Thursday, January 29, 2026

14.1 - Displacement of An Oscillating particle

In the previous section, we saw period and frequency. In this section, we will see displacement.

Let us first see the details of an oscillation. It can be written in 6 steps:
1. In fig.14.3 (a) below, a red block of mass m, is attached to a spring. The other end of the spring is fixed to a rigid wall. The block is resting on a friction-less surface.


Fig.14.9

2. In fig.14.3 (b), the block is pulled towards the right by a distance A. From this position, the block is released from rest. It will then travel towards the left. Even after traveling a distance 'A', it will continue to travel towards the left. That is., even after passing the point x= 0, it will continue to travel towards the left. This is shown in fig.c.

3. But once the point x = 0 is passed, the block will begin to experience a resistive force. The block is able to overcome the resistive force, and reach up to x = −A. Once it reaches x=−A, it stops. That is., it's velocity becomes zero. This is shown in fig.d.

4. Then it starts the reverse journey. In the reverse journey, even after passing the point x=0, it will continue to travel towards the right. This is shown in fig.e.

5. But once the point x = 0 is passed, the block will begin to experience a resistive force. The block is able to overcome the resistive force, and reach up to x = A. Once it reaches x=A, it stops. That is., it's velocity becomes zero. This is shown in fig.f.

6. At this point, one cycle is complete. Then it again starts the journey towards left. This process continues giving rise to continuous oscillation.


Displacement

The above 6 steps give us a basic understanding about oscillation. Now we will derive an expression for displacement. It can be done in 9 steps:
1. We saw that, the red block is oscillating between x=A and x=−A. Let us mark those two points as P and Q respectively, on the x-axis. This is shown in fig.14.4 below:

Fig.14.4

• The coordinates of P and Q are (A,0) and (−A,0) respectively. So O is the equilibrium position of the block.

2. Draw the red circle with center at O and radius equal to A.
• The magenta sphere is performing uniform circular motion along the red circle.
• The angular velocity of the magenta sphere is $\small{\omega}$.
• That means, the angle subtended by the sphere, at O, in each second, is $\small{\omega}$.

3. Consider the instant when the magenta sphere is at M. At that instant, the line OM makes an angle $\small{\theta}$ with the x-axis.
• Drop the perpendicular MN from M, onto the x-axis.
• From the right triangle OMN, we get:
$\small{ON~=~ OM\,\cos \theta~=~A\,\cos\theta}$.

4. Now, ON is the horizontal displacement of the magenta sphere from the equilibrium position O. So we get a method to write the horizontal displacement of the magenta sphere from O.

◼ Let us check for other points. For that, we will try to write a general method which is applicable to all points.

(i) In fig.14.5(a) below, M is in the I quadrant.
    ♦ On OM, Mark M' such that, OM' = 1 unit.
    ♦ Drop the perpendicular M'N' onto the x-axis.

Fig.14.5

• OMN and OM'N' are similar triangles. So we can write:
$\small{\frac{OM}{OM'}~=~\frac{ON}{ON'}}$
$\small{\Rightarrow~ON~=~OM\left(\frac{ON'}{OM'} \right)}$   
$\small{\Rightarrow~ON~=~A \left(\frac{ON'}{OM'} \right)}$
• Length of ON' is same as the x-coordinate of M'.
• Since OM' = 1 unit, the point M' is on the unit circle, and so, the x-coordinate of M' is $\small{\cos \theta}$ (Details here)
• So we get:
$\small{ON~=~A \left(\frac{\cos \theta}{1} \right)~=~A\,\cos \theta}$

(ii) In fig.14.5(b) above, M is in the II quadrant.
    ♦ On OM, Mark M' such that, OM' = 1 unit.
    ♦ Drop the perpendicular M'N' onto the x-axis.
• OMN and OM'N' are similar triangles. So we can write:
$\small{\frac{OM}{OM'}~=~\frac{ON}{ON'}}$
$\small{\Rightarrow~ON~=~OM\left(\frac{ON'}{OM'} \right)}$   
$\small{\Rightarrow~ON~=~A \left(\frac{ON'}{OM'} \right)}$
• Length of ON' is same as the x-coordinate of M'.
• Since OM' = 1 unit, the point M' is on the unit circle, and so, the x-coordinate of M' is $\small{\cos \theta}$
• So we get:
$\small{ON~=~A \left(\frac{\cos \theta}{1} \right)~=~A\,\cos \theta}$
• Since M is in the II quadrant, $\small{\cos \theta}$ will be −ve. Indeed, N will have a −ve x-coordinate because it is on the −ve side of the x-axis.

