Physics > Simple Harmonic Motion > 10.0 Method for Calculating Time Period of a Simple Harmonic Motion

  Simple Harmonic Motion
    1.0 Types of Motion
    2.0 Causes of Oscillation
    3.0 Solution of the Equation of SHM
    4.0 Kinematics of SHM equation i.e., $x = A\sin \left( {\omega t + \phi } \right)$
    5.0 Relation between Simple Harmonic Motion and Uniform Circular Motion
    6.0 Sign Convention of a Simple Harmonic Motion
    7.0 How to Write the Simple Harmonic Motion Equation
    8.0 Force and Energy in Simple Harmonic Motion
    9.0 Basic Differential Equation of SHM
    10.0 Method for Calculating Time Period of a Simple Harmonic Motion
    11.0 Spring Block System
    12.0 Physical Pendulum
    13.0 Vector Method of Combining Two or More Simple Harmonic Motions
    14.0 Simple Harmonic Oscillation of a Fluid Column

10.2 Energy Method
Step 1.

Find the stable equilibrium position, which is usually known, as the mean position. Net force or torque on the particle in this position is zero. Potential energy is minimum.


Step 2.

Displace the particle from its mean position by a small displacement $x$ (in case of linear SHM) or $\theta$ (in case of an angular SHM).


Step 3.

Find the total mechanical energy ($E$) in the displaced position. Since, mechanical energy in SHM remains constant. $$\frac{{dE}}{{dt}} = 0$$
By differentiating the energy equation with respect to time and substituting $$\frac{{dx}}{{dt}} = v,\frac{{d\theta }}{{dt}} = \omega ,\frac{{dv}}{{dt}} = a,\frac{{d\omega }}{{dt}} = \alpha $$
Convert linear acceleration and velocity into angular acceleration and velocity respectively.



Step 4.

Find the angular acceleration by dividing the above equation by mass $m$ and calculate the time period.



Example: The Simple Pendulum (Using Energy Method)

Let us derive the same expression by energy method. Suppose $\omega$ be the angular velocity of particle at angular displacement $\theta$ about point $O$.

Then, total mechanical energy of particle in position $P$ is,
$$\begin{equation} \begin{aligned} E = \frac{1}{2}I{\omega ^2} + mg\left( {{h_P} - {h_R}} \right) \\ E = \frac{1}{2}\left( {m{l^2}} \right){\omega ^2} + mgl\left( {1 - cos\theta } \right) \\ E{\text{ }}{\text{is constant}},{\text{therefore}},\frac{{dE}}{{dt}} = 0 \\ 0 = m{l^2}\omega \left( {\frac{{d\omega }}{{dt}}} \right) + mglsin\theta \left( {\frac{{d\theta }}{{dt}}} \right) \\\end{aligned} \end{equation} $$
Putting $$\frac{{d\theta }}{{dt}} = \omega ,\frac{{d\omega }}{{dt}} = \alpha {\text{ and }}sin\theta \approx \theta ,$$ we get the same expression i.e.,
$$\begin{equation} \begin{aligned} 0 = m{l^2}\omega \alpha + mgl\theta \omega \\ 0 = ml\omega \left( {l\alpha + g\theta } \right) \\\end{aligned} \end{equation} $$
Since, $$\begin{equation} \begin{aligned} ml\omega \ne 0, \\ \therefore \left( {l\alpha + g\theta } \right) = 0 \\\end{aligned} \end{equation} $$
$$\begin{equation} \begin{aligned} \alpha = - \left( {\frac{g}{l}} \right)\theta ..\left( A \right) \\ \alpha = - {\omega ^2}\theta \;\left( {{\text{SHM acceleration}}} \right)..\left( B \right) \\\end{aligned} \end{equation} $$
On equating $A$ & $B$ we get,
$$\begin{equation} \begin{aligned} \omega = \sqrt {\frac{g}{l}} ..\left( C \right) \\ T = \frac{{2\pi }}{\omega } \\ T = 2\pi \sqrt {\frac{l}{g}} \;\left( {{\text{from equation }}C} \right) \\\end{aligned} \end{equation} $$
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