Gas pressure in gravitational field from the partition function

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SUMMARY

The discussion focuses on deriving expressions for gas pressure in a gravitational field using the partition function, specifically referencing the problem from the UNM prelims document. The user initially attempts to use the free energy equation, F=-kT ln Z, but finds it cumbersome for exam conditions. They shift to using the probability distribution p=exp[-β(p²/2m + mgz)]/Z, which allows for calculating the number of particles at a specific height z. The user concludes that integrating this probability across momentum coordinates simplifies the process of determining pressure at varying heights.

PREREQUISITES
  • Understanding of statistical mechanics and partition functions
  • Familiarity with thermodynamic derivatives and their applications
  • Knowledge of gravitational effects on gas behavior
  • Proficiency in calculus, particularly integration in multiple dimensions
NEXT STEPS
  • Study the derivation of the canonical partition function Z in statistical mechanics
  • Learn about the application of thermodynamic derivatives in calculating pressure
  • Explore the integration of probability distributions in phase space
  • Investigate the effects of gravitational fields on gas pressure and density profiles
USEFUL FOR

Graduate students in physics, particularly those studying statistical mechanics, as well as researchers interested in the thermodynamic properties of gases in gravitational fields.

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Homework Statement



Please see P2 in http://panda.unm.edu/pandaweb/graduate/prelims/SM_S09.pdf

"Starting with \mathbb{Z} (z_1,z_2) above, derive expressions for the gas pressure..."

Homework Equations





The Attempt at a Solution



To find the pressure at the top and the bottom of the gas column, I tried to use F=-kT\ln \mathbb{Z}, where F is the free energy, and P=-\left(\frac{\partial F}{\partial V}\right)_T by writing h=\frac{V}{A} and got a horrible expression. So I don't think that is the way to go for a timed exam. Moreover, I'm not sure how I can get the pressure at a specific height from that.

Now, I'm thinking about starting from the probability p=\frac{exp[-\beta (\frac{p^2}{2m}+mgz)]}{\mathbb{Z}}, which directly gives the number of particles at height z. But how can I get the pressure from that?

The second part where I have to calculate the pressure at the top given the pressure at the bottom looks easier though, since I have the pressure at the bottom as a reference point.
 
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I think I got it. Integrate p=exp[-\beta (\frac{p^2}{2m}+mgz)] along all three momenta, x and y coordinates, and all particle but one. Then I get the probability of a particle to be at height z. From there, I can get the number of particles at height z, and then the force and the pressure.
 
It seems like it's easier to just write Z as an integral over 6N dimensional phase space, do the integrals over p and q. All that's left is a function of z1 and z2, then try using the thermodynamic derivatives to give you the pressure.
 

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