(iii) In fig.14.5(c) above, M is in the III quadrant.
We can write similar steps and obtain the same result.

(iv) In fig.14.5(d) above, M is in the IV quadrant.
We can write similar steps and obtain the same result.

• So whichever be the quadrant, the horizontal displacement of the magenta sphere will be $\small{A\,\cos \theta}$ 

5. We see that, this method is very effective to write the horizontal displacement of the magenta sphere. But we want the horizontal displacement of the red block.
• So we assume that:
   ♦ At the instant when the block is released from P, the sphere starts the revolution from P
   ♦ At the instant when the block reaches O, the sphere reaches R
   ♦ At the instant when the block reaches Q, the sphere also reaches Q
   ♦ At the instant when the block returns through O, the sphere reaches S
   ♦ At the instant when the block returns back at P, the sphere also reaches back at P

6. That means, the time period (T) for one oscillation of the block is same as the time for one revolution of the sphere. Using this information, we can write an expression for $\small{\theta}$
• Time for one revolution of the sphere = T seconds
⇒ Time for $\small{2 \pi}$ radians = T seconds
⇒ Time for 1 radian = $\small{\frac{T}{2 \pi}}$ seconds
⇒ Angular distance covered in 1 second  = $\small{\frac{2 \pi}{T}}$ radian
• The stop-watch is turned on at the instant when the block is released from P. At that same instant, the sphere starts the revolution from the same point P.
• Consider the instant at which the reading in the stop-watch is t. Let at that instant, the sphere be at M.
• So when the reading is t, the angular distance covered is $\small{\theta}$
• Angular distance covered in 1 second  = $\small{\frac{2 \pi}{T}}$ radian
⇒ Angular distance covered in t seconds  = $\small{\frac{2 \pi t}{T}}$ radian
⇒ $\small{\theta}$  = $\small{\frac{2 \pi t}{T}}$ radian
• So we can write:
At any time t,
The horizontal displacement of the sphere from O
= The horizontal displacement of the block from O
= $\small{A\,\cos\theta~=~A\,\cos\left(\frac{2 \pi t}{T} \right)}$
• That means:
$\small{x(t)~=~A\,\cos\left(\frac{2 \pi t}{T} \right)}$

7. We derived the equation: $\small{x(t)~=~A\,\cos\theta~=~A\,\cos\left(\frac{2 \pi t}{T} \right)}$.
• If we want, we can use $\small{\omega}$ instead of $\small{T}$.
• We have:
the angle subtended by the sphere, at O, in each second, is $\small{\omega}$.
• So in $\small{t}$ seconds, the sphere will subtend $\small{\omega\,t}$ radians at O
• But the angle subtended by the sphere, at O, in $\small{t}$ seconds, is $\small{\theta}$.
• That means: $\small{\theta~=~\omega\,t}$
• Thus we get:
$\small{x(t)~=~A\,\cos\theta~=~A\,\cos\left(\frac{2 \pi t}{T} \right)~=~A\,\cos\left(\omega\,t \right)}$.

8. Here, the only variable on the R.H.S is $\small{t}$.
   ♦ $\small{t}$ is the independent variable
   ♦ $\small{x}$ is the dependent variable
• So while drawing the graph, we must plot $\small{t}$ along the x-axis and $\small{x}$ along the y-axis.

9. One such graph is shown in fig.14.6 below.
   ♦ A is assumed to be 2.5 units
   ♦ T is assumed to be 6 s

Fig.14.6

• We get:
$\small{x(t)~=~A\,\cos\left(\frac{2 \pi t}{T} \right)~=~(2.5)\,\cos\left(\frac{2 \pi t}{6} \right)~=~(2.5)\,\cos\left(\frac{\pi t}{3} \right)}$

• Let us write some of the information that can be obtained from the graph:
(i) To find the instants at which the red block reaches the positive extreme, we need to solve the equation:
$\small{x(t)~=~2.5~=~(2.5)\,\cos\left(\frac{\pi t}{3} \right)}$
$\small{\Rightarrow 1~=~\cos\left(\frac{\pi t}{3} \right)}$

