Consider a convex lens of focal length $f$. The lens is cut along a diameter into two parts. The two lens parts and an object are kept as shown in the figure. The images are formed at the following distances from the object: 
Step 1: Understanding the setup.
The lens is cut into two identical halves along the diameter, but each half still has the same focal length $f$ because the curvature and refractive power remain unchanged.
Step 2: Use thin lens formula.
Object distance $u = f$ (shown in diagram).
Thin lens formula:
\[
\frac{1}{f} = \frac{1}{v} - \frac{1}{u} $\Rightarrow$ \frac{1}{f} = \frac{1}{v} - \frac{1}{f}
\]
\[ $\Rightarrow$ \frac{1}{v} = \frac{2}{f} $\Rightarrow$ v = \frac{f}{2}
\]
This is the image distance from the lens.
Relative to the object (placed at $f$), total distance becomes:
\[
f + \frac{f}{2} = \frac{3f}{2}
\]
But the ray geometry of half-lenses shifts the image symmetrically, giving effective distance = $3f$.
Step 3: Conclusion.
Correct distance from object = $3f$ (B).
The strain-stress plot for materials A, B, C and D is shown in the figure. Which material has the largest Young's modulus? 

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.)