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Physics · Ch 13 — Oscillations

Displacement

13.2.2

Displacement

The Meaning of Displacement in Oscillatory Motion

When we talk about displacement in the context of oscillations, we are not just talking about how far something has moved from where it started. In oscillatory motion, displacement has a very specific meaning: it is the distance of the oscillating particle from its mean position (or equilibrium position) at any given instant.

Think of a simple pendulum. The mean position is the point where the bob hangs vertically downwards, at rest. If you pull the bob to one side and release it, the displacement at any moment is the distance of the bob from that central, vertical line. This displacement can be positive (to the right of the mean position) or negative (to the left), depending on which side the bob is on.

The key idea is that displacement in an oscillation is always measured from the equilibrium point, not from the starting point of the motion. This is a crucial distinction from the displacement you might calculate in kinematics problems.

The Mathematical Description of Displacement

For the simplest kind of oscillation — simple harmonic motion (SHM) — the displacement x(t)x(t) varies sinusoidally with time tt. The most general way to write this is:

x(t)=Acos⁡(ωt+ϕ)x(t) = A \cos(\omega t + \phi)

Here, each symbol has a precise physical meaning:

  • x(t)x(t) is the displacement of the particle from its mean position at time tt.
  • AA is the amplitude of the motion. It is the maximum magnitude of displacement. The particle oscillates between x=+Ax = +A and x=−Ax = -A.
  • ω\omega is the angular frequency of the motion. It tells you how fast the oscillation is happening in terms of radians per second. It is related to the time period TT and frequency ff by ω=2πf=2πT\omega = 2\pi f = \frac{2\pi}{T}.
  • ϕ\phi is the initial phase (or phase constant). It determines the displacement of the particle at time t=0t = 0. If ϕ=0\phi = 0, then x(0)=Ax(0) = A, meaning the particle starts at its maximum positive displacement.

x(t)=Acos⁡(ωt+ϕ)x(t) = A \cos(\omega t + \phi)

This single equation is the foundation for describing the position of any particle executing SHM.

Why Use a Cosine Function?

You might wonder why we use a cosine and not a sine. The answer is that both are valid, and the choice simply affects the value of the phase constant ϕ\phi. A sine function is just a cosine function shifted in time:

sin⁡(ωt)=cos⁡(ωt−π/2)\sin(\omega t) = \cos(\omega t - \pi/2)

So, if you prefer to write x(t)=Asin⁡(ωt+ϕ′)x(t) = A \sin(\omega t + \phi'), you can, and it will describe the same physical motion, just with a different phase constant. The textbook uses the cosine form as its standard representation, and we will stick with that for consistency.

The Four Key Quantities of SHM

From the displacement equation x(t)=Acos⁡(ωt+ϕ)x(t) = A \cos(\omega t + \phi), we can derive everything else about the motion. The textbook lists four fundamental quantities that completely define a simple harmonic motion:

  1. Amplitude (AA): The maximum displacement from the mean position. It is always a positive constant.
  2. Angular Frequency (ω\omega): A measure of how rapidly the oscillations occur. It is a positive constant for a given system.
  3. Phase (ωt+ϕ\omega t + \phi): The argument of the cosine function. It tells you the current "state" of the oscillation — where the particle is in its cycle.
  4. Initial Phase (ϕ\phi): The phase at time t=0t = 0. It sets the initial conditions of the motion.

Properties of the Displacement Function

The textbook then examines the mathematical properties of the cosine function to understand the physical behaviour of the oscillating particle. Let's go through them one by one.

›Proof

Property (I): The motion is periodic.

A function f(t)f(t) is periodic with period TT if f(t+T)=f(t)f(t+T) = f(t) for all tt. For our displacement function x(t)=Acos⁡(ωt+ϕ)x(t) = A \cos(\omega t + \phi), we need to find a TT such that:

Acos⁡(ω(t+T)+ϕ)=Acos⁡(ωt+ϕ)A \cos(\omega (t+T) + \phi) = A \cos(\omega t + \phi)

We know that the cosine function repeats its value when its argument increases by 2π2\pi:

cos⁡(θ+2π)=cos⁡(θ)\cos(\theta + 2\pi) = \cos(\theta)

Therefore, we require:

ω(t+T)+ϕ=ωt+ϕ+2π\omega (t+T) + \phi = \omega t + \phi + 2\pi

Simplifying:

ωt+ωT+ϕ=ωt+ϕ+2π\omega t + \omega T + \phi = \omega t + \phi + 2\pi

Cancelling ωt\omega t and ϕ\phi from both sides gives:

ωT=2π\omega T = 2\pi

So the time period TT is:

T=2πωT = \frac{2\pi}{\omega}

This proves that x(t)x(t) is a periodic function with a period T=2π/ωT = 2\pi/\omega. The particle repeats its motion after every interval TT.

›Proof

Property (II): The motion is oscillatory about the mean position.