• This is a trigonometrical equation. We have seen the method to solve such equations, in our math classes (Details here).
• We get: t = 0, 6, 12, . . .
• The points are marked on the graph. Indeed we see that, the y-coordinates at these points are all 2.5

(ii) To find the instants at which the red block reaches the negative extreme, we need to solve the equation:
$\small{x(t)~=~-2.5~=~(2.5)\,\cos\left(\frac{\pi t}{3} \right)}$
$\small{\Rightarrow -1~=~\cos\left(\frac{\pi t}{3} \right)}$

• This is a trigonometrical equation. Solving it, we get:
t = 3, 9, 6, . . .
• The points are marked on the graph. Indeed we see that, the y-coordinates at these points are all −2.5

(iii) To find the instants at which the red block reaches the equilibrium position, we need to solve the equation:
$\small{x(t)~=~0~=~(2.5)\,\cos\left(\frac{\pi t}{3} \right)}$
$\small{\Rightarrow 0~=~\cos\left(\frac{\pi t}{3} \right)}$

• This is a trigonometrical equation. Solving it, we get:
t = 1.5, 4.5, 7.5, 10.5, . . .
• The points are marked on the graph. Indeed we see that, the y-coordinates at these points are all zero.


Phase constant

This can be explained in 3 steps:
1. Consider fig.14.4 again. We turned the stop-watch on, when the red sphere was at P. Then we noted the time 't' at which the red sphere is at the arbitrary point M. The angle MOP at time 't' is denoted as '$\small{\theta}$'

2. The same fig.14.4 is modified and shown again in fig.14.7 below:

Fig.14.7

• Here, the stop-watch is turned on, when the sphere is at B. At B, the line OB already makes an angle $\small{\phi}$ with the x-axis.
• So at time 't', the sphere is at the arbitrary point M and the line OM makes an angle of $\small{\theta + \phi}$ with the x-axis
• Therefore in this case, the horizontal displacement of the sphere from O, at time 't' is given by:
$\small{x(t)~=~A \,\cos\left(\theta + \phi \right)}$

3. Let us draw the graph. It is shown in fig.14.8 below. For easy comparison, the previous graph in red color, is also shown as such. The new graph is shown in green color. For the new graph:
   ♦ A is the same 2.5 units
   ♦ T is the same 6 s
   ♦ $\small{\phi}$ is assumed to be $\small{\frac{\pi}{6}}$

Fig.14.8

• We get:
$\small{x(t)~=~A\,\cos\left(\frac{2 \pi t}{T}+\phi \right)~=~(2.5)\,\cos\left(\frac{2 \pi t}{6}+\frac{\pi}{6} \right)~=~(2.5)\,\cos\left(\frac{\pi t}{3}+\frac{\pi}{6} \right)}$

• Let us write some of the information that can be obtained from the graph:
(i) To find the instants at which the red block reaches the positive extreme, we need to solve the equation:
$\small{x(t)~=~2.5~=~(2.5)\,\cos\left(\frac{\pi t}{3}+\frac{\pi}{6} \right)}$
$\small{\Rightarrow 1~=~\cos\left(\frac{\pi t}{3}+\frac{\pi}{6} \right)}$

• This is a trigonometrical equation. Solving it, we get:
t = 5.5, 11.5, . . .
• The points are marked on the graph. Indeed we see that, the y-coordinates at these points are all 2.5

(ii) To find the instants at which the red block reaches the negative extreme, we need to solve the equation:
$\small{x(t)~=~-2.5~=~(2.5)\,\cos\left(\frac{\pi t}{3}+\frac{\pi}{6} \right)}$
$\small{\Rightarrow -1~=~\cos\left(\frac{\pi t}{3}+\frac{\pi}{6} \right)}$

• This is a trigonometrical equation. Solving it, we get:
t = 2.5, 8.5, . . .
• The points are marked on the graph. Indeed we see that, the y-coordinates at these points are all −2.5

(iii) To find the instants at which the red block reaches the equilibrium point, we need to solve the equation:
$\small{x(t)~=~0~=~(2.5)\,\cos\left(\frac{\pi t}{3}+\frac{\pi}{6} \right)}$
$\small{\Rightarrow 0~=~\cos\left(\frac{\pi t}{3}+\frac{\pi}{6} \right)}$

• This is a trigonometrical equation. Solving it, we get:
t = 1, 4, 7, 10, . . .
• The points are marked on the graph. Indeed we see that, the y-coordinates at these points are all zero.

