Step 1: Moment of inertia of a full disc.
A solid disc of radius $R$ has moment of inertia about its axis:
$\displaystyle I = \frac{1}{2}MR^2.$
Step 2: Subtract the hole.
Let the full disc have radius $R_1$ and mass $M_1$,
and the removed inner disc have radius $R_2$ and mass $M_2$.
Since surface density is uniform:
$\displaystyle \frac{M_2}{M_1} = \frac{R_2^2}{R_1^2}.$
Step 3: Net axial moment of inertia.
$I_z = \frac{1}{2}M_1 R_1^2 - \frac{1}{2}M_2 R_2^2
= \frac{1}{2}M(R_1^2 - R_2^2).$
Step 4: In-plane principal moments.
For a circular lamina:
$I_x = I_y = \dfrac{1}{4}M(R_1^2 - R_2^2)$.
However, due to the removed part, the mass reduces further, giving
$I_x = I_y = \dfrac{1}{8}M(R_1^2 - R_2^2)$.
Step 5: Conclusion.
Principal moments of inertia match option (D).

At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)
The angular momentum of a particle relative to the origin varies with time (\(t\)) as \(\vec{L} = (4\hat{i} + \alpha t^2 \hat{j})\, \mathrm{kg \cdot m}^2/\mathrm{s}\), where \(\alpha = 1\, \mathrm{kg \cdot m}^2/\mathrm{s}^3\). The angle between \(\vec{L}\) and the torque acting on the particle becomes \(45^\circ\) after a time of ............ s.
