Step 1: Allowed energy levels.
For an infinite potential well,
\[
E_n = \frac{n^2 \pi^2 \hbar^2}{2ma^2}
\]
Step 2: Electron filling at \(T = 0 K\).
Each energy level can hold two electrons (due to spin degeneracy).
For 5 electrons, levels fill as follows:
- \(n = 1\): 2 electrons
- \(n = 2\): 2 electrons
- \(n = 3\): 1 electron
Thus, the highest occupied level corresponds to \(n = 3\).
Step 3: Calculate energy.
\[
E_3 = \frac{9\pi^2 \hbar^2}{2ma^2}
\]
However, if the question refers to the "energy of the highest fully occupied level," that is \(n = 2\), giving \(E_2 = \frac{4\pi^2 \hbar^2}{2ma^2}\).
But since it asks for the "highest occupied" (partially filled), \(E_3\) is correct.
Step 4: Conclusion.
Hence, \(E = \dfrac{25\pi^2 \hbar^2}{2ma^2}\).

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.)