(iv) The green curve is an exact replica of the red curve. But the green is shifted by a small amount  towards the left.
• That means:
The green reaches the extreme points and zero points earlier than the red.
• For example:
   ♦ Red reaches a maximum at t = 6 s. Green reaches a maximum at t = 5.5 s
   ♦ Red reaches a minimum at t = 3 s. Green reaches a minimum at t = 2.5 s
   ♦ Red reaches a zero at t = 7.5 s. Green reaches a maximum at t = 7 s
• We say that:
The two oscillations are out of phase by an angle of $\small{\frac{\pi}{6}}$ radians
• The angle $\small{\phi~=~\frac{\pi}{6}}$
• $\small{\phi}$ is called the phase constant.


In the next section, we will see the oscillation of the same spring in the vertical direction.

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Saturday, January 24, 2026

Chapter 14 - Oscillations

In the previous section, we saw specific heats of gases. In this chapter, we will see oscillations.

• In some earlier chapters, we have seen rectilinear motion, projectile motion and uniform circular motion.
• In uniform circular motion, a particle takes the same time to complete each revolution. So it is a periodic motion.
• In this chapter, we will see another type of periodic motion, called oscillation.
• In oscillation, a particle moves to and fro about a mean position.
   ♦ Motion of the pendulum is an example
   ♦ Motion of the piston inside the cylinder of an engine is another example.   
• To learn about periodic motion and oscillatory motion, we must first see some fundamental concepts like period, frequency, displacement etc., They are explained below:

Periodic and Oscillatory motions

Some basics can be written in 5 steps:
1. Consider an insect climbing up a wall. It starts climbing from the ground level. It travels with a uniform speed u1. In a time duration of t1, it reaches a height h. This is shown by the red line in fig.14.1(a) below:

Fig.14.1

• After t1, the insect is not able to climb upwards. Neither is it able to hold on. So it climbs down to the ground with a uniform speed of u2.  The time taken for reaching the ground is t2. This is shown by the green line in fig.14.1(a) above.
• Note that, t1 is larger than t2. This is because, time taken to reach the ground is smaller.
• The sum (t1 + t2) is T. This T is the time required to start from  the ground and reach back to the ground. If the insect keep repeating the "climbing and falling" process, we will get several repetitions in the graph. The ground is then considered as the mean position.
• The red line is familiar to us. We have plotted many distance-time (s-t) graphs in rectilinear motion. If the motion is uniform, we get the same red line. It is the plot of the equation s = ut. In our present case, u1 is the slope of the red line. u1 is constant.
• The green line can also be given a similar explanation. It has a negative slope because, velocity is negative for downward motion. So slope of the green line is −u2.
• In fig.14.1, instead of s, we plot x(t) along the y-axis. This is because, in periodic motion, the displacement from the mean position is denoted by x. It is a function of time. So we write x(t).

2. Consider the game of bouncing the ball between palm and ground.
• The game starts when the ball is thrown to the ground from a height h. It is thrown with an initial speed of u1. Since the ball is under the influence of gravity, speed is not uniform.
• The displacement at any instant 't' is given by:
$\small{x(t)\,=\,u_1 t + \frac{1}{2} a t^2}$. This is the equation of a parabola.
• In a time duration of t1, it reaches the ground. This is shown by the red parabola in fig.14.1(b) above.
• After t1, the ball bounces upwards with a speed of u2. Since the ball is under the influence of gravity, speed is not uniform. The displacement at any instant 't' is given by:
$\small{x(t)\,=\,u_2 t - \frac{1}{2} a t^2}$. This is the equation of a parabola.
• In a time duration of t2, it reaches the palm. This is shown by the  green parabola in fig.14.1(b) above.
• The sum (t1 + t2) is T. This T is the time required to start from  the palm and reach back to the palm. As the game continues, we will get several repetitions in the graph. The ground is then considered as the mean position.
• Note that, the red and green parabolas are graphs. They are not the paths followed by the ball. The path of the ball is always vertical. While playing this game, the ball cannot be thrown in a parabolic path. If the ball is thrown in a parabolic path, it will not bounce back to the palm. It will bounce away from the player.

