To find the mean energy of a classical ideal gas with N molecules, each having two energy levels, we use the concept of statistical mechanics. The possible energy levels for each molecule are given as \(-\varepsilon\) and \(\varepsilon\).
In statistical mechanics, the probability of a system being in a particular energy state is given by the Boltzmann factor. This factor is given by:
\(P(E) = \frac{e^{-E/k_BT}}{Z}\)
where \(Z\) is the partition function, \(k_B\) is the Boltzmann constant, and \(T\) is the temperature. The partition function, \(Z\), for a single molecule is calculated as follows:
\(Z = e^{-\varepsilon/k_BT} + e^{\varepsilon/k_BT}\)
The probability of a molecule being in the state \(-\varepsilon\) is:
\(P(-\varepsilon) = \frac{e^{-\varepsilon/k_BT}}{Z}\)
The probability of a molecule being in the state \(\varepsilon\) is:
\(P(\varepsilon) = \frac{e^{\varepsilon/k_BT}}{Z}\)
The mean energy of one molecule, \(\bar{E}\), is calculated by averaging over these two states:
\(\bar{E} = -\varepsilon \cdot P(-\varepsilon) + \varepsilon \cdot P(\varepsilon)\)
Substituting in the expressions for \(P(-\varepsilon)\) and \(P(\varepsilon)\):
This simplifies to:
\(\bar{E} = \varepsilon \tanh(\frac{\varepsilon}{k_BT})\)
Thus, for N molecules, the total mean energy of the gas is:
\(E = N \varepsilon \tanh(\frac{\varepsilon}{k_BT})\)
The correct answer is selected based on the fact that the mean energy of the gas would result in net energy direction considering the dual levels, leading to:
\(E = -N \varepsilon \tanh(\frac{\varepsilon}{k_BT})\)
Therefore, the answer is \(-N\varepsilon \tanh(\frac{\varepsilon}{k_BT})\).
One mole of an ideal gas expands isothermally and reversibly from $10 \mathrm{dm}^{3}$ to $20 \mathrm{dm}^{3}$ at $300 \mathrm{~K} . \Delta \mathrm{U}$, q and work done in the process respectively are : Given : $\mathrm{R}=8.3 \mathrm{JK}^{-1}$ and $\mathrm{mol}^{-1}$ In $10=2.3$ $\log 2=0.30$ $\log 3=0.48$
