as far as I understand, the canonical partition function of a single particle can be expressed as follows: $$ z = \sum_i e^{-\beta\cdot\epsilon_i} $$ Where $i$ are the micro states, $\beta$ is the inverse of the product of the Boltzman constant and the temperature, and $\epsilon_i$ is the energy at that state. Which can be expanded for a system of N particles as: $ Z=z^N$. Where Z can be expressed $$ Z=\sum_i e^{-\beta\cdot E_i} = \sum_j w(E_j)\cdot e^{-\beta\cdot E_j}$$ Where j represents the energy level, and $w$ is the degeneracy of that energy level. So at this point I have my first question:
- Are $\epsilon$ from the single particle partition function and $E$, from the system's partition function different?
Then the probability of occupancy of a micro state is given by: $$ P_i(E_i)= \frac{e^{-\beta\cdot E_i}}{Z} $$ And the probability of an energy level being occupied is: $$ P(E_j)= \frac{w(E_j)\cdot e^{-\beta\cdot E_j}}{Z} $$
And finally, the average energy can be equated to the internal energy. Which can be calculated as follows: $$ U=\bar{E}=\sum_i P_i(E_i)\cdot E_i $$
And here the second question:
- What would be the equivalent of the internal energy in terms of a summation over the energy levels ($j$) instead of the micro states ($i$)?
Thanks for any help in advance.