At what temperature do quantum effects become significant for a gas

Click For Summary
SUMMARY

This discussion focuses on estimating the temperature at which quantum effects become significant for a gas of interacting particles, specifically using the Lennard-Jones potential parameters (equilibrium distance R and well-depth E). The critical temperature can be approximated using the formula T_c ≈ \frac{\hbar^2}{2m} n^{2/3}, where n is the particle number density. The conversation highlights that for rare gas atoms, such as Helium and Argon, the quantum temperature is influenced by the strength of their interactions, although interactions do not significantly alter the critical temperature. The de Boer parameter values calculated for Argon (0.027) and Neon (0.079) illustrate differences in interaction energies among rare gases.

PREREQUISITES
  • Understanding of quantum mechanics principles, particularly thermal de Broglie wavelength.
  • Familiarity with statistical physics and thermodynamic properties of gases.
  • Knowledge of the Lennard-Jones potential and its parameters (R & E).
  • Basic concepts of bosons and fermions in quantum statistics.
NEXT STEPS
  • Research the derivation of the critical temperature formula in statistical physics textbooks.
  • Explore the implications of the Pauli exclusion principle on fermionic gases.
  • Investigate the role of the de Boer parameter in characterizing rare gas interactions.
  • Learn about the differences in quantum behavior between weakly and strongly interacting gases.
USEFUL FOR

Physicists, chemists, and students interested in quantum mechanics, statistical physics, and the thermodynamic behavior of gases, particularly in the context of rare gas interactions.

Signifier
Messages
75
Reaction score
0
Hi, I was wondering how to calculate a rough estimate of the temperature at which quantum effects begin to become important for a gas of interacting particles. Let's say the particles interact via a spherically symmetric potential with an equilibrium distance R and a well-depth E (such as the Lennard-Jones potential). Can I use the mass of the particles and the interaction energy parameters (R & E) to estimate a temperature around which quantum effects become important?

By quantum effects becoming important, I mean they begin to significantly affect thermodynamic properties of the gas, such as the magnitude of the second virial coefficient B(T).

I can calculate things like the thermal de Broglie wavelength, the de Boer parameter, etc., but I was wondering if there was some straightforward way to estimate this. Presumably for rare gas atoms with weaker interactions (Helium) the "quantum temperature" should be larger than that for rare gas atoms with strong interactions (eg, argon).

Thank you - I hope I am clear!
 
Physics news on Phys.org
The derivation is not exactly trivial, and it depends on whether your gas consists of bosons or fermions (you get the same general formula but with different constants in front). Interparticle interactions do not really matter too much. You can find it in most statistical physics textbooks. The critical temperature is on the order of

\frac{\hbar^2}{2m} n^{2/3},

where n is particle number density. For a typical gas at atmospheric pressure, it's on the order of a few kelvin.
 
Hm... a very interesting result. I have been calculating interaction parameters for the rare gas atoms. Following Pahl, Calvo, Kocˇi, and Schwerdtfeger (Angew. Chem. Int. Ed. 2008, 47, 8207 –8210), I've calculated the de Boer parameter for the different RG atoms, getting for instance 0.027 for Ar and 0.079 for Neon.

I am far from an expert but surely there must be some relationship between well depth, width and position and the temperature at which quantum effects begin to become important? Your result tells me there is no difference between the temp for Ar and the temp for He? But there are definite differences between the interaction energies of these atoms...
 
These quantum effects are present even if the interaction is zero. The dominant effect for fermions, for example, is Pauli exclusion principle. Interactions affect some thermodynamic properties, but I don't think that they significantly change the critical temperature.

Maybe this thread should be moved into the atomic physics subforum. It's a condensed-matter problem. Personally, I'm not an expert on condensed matter.
 
Last edited:

Similar threads

  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 18 ·
Replies
18
Views
2K
  • · Replies 46 ·
2
Replies
46
Views
5K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 4 ·
Replies
4
Views
1K
  • · Replies 15 ·
Replies
15
Views
4K
  • · Replies 9 ·
Replies
9
Views
2K
  • · Replies 21 ·
Replies
21
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 14 ·
Replies
14
Views
2K