Question
Question: Two coaxial discs having moments of inertia \({I_1}\) and \(\dfrac{{{I_1}}}{2}\) are rotating with r...
Two coaxial discs having moments of inertia I1 and 2I1 are rotating with respective angular velocities ω1 and 2ω1 , about their common axis. They are brought in contact with each other and thereafter they rotate with a common angular velocity. If Ef and Ei are the final and initial total energies, then (Ef−Ei) is:
\left( a \right)$$$\dfrac{{{I_1}\omega _1^2}}{{12}}$$
\left( b \right)\dfrac{3}{8}{I_1}\omega _1^2\left( c \right)\dfrac{{{I_1}\omega _1^2}}{6}\left( d \right)\dfrac{{ - {I_1}\omega _1^2}}{{24}}$
Solution
Hint So in this question, it is given that there are the two-discs and they are having a moment of inertia and having some angular velocities. Now they are saying that it will be brought in contact with one another and then it gets rotated. By using the equation given on conservation of angular momentum. And so by doing this we get the answer.
Formula:
Conservation of angular momentum,
Li=Lf
And Kinetic energy,
⇒21Iω2
Where,
I , will be the inertia and ω will be the angular velocity.
Complete Step By Step Solution As from the question it is clear that we have to find the difference between the two energies which is final and the initial.
As we know energy in terms of inertia for both the disc will be equal to
⇒E=21I1×ω12+212I2×4Ω12
Now putting the values from the question,
⇒2I1ω12(89)=169I1ω12=EI
Now on further solving the above equation,
We get
⇒I1ω1=4I1ω1=23I1ω
And from here
⇒ω=65ω1
Now we will calculate the final energy, so for this final energy will be equal to
⇒Ef=21×23I1×3625ω12
After solving the above equation, we will get the equation as
⇒4825I1ω12
Now we will calculate the difference between that will be represented as (Ef−Ei) ,
So equating the value we obtained from the above calculation, we get
⇒Ef−Ei=I1ω12(4825−169)
Again on further solving the above equation, we get
⇒48−2I1ω12
And after simplifying, we get
⇒24−I1ω12
Therefore, 24−I1ω12 , is the difference between the final and initial energies. Hence the option D is the correct one among all the four options given here.
Note The Law of Conservation of Angular Momentum is extremely important: it explains how explosions work, why our planet still spins, why we orbit the sun, and why, when two things crash into each other, they sometimes bounce.