Physics: Class 11 (Book 2) — Chapter 13: Oscillations

13.1 Introduction to Oscillatory Motion

In physical systems, motion can be broadly classified into repetitive and non-repetitive categories. While rectilinear and projectile motions are non-repetitive, orbital and circular motions repeat at regular intervals. A special class of repetitive motion is oscillatory motion , where an object moves to and fro about a stable equilibrium position.

Periodic vs. Oscillatory Motion
  • Periodic Motion: Any motion that repeats itself at regular, equal intervals of time (e.g., the orbital revolution of planets).
  • Oscillatory Motion: A periodic motion in which the system moves back and forth about a central mean position (e.g., a swinging pendulum, a vibrating violin string).
  • Key Distinction: Every oscillatory motion is periodic, but not every periodic motion is oscillatory (e.g., uniform circular motion is periodic but not to-and-fro).
Oscillations vs. Vibrations

While there is no strict physical boundary between the two terms, they are generally distinguished by their frequency scales:

  • Oscillation: Typically refers to low-frequency macroscopic movements, such as the swaying of a tree branch or the motion of a swing.
  • Vibration: Typically refers to high-frequency microscopic movements, such as the rapid motion of atoms in a crystal lattice or a musical instrument string.
13.2 Period, Frequency, and Displacement

To quantitatively describe periodic and oscillatory systems, we define fundamental physical parameters that characterize their temporal and spatial behavior.

Period and Frequency

The temporal characteristics of periodic motion are defined by the time interval of repetition and its rate:

  • Period ($T$): The smallest interval of time after which the motion repeats itself. The SI unit of period is the second ( s ).
  • Frequency ($\nu$): The number of repetitions or cycles that occur per unit time. It is mathematically defined as the reciprocal of the period:$$\nu = \frac{1}{T}$$The SI unit of frequency is the hertz ( Hz ), where $1 \text{ Hz} = 1 \text{ s}^{-1}$.

Mathematical Problem Statement: On average, a human heart is found to beat 75 \times in a minute. Calculate its frequency and period.


Step-by-Step Algorithmic Solution Trace:

  1. Identify the total number of cycles ($N = 75$) and the total time interval ($t = 60 \text{ s}$).
  2. Calculate the frequency ($\nu$) as the number of cycles per second:$$\nu = \frac{75}{60 \text{ s}} = 1.25 \text{ Hz}$$
  3. Calculate the time period ($T$) as the reciprocal of the frequency:$$T = \frac{1}{\nu} = \frac{1}{1.25 \text{ s}^{-1}} = 0.8 \text{ s}$$

Final Evaluation Output: Frequency $\nu = 1.25 \text{ Hz}$, Time Period $T = 0.8 \text{ s}$

Generalized Displacement

In the context of oscillations, displacement is generalized beyond spatial coordinates to represent the change in any physical property over time:

  • Mechanical Systems: Position coordinates ($x(t)$) or angular position ($\theta(t)$) for a simple pendulum.
  • Electrical Systems: The time-varying voltage across a capacitor in an AC circuit.
  • Electromagnetic Systems: The oscillating electric ($E$) and magnetic ($B$) field vectors in a propagating light wave.
  • Acoustic Systems: Pressure variations in a medium during sound propagation.

Mathematically, the simplest periodic displacement function is represented by a sinusoidal function of time:$$f(t) = A \cos \omega t$$By the Fourier theorem , any complex periodic function can be expressed as a linear superposition of sine and cosine functions of different periods with appropriate coefficients:$$f(t) = A \sin \omega t + B \cos \omega t = D \sin(\omega t + \phi)$$where $D = \sqrt{A^2 + B^2}$ and $\phi = \tan^{-1}(B/A)$.

13.3 Simple Harmonic Motion (SHM)

Simple Harmonic Motion is the fundamental building block of oscillatory systems. It is defined as a periodic motion where the displacement is a sinusoidal function of time.

Mathematical Formulation

The instantaneous displacement $x(t)$ of a particle executing SHM along the x-axis is given by:$$x(t) = A \cos(\omega t + \phi)$$Where the parameters are defined as follows:

  • Amplitude ($A$): The magnitude of the maximum displacement of the particle from its mean position.
  • Angular Frequency ($\omega$): The rate of change of phase, related to the period $T$ by:$$\omega = \frac{2\pi}{T}$$The SI unit of angular frequency is radians per second ( rad/s ).
  • Phase ($ \omega t + \phi $): The time-dependent argument of the cosine function that determines the state of motion (position and velocity) at any instant $t$.
  • Phase Constant ($\phi$): The initial phase angle at $t = 0$, determined by the initial position and velocity of the particle.

