Statistical Mechanics, Simplifying dq/dT

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SUMMARY

The discussion focuses on the derivation of the equation \(\frac{dq}{dT}=\sum_{i} g_i \frac{dq}{dT} e^{-\frac{ε_i}{kT}}\) in statistical mechanics, specifically addressing the calculation of average molecular energy \(\bar{ε}\). Participants clarify that \(\bar{ε}\) represents the mean energy, calculated using the probability distribution \(\mathcal{P}(\varepsilon_i) = \frac{1}{q} g_i e^{-\varepsilon_i / kT}\). The confusion regarding the absence of division by the number of states \(N\) in the calculation of \(\sum_{i} g_i ε_i\) is resolved by recognizing it as a weighted average rather than a total energy. This understanding is crucial for correctly applying statistical mechanics principles.

PREREQUISITES
  • Understanding of statistical mechanics concepts, particularly partition functions.
  • Familiarity with Boltzmann distribution and its applications.
  • Knowledge of average energy calculations in thermodynamics.
  • Basic proficiency in calculus, especially in handling summations and limits.
NEXT STEPS
  • Study the derivation of the partition function \(q\) in statistical mechanics.
  • Explore the concept of probability distributions in thermodynamic systems.
  • Learn about the relationship between temperature and average molecular energy in ideal gases.
  • Investigate the implications of degeneracy in energy states on statistical calculations.
USEFUL FOR

Students and researchers in physics, particularly those specializing in statistical mechanics and thermodynamics, as well as educators looking to clarify concepts related to energy distributions and partition functions.

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Homework Statement



[tex]\frac{dq}{dT}=\sum_{i} g_i \frac{dq}{dT} e^{-\frac{ε_i}{kT}} = \frac{1}{kT^2}\sum_{i} g_i ε_i e^{-\frac{ε_i}{kT}} = \frac{1}{kT^2} \bar{ε} q[/tex]

Homework Equations



[tex]q=\sum_{i} e^{-\frac{ε_i}{kT}}[/tex] or for degenerate states, [tex]q=\sum_{I} g_i e^{-\frac{ε_I}{kT}}[/tex]

The Attempt at a Solution



The equations in (1) are just set out in my notes. My problem is understanding the last step: I take [itex]\bar{ε}[/itex] to be the average molecular energy, since later they show that [itex]\bar{ε}_{trans}=\frac{3}{2}kT[/itex].

How can [itex]\sum_{i} g_i ε_i[/itex] be the mean, without dividing by N? Isn't it the total molecular energy?
 
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The probability for a particle to have energy ##\varepsilon_i## is
$$
\mathcal{P}(\varepsilon_i) = \frac{1}{q} g_i e^{-\varepsilon_i / kT}
$$
Therefore, the average energy can be calculated as
$$
\begin{align}
\bar{\varepsilon} &= \sum_i \varepsilon_i \mathcal{P}(\varepsilon_i) \\
&= \sum_i \varepsilon_i \frac{1}{q} g_i e^{-\varepsilon_i / kT}
\end{align}
$$
Compare to your equation.
 

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