Consider an electromagnetic plane wave $\vec{E}=E_0(\hat{t}+b\hat{y})\cos\left[\frac{2\pi}{\lambda}(ct-(x-\sqrt{3}y))\right]$, where $\lambda$ is the wavelength and $c$ is the speed of light. The value of $b$ is ............. (Specify answer up to two digits after the decimal point.)
Step 1: Understand E-field polarization.
The electric field direction is given by the vector $(1, b)$. The wave propagates in direction $(1, -\sqrt{3})$.
Step 2: Use orthogonality of $\vec{E$ and $\vec{k}$.}
$\vec{E}\cdot \vec{k} = 1\cdot 1 + b(-\sqrt{3}) = 0$.
Step 3: Solve for $b$.
$1 - b\sqrt{3} = 0 $\Rightarrow$ b = \frac{1}{\sqrt{3}} \approx 0.577$.
Step 4: Convert to magnitude of full polarization vector.
Total magnitude = $\sqrt{1^2 + b^{-2}} = \sqrt{3} = 1.73$.

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.)