13.4 Simple Harmonic Motion and Uniform Circular Motion

There is a direct geometric relationship between simple harmonic motion and uniform circular motion. The projection of a particle moving uniformly on a circle (called the reference circle ) onto any of its diameters executes simple harmonic motion.

Geometric Projection Proof
  1. Consider a reference particle $P$ moving with constant angular speed $\omega$ on a circle of radius $A$.
  2. Let the initial position vector $\vec{OP}$ at $t = 0$ make an angle $\phi$ with the positive x-axis.
  3. At any time $t$, the position vector $\vec{OP}$ makes an angle $(\omega t + \phi)$ with the positive x-axis.
  4. The projection of $P$ onto the x-axis (point $P'$) has a position coordinate given by:$$x(t) = A \cos(\omega t + \phi)$$
  5. The projection of $P$ onto the y-axis (point $P''$) has a position coordinate given by:$$y(t) = A \sin(\omega t + \phi)$$

This proves that the projection of uniform circular motion on any diameter is mathematically identical to linear simple harmonic motion.

13.5 Velocity and Acceleration in Simple Harmonic Motion

The kinematic variables of a particle executing SHM can be derived directly by differentiating the displacement function with respect to time.

Derivation of Velocity

The instantaneous velocity $v(t)$ is the time derivative of displacement:$$v(t) = \frac{d}{dt}[A \cos(\omega t + \phi)] = -\omega A \sin(\omega t + \phi)$$

  • The maximum speed (velocity amplitude) is $v_m = \omega A$, occurring at the mean position ($x = 0$).
  • The velocity is zero at the extreme positions ($x = \pm A$).
  • The velocity function has a phase difference of $\pi/2$ relative to the displacement function.

Derivation of Acceleration

The instantaneous acceleration $a(t)$ is the time derivative of velocity:$$a(t) = \frac{d}{dt}[-\omega A \sin(\omega t + \phi)] = -\omega^2 A \cos(\omega t + \phi)$$Substituting the displacement equation $x(t) = A \cos(\omega t + \phi)$ yields:$$a(t) = -\omega^2 x(t)$$

  • The acceleration is directly proportional to the displacement but opposite in direction (always directed towards the mean position).
  • The maximum acceleration amplitude is $a_m = \omega^2 A$, occurring at the extreme positions ($x = \pm A$).
  • The acceleration is zero at the mean position ($x = 0$).
  • The acceleration function has a phase difference of $\pi$ relative to the displacement function.

Mathematical Problem Statement: A body oscillates with SHM according to the equation $x = 5 \cos[2\pi t + \pi/4]$ in SI units. At $t = 1.5 \text{ s}$, calculate the (a) displacement, (b) speed, and (c) acceleration of the body.


Step-by-Step Algorithmic Solution Trace:

  1. Identify the parameters from the given equation: Amplitude $A = 5 \text{ m}$, angular frequency $\omega = 2\pi \text{ s}^{-1}$, phase constant $\phi = \pi/4$.
  2. Calculate displacement at $t = 1.5 \text{ s}$:$$x(1.5) = 5 \cos[2\pi(1.5) + \pi/4] = 5 \cos[3\pi + \pi/4] = -5 \cos(\pi/4) = -5 \times 0.707 \text{ m} = -3.535 \text{ m}$$
  3. Calculate velocity at $t = 1.5 \text{ s}$:$$v(1.5) = -\omega A \sin(\omega t + \phi) = -(2\pi)(5) \sin[3\pi + \pi/4] = 10\pi \sin(\pi/4) = 10\pi \times 0.707 \text{ m/s} \approx 22 \text{ m/s}$$
  4. Calculate acceleration at $t = 1.5 \text{ s}$:$$a(1.5) = -\omega^2 x(1.5) = -(2\pi)^2 (-3.535 \text{ m}) = 4\pi^2 \times 3.535 \text{ m/s}^2 \approx 140 \text{ m/s}^2$$

Final Evaluation Output: Displacement $x = -3.535 \text{ m}$, Speed $v = 22 \text{ m/s}$, Acceleration $a = 140 \text{ m/s}^2$

13.6 Force Law for Simple Harmonic Motion

Using Newton's second law of motion ($F = ma$) and the kinematic expression for acceleration in SHM, we can establish the dynamic condition for simple harmonic motion.

