Semi-Classical/Classical derivation of ideal gas partition function

In summary, the factors of ##\frac{5}{2}## and ##\frac{3}{2}## in the entropy of the semi-classical and classical ideal gases respectively are coincidental and have no relation to the degrees of freedom of the gases.
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CAF123
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In the semi-classical treatment of the ideal gas, we write the partition function for the system as $$Z = \frac{Z(1)^N}{N!}$$ where ##Z(1)## is the single particle partition function and ##N## is the number of particles. It is semi-classical in the sense that we consider the indistinguishability of the particles, so we divide by ##N!##.

The resulting expression for the entropy of the system is $$S = Nk \left(\ln \left[\left(\frac{V}{N}\right) \left(\frac{2\pi mkT}{h^2}\right)^{3/2} \right] + \frac{5}{2}\right)$$

Now consider a fully classical analysis. There ##Z(1) = \sum_{E} \exp (-\frac{E}{kT})##, where ##E = p^2/2m## (assuming no interaction potentials). The problem can be mapped to an integral over the phase space of the Hamiltonian to give $$Z(1) \rightarrow \int \exp \left(-\frac{1}{2mkT} (p_x^2 + p_y^2 + p_z^2) \right)\text{d}^3 \underline{p} \,\text{d}^3 \underline{x}$$ This can then be rewritten like $$ \int \exp \left(-\frac{p_x^2}{2mkT}\right) \text{d}p_x \int \exp \left(-\frac{p_y^2}{2mkT}\right) \text{d}p_y \int \exp \left(-\frac{p_z^2}{2mkT} \right) \text{d}p_z \cdot V$$ where ##V## is the volume of the container. Those are Gaussian integrals and so evaluation is immediate. The result is that ##Z(1) = (2\pi mkT)^{3/2} V##. The corresponding entropy can be calculated and the result is that $$S = Nk \left(\frac{3}{2} + \ln\left(\frac{(2\pi mkT)^{3/2}}{V}\right)\right).$$

What is the significance of the factors 5/2 in the semi-classical treatment and the factor 3/2 in the classical treatment and why are they different? They look like the number of degrees of freedom a monatomic and diatomic molecule would have at room temperature, but I think this is a coincidence.

Many thanks.
 
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  • #2
It's just a coincidence. The factor of ##N!## in ##Z## ends up giving a factor of ##-k_B T N## in the free energy ##F = -k_B T \ln Z## which then gives a factor of ##k_B N ## in ##S = -\frac{\partial F}{\partial T} ## which gets added on to the factor of ##\frac{3}{2} k_B N## coming from ##\frac{\partial }{\partial T} \ln Z_1## present also in the classical gas, this giving an overall factor of ##\frac{5}{2}##. It has nothing to do with the degrees of freedom of the classical and semi-classical monoatomic gases as both have a factor of ##\frac{3}{2}## in ##\bar{E} = -\frac{\partial }{\partial \beta} \ln Z## in accordance with equipartition.
 
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What is the ideal gas partition function?

The ideal gas partition function is a mathematical function that describes the distribution of particles in an ideal gas system. It is used to calculate the thermodynamic properties of an ideal gas, such as its energy and entropy.

What is the difference between Semi-Classical and Classical derivation of the ideal gas partition function?

The Semi-Classical derivation takes into account the quantum nature of particles, while the Classical derivation assumes that particles behave as classical particles. This leads to slight differences in the equations used to calculate the partition function.

What is the formula for the Semi-Classical derivation of the ideal gas partition function?

The formula for the Semi-Classical derivation is Z = (1/N!) * (2πmkT/h^2)^(3N/2) * V^N, where N is the number of particles, m is the mass of each particle, k is the Boltzmann constant, T is the temperature, h is the Planck constant, and V is the volume of the system.

What is the formula for the Classical derivation of the ideal gas partition function?

The formula for the Classical derivation is Z = (1/N!) * (2πmkT)^(3/2) * V^N, where N is the number of particles, m is the mass of each particle, k is the Boltzmann constant, T is the temperature, and V is the volume of the system. This formula does not include the Planck constant, as classical particles are assumed to not have quantized energy levels.

How is the ideal gas partition function used in thermodynamics?

The ideal gas partition function is used to calculate various thermodynamic quantities, such as the internal energy, entropy, and free energy of an ideal gas system. It is also used in statistical mechanics to calculate the probability of a system being in a certain energy state.

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