Partition sum of particle, high/low temperature limits

In summary, the partition sum of a particle is a mathematical concept used in statistical mechanics to describe the distribution of energy states of a system at a given temperature. At high temperatures, the partition sum increases exponentially due to the Boltzmann factor, resulting in a higher average energy for the system. At low temperatures, the partition sum decreases due to the Boltzmann factor, resulting in a lower average energy. The high temperature limit in the partition sum allows for predictions about the system's behavior and simplifies to the classical expression for the average energy, known as the equipartition theorem. However, for quantum particles, the partition sum can deviate from the classical result at high temperatures due to their quantum nature.
  • #1
SoggyBottoms
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Homework Statement


We have a single particle that can be in one of three different microstates, [itex]\epsilon_0[/itex], [itex]\epsilon_1[/itex] or [itex]\epsilon_2[/itex], with [itex]\epsilon_0 < \epsilon_1 < \epsilon_2[/itex]. The particle is in thermal equilibrium with a heat bath at temperature T.

1) Calculate the canonical partition function.

2) Give the probabilities [itex]P_j[/itex] that this particle is in state [itex]j[/itex] for [itex]j = 0, 1, 2[/itex].

3) What is the average energy in the high and low temperature limit?

The Attempt at a Solution



1) [tex]Z(\beta) = e^{- \beta \epsilon_0} + e^{- \beta \epsilon_1} + e^{- \beta \epsilon_2} [/tex]

2)

[tex]P(0) = \frac{e^{- \beta \epsilon_0}}{Z(\beta)}[/tex]

[tex]P(1) = \frac{e^{- \beta \epsilon_1}}{Z(\beta)}[/tex]

[tex]P(2) = \frac{e^{- \beta \epsilon_2}}{Z(\beta)}[/tex]

3)

[tex]
\langle E \rangle = \epsilon_0 \cdot P(0) + \epsilon_1 \cdot P(1) + \epsilon_2 \cdot P(2) \\
= \frac{\epsilon_0 e^{- \beta \epsilon_0} + \epsilon_1 e^{- \beta \epsilon_1} + \epsilon_2 e^{- \beta \epsilon_2}}{e^{- \beta \epsilon_0} + e^{- \beta \epsilon_1} + e^{- \beta \epsilon_2}}
[/tex]

So then I just plug in [itex]\beta = \frac{1}{k_B T}[/itex] and see what happens when T gets very low or very high, and then for high temperatures I get [itex]U = \frac{\epsilon_0 + \epsilon_1 + \epsilon_2}{3}[/itex] and for low temperatures it goes to 0. Is this correct?

Edit: I meant partition function in the title.
 
Last edited:
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  • #2


Thank you for your question. Your calculations for the canonical partition function and probabilities are correct. However, your calculation for the average energy in the high and low temperature limits is incorrect.

In the high temperature limit, the average energy would approach the average of all possible energies, which is given by:

\langle E \rangle = \frac{\epsilon_0 + \epsilon_1 + \epsilon_2}{3}

This is because at high temperatures, the particle has equal probabilities of being in any of the three states.

In the low temperature limit, the average energy would approach the lowest energy state, which is \epsilon_0. This is because at low temperatures, the particle would mostly be in the lowest energy state due to the Boltzmann factor, e^{- \beta \epsilon_0}, being the largest.

I hope this helps clarify your understanding. If you have any further questions, please don't hesitate to ask. Keep up the good work!


 

Related to Partition sum of particle, high/low temperature limits

1. What is the partition sum of a particle?

The partition sum of a particle is a mathematical concept used in statistical mechanics to describe the distribution of energy states of a system at a given temperature. It is a sum of all possible energy states of the particles in the system, weighted by the Boltzmann factor.

2. How is the partition sum affected by high temperatures?

At high temperatures, the partition sum increases exponentially due to the Boltzmann factor, which takes into account the increased probability of particles being in higher energy states. This results in a higher average energy for the system.

3. How does the partition sum change at low temperatures?

At low temperatures, the partition sum decreases due to the Boltzmann factor, as there is a lower probability of particles being in higher energy states. This results in a lower average energy for the system.

4. What is the significance of the high temperature limit in the partition sum?

The high temperature limit in the partition sum is an important concept in statistical mechanics, as it allows us to make predictions about the behavior of a system at high temperatures. In this limit, the partition sum simplifies to the classical expression for the average energy of a system, known as the equipartition theorem.

5. How does the partition sum at high temperatures differ for classical and quantum particles?

For classical particles, the partition sum at high temperatures is given by the equipartition theorem, which assumes that energy is evenly distributed among all degrees of freedom. However, for quantum particles, the partition sum takes into account the quantum nature of the particles and can deviate from the classical result at high temperatures.

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