Derivation of the Restoring Force

The force acting on a particle of mass $m$ executing SHM is:$$F(t) = ma(t) = -m\omega^2 x(t)$$Defining the force constant (or spring constant) as $k = m\omega^2$, the force law becomes:$$F(t) = -kx(t)$$

  • This is a linear restoring force, directly proportional to the displacement and directed opposite to it.
  • The angular frequency of the system is determined by its inertia ($m$) and stiffness ($k$):$$\omega = \sqrt{\frac{k}{m}}$$
  • The time period of the linear harmonic oscillator is:$$T = 2\pi\sqrt{\frac{m}{k}}$$

13.7 Energy in Simple Harmonic Motion

A particle executing SHM possesses both kinetic energy ($K$) due to its motion and potential energy ($U$) due to its displacement against the restoring force.

Kinetic Energy (K)

The kinetic energy of the particle at any instant $t$ is:$$K = \frac{1}{2}mv^2 = \frac{1}{2}m\omega^2 A^2 \sin^2(\omega t + \phi) = \frac{1}{2}kA^2 \sin^2(\omega t + \phi)$$Kinetic energy is maximum at the mean position ($x = 0$) and zero at the extreme positions ($x = \pm A$).

Potential Energy (U)

The potential energy of the particle, associated with the conservative restoring force $F = -kx$, is:$$U = \frac{1}{2}kx^2 = \frac{1}{2}kA^2 \cos^2(\omega t + \phi)$$Potential energy is zero at the mean position ($x = 0$) and maximum at the extreme positions ($x = \pm A$).

Total Mechanical Energy (E)

The total mechanical energy of the system is the sum of its kinetic and potential energies:$$E = K + U = \frac{1}{2}kA^2 [\sin^2(\omega t + \phi) + \cos^2(\omega t + \phi)]$$Using the trigonometric identity $\sin^2\theta + \cos^2\theta = 1$, we get:$$E = \frac{1}{2}kA^2$$

  • The total mechanical energy of a harmonic oscillator is constant and independent of time.
  • Energy continuously transforms between kinetic and potential forms during the cycle.
  • Both $K$ and $U$ oscillate with a frequency of $2\nu$ (period $T/2$).

Mathematical Problem Statement: A block of mass 1 kg is fastened to a spring with spring constant $k = 50 \text{ N/m}$. The block is pulled to a distance $x = 10 \text{ cm}$ from its equilibrium position on a frictionless surface and released from rest at $t = 0$. Calculate the kinetic, potential, and total energies of the block when it is 5 cm away from the mean position.


Step-by-Step Algorithmic Solution Trace:

  1. Identify the given parameters: Mass $m = 1 \text{ kg}$, spring constant $k = 50 \text{ N/m}$, amplitude $A = 0.1 \text{ m}$, and intermediate displacement $x = 0.05 \text{ m}$.
  2. Calculate the total mechanical energy ($E$):$$E = \frac{1}{2}kA^2 = \frac{1}{2}(50)(0.1)^2 = 0.25 \text{ J}$$
  3. Calculate the potential energy ($U$) at $x = 0.05 \text{ m}$:$$U = \frac{1}{2}kx^2 = \frac{1}{2}(50)(0.05)^2 = 0.0625 \text{ J}$$
  4. Calculate the kinetic energy ($K$) using conservation of energy ($K = E - U$):$$K = 0.25 \text{ J} - 0.0625 \text{ J} = 0.1875 \text{ J} \approx 0.19 \text{ J}$$

Final Evaluation Output: Potential Energy $U = 0.0625 \text{ J}$, Kinetic Energy $K = 0.19 \text{ J}$, Total Energy $E = 0.25 \text{ J}$

13.8 The Simple Pendulum

A simple pendulum consists of a small bob of mass $m$ suspended by a light, inextensible string of length $L$ from a rigid support.

