Partition Function of N particles in an assymetrical box

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SUMMARY

The discussion focuses on calculating the partition function and average energy of N identical molecules in an asymmetrical box using statistical mechanics principles. Participants derive the energy for a single particle as $$\varepsilon = {\frac {h^2} {8m}} \left[ \left( \frac {n_x} {L_x} \right)^2 + \left( \frac {n_y} {L_y} \right)^2 + \left( \frac {n_z} {L_z} \right)^2 \right]$$ and utilize the indistinguishability of particles to express the partition function as $$Z\left(T,V,N\right) = \frac 1 {N!} Z\left(T,V,1\right)^N$$. The partition function for one molecule is derived as $$Z\left(T,V,1\right)= \left(\frac {2m\pi} {h^2\beta} \right)^{3/2} L_x L_y L_z$$, leading to the calculation of average energy using $$\bar \varepsilon = -\frac {\partial ln(Z)} {\partial \beta}$$.

PREREQUISITES
  • Understanding of statistical mechanics concepts, particularly partition functions.
  • Familiarity with quantum mechanics, specifically quantum states and energy levels.
  • Knowledge of thermodynamic variables such as temperature (T), volume (V), and beta (β).
  • Ability to perform mathematical operations involving sums and integrals in the context of physics.
NEXT STEPS
  • Study the derivation of the partition function in more complex systems, such as interacting particles.
  • Learn about the implications of indistinguishability in statistical mechanics.
  • Explore the relationship between partition functions and thermodynamic potentials.
  • Investigate the application of the canonical ensemble in statistical mechanics.
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Students and professionals in physics, particularly those studying statistical mechanics, thermodynamics, and quantum mechanics. This discussion is especially beneficial for those working on problems involving partition functions and average energy calculations.

FranciscoSili
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Homework Statement


Consider a gas sufficiently diluted containing N identical molecules of mass m in a box of dimensions Lx, Ly, Lz.

  • Calculate the probability of finding the molecules in any of their quantum states.
  • Calculate the energy of each quantum state εr, as a function of the quantum numbers ##n_x##, ##n_y## and ##n_z##.
  • Calculate the average energy using the expression
    $$\bar \varepsilon = \sum_{r} P_r \varepsilon_r$$
    Demonstrate that the last expression is equivalent to $$\bar \varepsilon = -\frac {\partial ln(Z)} {\partial \beta}$$
    where ## Z= \sum_{r} exp\{-\beta\varepsilon_r\} ##, it's called the partition function.
  • Found the partition function and calculate the average energy.

    Help: the sum over ##r## can be replaced by an integral. Why?

    2. The attempt at a solution
    I have tried solving this problem this way, but I am not sure this is the correct solution and/or way.

    First, I calculated the energy for a single particle in this box as $$\varepsilon = {\frac {h^2} {8m}} \left[ \left( \frac {n_x} {L_x} \right)^2 + \left( \frac {n_y} {L_y} \right)^2 + \left( \frac {n_z} {L_z} \right)^2 \right]$$
    Because these particles are indistinguishable I can use the property of the partition function that reads $$Z\left(T,V,N\right) = \frac 1 {N!} Z\left(T,V,1\right)^N$$ that will let me calculate only the partition function of a single particle and then obtain it to N of them.
    Now I calculate the partition function for one molecule as indicated in the problem statement, $$Z\left(T,V,1\right)=\sum_{n_x,n_y,n_z} exp\left\{\ {\frac {-h^2\beta} {8m}} \left[ \left( \frac {n_x} {L_x} \right)^2 + \left( \frac {n_y} {L_y} \right)^2 + \left( \frac {n_z} {L_z} \right)^2 \right]\right\}$$ which can be split into three different sums, multiplying one another: $$Z\left(T,V,1\right)=\sum_{n_x=1}^\infty exp\left\{\ {\frac {-\beta h^2} {8m}}\left( \frac {n_x} {L_x} \right)^2\right\} \sum_{n_y=1}^\infty exp\left\{\ {\frac {-\beta h^2} {8m}}\left( \frac {n_y} {L_y} \right)^2\right\} \sum_{n_z=1}^\infty exp\left\{\ {\frac {-\beta h^2} {8m}}\left( \frac {n_z} {L_z} \right)^2\right\}.$$ If I can change the sums for integrals which, approximately, run from 0 to infinity, the partition function becomes
    \begin{equation}
    Z\left(T,V,1\right)=\int_0^\infty exp\left\{\ {\frac {-\beta h^2} {8m}}\left( \frac {n_x} {L_x} \right)^2\right\} \, dn_x \int_0^\infty exp\left\{\ {\frac {-\beta h^2} {8m}}\left( \frac {n_y} {L_y} \right)^2\right\} \, dn_y \int_0^\infty exp\left\{\ {\frac {-\beta h^2} {8m}}\left( \frac {n_z} {L_z} \right)^2\right\} \, dn_z,
    \end{equation}
    and solving them we get
    \begin{equation}
    Z\left(T,V,1\right)= \left(\frac {2m\pi} {h^2\beta} \right)^{3/2} L_x L_y L_z.
    \end{equation}
    Then I can calculate the partition function for the hole system of N particles, then the probability ##P_r## and finally the average energy,##\bar \varepsilon##, as in the statement

    Any help or comments that you might have is welcomed, since this is my second week of my Statistical Mechanics course. Thank you very much :D
 
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I think your work looks good.

The order of the questions indicates to me that you are to answer the first 3 dotted questions before working out the partition function. I'm guessing that in the first question, you are to write out a general expression for ##P_r## in terms of the symbols ##\epsilon_r## and ##\beta## but you are not meant to evaluate it explicitly. Likewise in the third question, express the average energy in terms of ##\epsilon_r## and ##\beta## using your expression for ##P_r## from the first question. The partition function ##Z## is defined here and you should show the identity involving the derivative of ##Z## with respect to ##\beta##. Finally, in the fourth (last) question, evaluate ##Z## as you have done and then evaluate explicitly the average energy. Hope I'm not misleading you here.
 
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TSny said:
I think your work looks good.
Ohh ok, that's good to hear. Thank you.

TSny said:
The order of the questions indicates to me that you are to answer the first 3 dotted questions before working out the partition function. I'm guessing that in the first question, you are to write out a general expression for ##P_r## in terms of the symbols ##\epsilon_r## and ##\beta## but you are not meant to evaluate it explicitly. Likewise in the third question, express the average energy in terms of ##\epsilon_r## and ##\beta## using your expression for ##P_r## from the first question. The partition function ##Z## is defined here and you should show the identity involving the derivative of ##Z## with respect to ##\beta##. Finally, in the fourth (last) question, evaluate ##Z## as you have done and then evaluate explicitly the average energy. Hope I'm not misleading you here.

Yes I know that I did everything in reverse, but the most complicated calculations were the ones for the partition function, so that's what I wanted to ask, if it was correct. I should have said that in the beginning, sorry for that.

Thank you.
 
FranciscoSili said:
Yes I know that I did everything in reverse, but the most complicated calculations were the ones for the partition function, so that's what I wanted to ask, if it was correct. I should have said that in the beginning, sorry for that.

Thank you.
That's fine. Good work.
 
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