Step 1: Retardation condition.
For conversion between opposite circular polarizations, phase difference = \(\pi\) radians.
\[
\Delta \phi = \frac{2\pi (n_e - n_o) t}{\lambda} = \pi
\]
Step 2: Solve for thickness \(t\).
\[
t = \frac{\lambda}{2(n_e - n_o)} = \frac{600 \times 10^{-9}}{2(1.551 - 1.542)} = \frac{600 \times 10^{-9}}{0.018} = 33.33 \times 10^{-6} \, \text{m}
\]
\[
t = 33.33 \, \mu\text{m}
\]
Step 3: Conclusion.
Hence, the thickness of the retarder = 33.33 µm.
A beam of unpolarized light of intensity \(I_0\) falls on a system of four identical linear polarizers placed in a line as shown in the figure. The transmission axes of any two successive polarizers make an angle of \(30^\circ\) with each other. If the transmitted light has intensity \(I\), the ratio \(\dfrac{I}{I_0}\) is: 

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.)