To solve this problem, we need to understand the concept of rotational motion and how angular momentum is conserved. We are given two discs with the same moment of inertia rotating with angular velocities \(\omega_1\) and \(\omega_2\). When these discs are brought into contact face-to-face, their axes of rotation coincide, leading to a change in energy due to the conservation of angular momentum.
Let's denote the moment of inertia of each disc as \(I\). The initial angular momentum (\(L_i\)) of the system is the sum of the angular momenta of the two discs:
L_i = I \omega_1 + I \omega_2 = I (\omega_1 + \omega_2)
When the discs are brought together, they will rotate with a common angular velocity (\(\omega'\)) due to conservation of angular momentum, which is:
L_f = 2I \omega'
Equating initial and final angular momentum:
I (\omega_1 + \omega_2) = 2I \omega'
Solving for \(\omega'\):
\omega' = \frac{(\omega_1 + \omega_2)}{2}
Next, let's analyze the initial and final kinetic energies to find the loss in energy. The initial kinetic energy (\(KE_i\)) is:
KE_i = \frac{1}{2}I \omega_1^2 + \frac{1}{2}I \omega_2^2
The final kinetic energy (\(KE_f\)) with common angular velocity is:
KE_f = \frac{1}{2}(2I)(\frac{(\omega_1 + \omega_2)}{2})^2 = I \frac{(\omega_1 + \omega_2)^2}{4}
Therefore, the loss of energy (\(\Delta KE\)) is:
\Delta KE = KE_i - KE_f = \left[ \frac{1}{2}I \omega_1^2 + \frac{1}{2}I \omega_2^2 \right] - I \frac{(\omega_1 + \omega_2)^2}{4}
Simplifying this expression:
\Delta KE = \frac{1}{2}I (\omega_1^2 + \omega_2^2) - \frac{1}{4}I (\omega_1^2 + 2\omega_1\omega_2 + \omega_2^2)
\Delta KE = \frac{1}{2}I \omega_1^2 + \frac{1}{2}I \omega_2^2 - \frac{1}{4}I \omega_1^2 - \frac{1}{2}I \omega_1\omega_2 - \frac{1}{4}I \omega_2^2
\Delta KE = \frac{1}{4}I (\omega_1^2 + \omega_2^2 - 2\omega_1\omega_2)
\Delta KE = \frac{1}{4}I (\omega_1 - \omega_2)^2
Therefore, the loss of energy during the process when the discs are brought in contact is given by the expression: \(\frac{1}{4}I (\omega_1 - \omega_2)^2\).
For a uniform rectangular sheet shown in the figure, the ratio of moments of inertia about the axes perpendicular to the sheet and passing through \( O \) (the center of mass) and \( O' \) (corner point) is:
