A monatomic gas in a 2d Universe - multiplicity

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SUMMARY

The discussion centers on the multiplicity of a monatomic ideal gas in a two-dimensional universe, specifically deriving the expression for multiplicity as Ω = (1/N!) * (A^N/h^(2N)) * (π^N/N!) * (2MU)^N. A participant queries the presence of a factor of 2 in their calculations, which is later clarified by referencing Schroeder's book, indicating that the factor can be disregarded due to its negligible impact on the overall multiplicity. The entropy expression for the gas is also sought, emphasizing the relationship between entropy, energy (U), area (A), and particle number (N).

PREREQUISITES
  • Understanding of statistical mechanics principles, particularly multiplicity and entropy.
  • Familiarity with the Heisenberg Uncertainty Principle.
  • Knowledge of ideal gas behavior in two-dimensional systems.
  • Basic proficiency in mathematical derivations involving factorials and limits.
NEXT STEPS
  • Study the derivation of entropy for ideal gases in two dimensions.
  • Explore the implications of the Heisenberg Uncertainty Principle in statistical mechanics.
  • Investigate the differences between three-dimensional and two-dimensional gas behavior.
  • Review Schroeder's book on statistical mechanics for deeper insights into multiplicity calculations.
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Students and researchers in physics, particularly those focusing on statistical mechanics, thermodynamics, and the behavior of gases in non-traditional dimensions.

TFM
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Homework Statement



Consider a monatomic ideal gas that lives in a two-dimensional universe (“flatland”), occupying an area A instead of a volume V.

(a)

By following the logic of the derivation for the three-dimensional case, show that the multiplicity of this gas can be written:

\Omega = \frac{1}{N!}\frac{A^N}{h^{2N}}\frac{\pi^N}{N!}(2MU)^N

(b)

Find an expression for the entropy of this two-dimensional gas. Express your result in terms of U, A and N.

Homework Equations



N/A

The Attempt at a Solution



I have practically finished part a, with one small exception. for the pi fraction, I have 2pi instead of pi?

Some of my working out:

The space multiplicity:

\Omega_{space} = (\frac{A}{(\Delta x)^2})^N

The multiplicity of momentum:

\Omega_{mom} = (\frac{A_{hypercircle}}{(\Delta p_x)})^{2N}

\Omega_{mom} = (\frac{A_{hypercircle} ^{2N}}{(\Delta p_x^{2N})})

The total multiplicity is the multiple:

\Omega = \Omega_{space}\Omega_{mom}

\Omega = ((\frac{A}{(\Delta x)^2})^N )(\frac{A_{hypercircle} ^{2N}}{(\Delta p_x^{2N})} )

This can be rearranged, and using Heisenberg's Uncertainty princeple, \Delta x \Delta p_x \approx h

this gives:
\Omega = \frac{A^N A_{hypercircle}}{h^{2N}}

For indistinguishable particles:

\Omega = \frac{1}{N!}\frac{A^N}{h^{2N}}A_{hypercircle}

Area of hypercircle:

\frac{2\pi^N}{(N - 1)!}{\sqrt{2mu}^{2N-1}}

and using approximations:

\Omega = \frac{1}{N!}\frac{A^N}{h^{2N}}\frac{2\pi^N}{N!}{2mu^N}

As you can see, close, just that annoying 2...

Any ideas how to get rid of it?

Thanks in advanced,

TFM
 
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I have attached the entre workings out. any idewa how to get rid iof that pesky 2...?

TFM
 

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Sorry for 2 year late reply. You're probably graduated by now. But according to Schroeder's book, for part (a),

you can simply throw away the 2 because the multiplicity is very large compared to the 2, and thus it won't really make a difference. He then apologizes below for sloppy working. But... oh well that's what I just read.
 

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