equilibrium position and released. Find (a) the frequency of the resulting oscillations, (b) the maximum acceleration of the block, and (c) its maximum speed.
Solution
The angular frequency depends only on and :
With amplitude m:
NCERT Exercise 13.14
The acceleration due to gravity on the surface of the Moon is 1.7 m/s². A simple pendulum has a time period of 3.5 s on the surface of the Earth, where g = 9.8 m/s². What is the time period of the same pendulum on the surface of the Moon?
Solution
The pendulum’s length does not change between the two locations, so from , is the same on both:
Weaker lunar gravity gives a much weaker restoring force for the same displacement, so each swing takes noticeably longer, more than double the Earth period, even though nothing about the pendulum itself changed.
