Gas pressure in gravitational field from the partition function

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The discussion focuses on deriving expressions for gas pressure in a gravitational field using the partition function. The initial approach using free energy and its relation to pressure resulted in a complex expression, prompting a reconsideration of the method. A more promising strategy involves using the probability distribution to find the number of particles at a specific height, which can then be integrated to determine pressure. The second part of the problem, calculating pressure at the top given the bottom pressure, appears more straightforward by integrating over momenta and coordinates. Ultimately, the goal is to express the partition function as an integral over phase space to simplify the calculations for pressure.
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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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