The reflectance \( R \) at an air-dielectric interface for normal incidence is given by:
\[ R = \left(\frac{n_2 - n_1}{n_2 + n_1}\right)^2 \]
Substituting \( n_1 = 1.0 \) and \( n_2 = 2.0 \):
\[ R = \left(\frac{2.0 - 1.0}{2.0 + 1.0}\right)^2 \]
\[ R = \left(\frac{1.0}{3.0}\right)^2 \]
\[ R = \frac{1.0}{9.0} \]
\[ R \approx 0.111 \]
The intensity of the reflected light is given by:
\[ I_{\text{reflected}} = R \cdot I_0 \]
Using \( R \approx 0.111 \):
\[ I_{\text{reflected}} \approx 0.111 I_0 \]
Thus, the intensity of the reflected light is approximately \( 0.111 I_0 \).
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.)