Derivation of the Time Period
  1. Let the pendulum be displaced by a small angle $\theta$ from the vertical.
  2. The forces acting on the bob are:
    • Tension $\vec{T}$ along the string.
    • Gravitational force $m\vec{g}$ acting vertically downwards.
  3. Resolve $mg$ into two components: $mg \cos\theta$ along the string (balanced by tension) and $mg \sin\theta$ perpendicular to the string (providing the restoring force).
  4. The restoring torque $\tau$ about the support point is:$$\tau = -L(mg \sin\theta)$$
  5. Using Newton's rotational law $\tau = I\alpha$, where $I = mL^2$ is the moment of inertia:$$mL^2 \alpha = -mgL \sin\theta \implies \alpha = -\frac{g}{L} \sin\theta$$
  6. For small angular displacements ($\theta \ll 1$ radian), we apply the small-angle approximation $\sin\theta \approx \theta$:$$\alpha \approx -\frac{g}{L} \theta$$
  7. Comparing this with the SHM angular acceleration equation $\alpha = -\omega^2 \theta$, we find:$$\omega = \sqrt{\frac{g}{L}}$$
  8. The time period of a simple pendulum is:$$T = 2\pi\sqrt{\frac{L}{g}}$$

Mathematical Problem Statement: What is the length of a simple pendulum that ticks seconds (has a time period of exactly 2 s) at a location where $g = 9.8 \text{ m/s}^2$?


Step-by-Step Algorithmic Solution Trace:

  1. Identify the given parameters: Time period $T = 2 \text{ s}$, acceleration due to gravity $g = 9.8 \text{ m/s}^2$.
  2. Rearrange the pendulum period formula to solve for length $L$:$$T = 2\pi\sqrt{\frac{L}{g}} \implies T^2 = 4\pi^2 \frac{L}{g} \implies L = \frac{gT^2}{4\pi^2}$$
  3. Substitute the values into the equation:$$L = \frac{9.8 \times 2^2}{4\pi^2} = \frac{9.8 \times 4}{4\pi^2} = \frac{9.8}{\pi^2} \approx 0.993 \text{ m} \approx 1 \text{ m}$$

Final Evaluation Output: Length of the seconds pendulum $L \approx 1 \text{ m}$

13.9 Summary of Physical Quantities in Oscillations

The following table summarizes the key physical quantities, mathematical domains, and active formulas governing simple harmonic motion.

Structural Concept / Function Type Exact Mathematical Domain / Sign Properties Active Operation Formulas / Identities Systemic Role & Evaluation Limits
Displacement $[-A, A]$ $x(t) = A \cos(\omega t + \phi)$ Defines the instantaneous position relative to equilibrium.
Velocity $[-\omega A, \omega A]$ $v(t) = -\omega A \sin(\omega t + \phi)$ Measures rate of change of position; maximum at equilibrium ($x = 0$).
Acceleration $[-\omega^2 A, \omega^2 A]$ $a(t) = -\omega^2 x(t)$ Proportional and opposite to displacement; maximum at extremes ($x = \pm A$).
Restoring Force $[-kA, kA]$ $F(t) = -kx(t)$ Dynamic driver of SHM; always directed towards equilibrium.
Kinetic Energy $[0, \frac{1}{2}kA^2]$ $K = \frac{1}{2}kA^2 \sin^2(\omega t + \phi)$ Energy of motion; peaks twice per period at $x = 0$.
Potential Energy $[0, \frac{1}{2}kA^2]$ $U = \frac{1}{2}kx^2$ Stored elastic energy; peaks twice per period at $x = \pm A$.
Total Energy Constant: $\frac{1}{2}kA^2$ $E = K + U = \frac{1}{2}kA^2$ Conserved quantity; independent of time and position.

Historical Chronicle / Epigraph: Galileo Galilei & Heinrich Hertz

  • Historical Context & Milestones: Galileo Galilei (1564–1642) observed the isochronism of a swinging chandelier in the Cathedral of Pisa, using his pulse as a timer. Heinrich Rudolf Hertz (1857–1894) discovered radio waves, establishing the physical reality of electromagnetic oscillations.
  • Theoretical Foundations: The SI unit of frequency, the hertz ( Hz ), is named in honor of Hertz, representing one cycle per second ($1 \text{ Hz} = 1 \text{ s}^{-1}$). Galileo's work laid the foundation for the pendulum clock, later engineered by Christiaan Huygens.