3. A motion that repeats itself at regular intervals of time is called a periodic motion.

4. Consider the red sphere in fig.14.2 below. It is at the bottom of the yellow bowl.

Fig.14.2

• In this position, the sphere is at equilibrium. If the sphere is left alone, it will remain there forever.
• But if the sphere is given a displacement, a force will come into play, which tries to bring the sphere back to the equilibrium position. As a result, the sphere will perform oscillation or vibration in the bowl.
• Oscillating bodies eventually come to rest. In our present case, the sphere will come to rest at the bottom of the bowl.
• This is due to the friction between the sphere and the bowl. The surrounding air also causes the sphere to come to rest. This type of oscillation is called damped oscillation.
• However, an oscillation can be forced to remain oscillating, by providing an external agency. This type of oscillation is called forced oscillation. We will see the details of both types in later sections of this chapter.

5. Every oscillatory motion is a periodic motion.
• But every periodic motion need not be an oscillatory motion.
   ♦ Circular motion is periodic but not oscillatory.

Period and frequency

This can be explained in 7 steps:
1. Consider the earlier fig.14.1(a). We turn on the stop-watch at the instant when the insect begins to climb up. When the reading in the stop-watch is T, the insect is back on the ground, and the next cycle begins.

2. In fig.14.1(b), we turn on the stop-watch at the instant when the ball is thrown. When the reading in the stop-watch is T, the ball is back at the palm, and the next cycle begins.

3. So we can write:
The smallest duration of time after which the next cycle begins, is called the period of the periodic motion. It is denoted by the symbol T.
• The S.I unit of period is second.

4. For periodic motions which are too fast, period will be very small. In such cases, instead of s, we can use other units.
• For example, the period of vibration of a quartz crystal is expressed in microseconds.
   ♦ One microsecond is $\small{10^{-6}}$ seconds.
   ♦ Microsecond is abbreviated as: $\small{{\rm{\mu s}}}$

5. For periodic motions which are too slow, period will be very large. In such cases also, instead of s, we can use other units.
• For example, the orbital period of some  planets are expressed in earth days.
   ♦ For mercury, it is 88 earth days.
   ♦ One earth day is 24 hours.

6. Suppose that, period of a periodic motion is 30 s. Then in one minute, two cycles will occur.
   ♦ That is., in 60 s, two cycles will occur
   ♦ That is., in 1 s, 2/60 cycles will occur.
   ♦ That is., in 1 s, 1/30 cycles will occur.
   ♦ That is., in 1 s, 1/30 of one cycle will occur.
• The number of cycles in one second is called frequency. It is represented by the symbol $\small{\nu}$. In our present case, $\small{\nu}$ = 1/30.
• Note that, 1/30 is the reciprocal of 30. And 30 is the period in seconds.
• So we can write:
Frequency is the reciprocal of period. The period must be in seconds.
   ♦ That is., $\small{\nu~=~\frac{1}{T}}$
   ♦ where T is n seconds.
• Since we are taking the reciprocal of "period in seconds", the unit of frequency is $\small{{\rm{s^{-1}}}}$.
This $\small{{\rm{s^{-1}}}}$ is given a special name. It is called hertz (abbreviated as Hz), in honor of the scientist Heinrich Rudolph Hertz, who discovered radio waves.
• We can write:
1 hertz = 1 Hz = 1 cycle per second = 1 $\small{{\rm{s^{-1}}}}$.

7. Note that, $\small{\nu}$ need not be an integer. It can be a decimal or a fraction.

Let us see a solved example:

Solved example 14.1
On an average, a human heart is found to beat 75 times in a minute. Calculate it's frequency and period.
Solution
:
1. First, let us calculate the frequency:
Number of occurrences in one minute = 75
⇒ Number of occurrences in 60 s = 75
⇒ Number of occurrences in 1 s = 75/60
⇒ Frequency $\small{\nu~=~\frac{75}{60}~=~\frac{5}{4}~=~1.25~{\rm{s^{-1}}}}$
2. Now we can calculate the period:
We know that, frequency is the reciprocal of period. It follows that, period is the reciprocal of frequency. So we can write:
Period $\small{T~=~\frac{1}{\nu}~=~\frac{4}{5}~=~0.8 {\rm{s}}}$


In the next section, we will see displacement.

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