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: 
Step 1: Initial intensity after first polarizer.
Unpolarized light passing through the first polarizer transmits half the intensity:
\[
I_1 = \frac{I_0}{2}
\]
Step 2: Use Malus's law for each subsequent polarizer.
For each polarizer making \(30^\circ\) angle with the previous one:
\[
I_2 = I_1 \cos^2 30^\circ = \frac{I_0}{2} \times \frac{3}{4} = \frac{3I_0}{8}
\]
\[
I_3 = I_2 \cos^2 30^\circ = \frac{3I_0}{8} \times \frac{3}{4} = \frac{9I_0}{32}
\]
\[
I_4 = I_3 \cos^2 30^\circ = \frac{9I_0}{32} \times \frac{3}{4} = \frac{27I_0}{128}
\]
Step 3: Conclusion.
\[
\frac{I}{I_0} = \frac{27}{128}
\]

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.)