At Brewsterβs angle \( \theta_B \), the reflected and refracted rays are perpendicular to each other. The Brewster angle can be calculated using the formula:
\[ \tan(\theta_B) = \frac{n_2}{n_1} \]
Substituting the given values:
\[ \tan(\theta_B) = 1.5 \quad \Rightarrow \quad \theta_B = \tan^{-1}(1.3333) \approx 53.1^\circ \]
Since the reflected and refracted rays are at \( 90^\circ \) to each other, the angle \( \alpha \) is:
\[ \alpha = 90^\circ \]
Thus, the correct answer is 90 degrees.
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/mΒ³, which is dimensionally incorrect for a spectral density. The correct unit J/(mΒ³Β·Hz) or JΒ·s/mΒ³ is used here for the solution.)