At the boundary between two dielectric media, the following conditions hold:
The electric field in medium 1 is: \[ \vec{E_1} = 3\hat{x} + 2\hat{y} + 4\hat{z}. \] - Tangential components (\( \vec{E_{1t}} \)): These are the components parallel to the interface (\( z = 0 \)): \[ \vec{E_{1t}} = 3\hat{x} + 2\hat{y}. \] - Normal component (\( \vec{E_{1n}} \)): This is the component perpendicular to the interface (\( z \)-direction): \[ \vec{E_{1n}} = 4\hat{z}. \]
Using the continuity conditions:
The displacement vector \( \vec{D} \) is related to \( \vec{E} \) by: \[ \vec{D} = \epsilon_0 \epsilon_r \vec{E}. \] For medium 2 (\( \epsilon_r = 3 \)): \[ \vec{D_2} = \epsilon_0 \cdot 3 \cdot (3\hat{x} + 2\hat{y} + \frac{16}{3}\hat{z}). \] Distribute \( \epsilon_0 \cdot 3 \): \[ \vec{D_2} = \epsilon_0 (9\hat{x} + 6\hat{y} + 16\hat{z}). \]
The displacement vector in medium 2 is: \[ \vec{D_2} = (9\hat{x} + 6\hat{y} + 16\hat{z})\epsilon_0. \]
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/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.)