In which one of the following limits does the Fermi-Dirac distribution \(n_F(\epsilon, T) = \left(e^{\frac{\epsilon - \mu}{k_B T}} + 1\right)^{-1}\) and the Bose-Einstein distribution \(n_B(\epsilon, T) = \left(e^{\frac{\epsilon - \mu}{k_B T}} - 1\right)^{-1}\) reduce to the Maxwell-Boltzmann distribution?
Step 1: Recall Maxwell-Boltzmann distribution form.
The Maxwell-Boltzmann (MB) distribution is given by:
\[
n_{MB}(\epsilon, T) = e^{-\frac{\epsilon - \mu}{k_B T}}
\]
Step 2: Approximation condition.
For both Fermi-Dirac and Bose-Einstein, if \(e^{\frac{\epsilon - \mu}{k_B T}} \gg 1\), then
\[
n_F \approx e^{-\frac{\epsilon - \mu}{k_B T}}, n_B \approx e^{-\frac{\epsilon - \mu}{k_B T}}
\]
which corresponds to the Maxwell-Boltzmann limit.
Step 3: Conclusion.
Therefore, the MB distribution is valid when \((\epsilon - \mu) \gg k_B T.\)
For a particular ideal gas, which of the following graphs represents the variation of mean squared velocity of the gas molecules with temperature?

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.)