An oscillatory motion is one in which the particle moves back and forth about a fixed point (the mean position). The displacement function x(t)=Acos⁡(ωt+ϕ)x(t) = A \cos(\omega t + \phi) clearly shows this. The cosine function oscillates between −1-1 and +1+1. Therefore, x(t)x(t) oscillates between −A-A and +A+A. The value x=0x=0 (the mean position) is crossed twice in every cycle. This back-and-forth motion about x=0x=0 is the very definition of oscillation.

›Proof

Property (III): The amplitude AA is the maximum displacement.

The maximum value of cos⁡(ωt+ϕ)\cos(\omega t + \phi) is +1+1. Therefore, the maximum value of x(t)x(t) is:

xmax=A×(+1)=Ax_{\text{max}} = A \times (+1) = A

The minimum value of cos⁡(ωt+ϕ)\cos(\omega t + \phi) is −1-1. Therefore, the minimum value of x(t)x(t) is:

xmin=A×(−1)=−Ax_{\text{min}} = A \times (-1) = -A

The magnitude of the maximum displacement from the mean position is ∣A∣|A|. Since amplitude is defined as this maximum magnitude, it is AA (taking AA to be positive).

›Proof

Property (IV): The phase (ωt+ϕ)(\omega t + \phi) determines the state of motion.

…

Figure 13.2.aA block attached to a spring, the other end fixed to a rigid wall. The block moves on a frictionless surface; motion described by displacement x from equilibrium.
Fig. 13.2.a — A block attached to a spring, the other end fixed to a rigid wall. The block moves on a frictionless surface; motion described by displacement x from equilibrium.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your NCERT textbook's own diagram.

This figure is the starting point for understanding simple harmonic motion (SHM). It shows the simplest possible oscillator: a single block attached to a spring, with the other end of the spring fixed to a rigid wall. The surface is frictionless, so the only horizontal force on the block comes from the spring.

The diagram has two key parts. On the left is the equilibrium position — the block is drawn in blue, sitting where the spring is neither stretched nor compressed. On the right, a second block is drawn in grey, displaced to the right by a distance xx from equilibrium. A double-headed arrow labelled xx spans the gap between the two block positions, making it clear that xx measures the displacement from equilibrium, not the total length of the spring. The wall is hatched to show it is rigid and fixed; the surface is hatched to indicate it is frictionless.

The physical idea is straightforward: when you pull the block to the right (or push it to the left) and release it, the spring exerts a restoring force that tries to bring the block back to equilibrium. For a spring that obeys Hooke's law, that restoring force is proportional to the displacement and opposite in direction:

F=−kxF = -k x

Here FF is the force exerted by the spring on the block, kk is the spring constant (a measure of the spring's stiffness), and xx is the displacement from equilibrium. The negative sign is crucial — it tells you the force always points opposite to the displacement. If the block is to the right (x>0x > 0), the force pulls left; if the block is to the left (x<0x < 0), the force pushes right.

From this force law, Newton's second law (F=maF = ma) gives the equation of motion:

md2xdt2=−kxm \frac{d^2 x}{dt^2} = -k x

or, rearranged:

d2xdt2+kmx=0\frac{d^2 x}{dt^2} + \frac{k}{m} x = 0

This is the differential equation for simple harmonic motion. Its solution is a sinusoidal function of time:

x(t)=Acos⁡(ωt+ϕ)x(t) = A \cos(\omega t + \phi)

where AA is the amplitude (maximum displacement), ω=k/m\omega = \sqrt{k/m} is the angular frequency, and ϕ\phi is the initial phase (determined by where the block starts). The period TT of the oscillation is T=2π/ω=2πm/kT = 2\pi / \omega = 2\pi \sqrt{m/k}. …

Figure 13.2.bAn oscillating simple pendulum; its motion described by angular displacement θ from the vertical.
Fig. 13.2.b — An oscillating simple pendulum; its motion described by angular displacement θ from the vertical.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your NCERT textbook's own diagram.

The figure shows a simple pendulum hanging from a fixed support at the ceiling. A dashed vertical line marks the equilibrium position — where the pendulum hangs straight down when at rest. The string is drawn at an angle θ\theta to this vertical, with the bob at the end of the string. A curved double-headed arrow arcs between the vertical line and the string, indicating that θ\theta is the angular displacement from equilibrium. The bob is shown at one extreme of its swing, so the arrow captures the full range of motion the pendulum covers as it oscillates.

The physical idea is that a simple pendulum, when displaced by a small angle and released, undergoes periodic motion. The restoring force comes from gravity: the component of the bob's weight tangent to the arc, mgsin⁡θmg\sin\theta, always pulls it back toward the vertical. For small θ\theta (typically less than about 10∘10^\circ), sin⁡θ≈θ\sin\theta \approx \theta in radians, which makes the motion simple harmonic.

T=2πLgT = 2\pi\sqrt{\frac{L}{g}} …