Boltzmann distribution of two different gases

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SUMMARY

The discussion centers on the Boltzmann distribution of two different ideal gases with varying molar masses in a uniform gravitational field. It is established that the density distribution of these gases at equilibrium is proportional to the Boltzmann probability, expressed as exp(-m*g*h/T), where m represents the molecular mass, g is the gravitational acceleration, h is the height, and T is the temperature in energy units. The conversation references the Feynman Lectures and highlights that the higher molecular weight gas exhibits a steeper density gradient with height. The implications of gas interactions and pressure effects are also considered.

PREREQUISITES
  • Understanding of the Boltzmann distribution
  • Familiarity with ideal gas laws
  • Knowledge of gravitational effects on gases
  • Basic principles of thermodynamics
NEXT STEPS
  • Study the Boltzmann distribution in detail, focusing on its applications in statistical mechanics
  • Explore the concept of isothermal atmospheres and their implications in gas behavior
  • Investigate the effects of molecular weight on gas density distributions
  • Review the Feynman Lectures on physics for deeper insights into gas interactions and equilibrium states
USEFUL FOR

Students and professionals in physics, particularly those studying thermodynamics and statistical mechanics, as well as researchers interested in gas behavior in gravitational fields.

oguz
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hi everyone,

consider two different masses of ideal gases with different molar masses, we're putting them in a uniform gravitational field and wait until they come to their equilibrium states. how would the density distribution change with height in this case?

( i came out with this question while working on a problem in "problems on general physics" by irodov. the answer to the problem seemed to be merely superposing two different distributions but doesn't this imply that molecules of both gases do not interact? if they don't, I'm asking should not they be stressing pressure on each other?)
 
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oguz said:
hi everyone,

consider two different masses of ideal gases with different molar masses, we're putting them in a uniform gravitational field and wait until they come to their equilibrium states. how would the density distribution change with height in this case?

( i came out with this question while working on a problem in "problems on general physics" by irodov. the answer to the problem seemed to be merely superposing two different distributions but doesn't this imply that molecules of both gases do not interact? if they don't, I'm asking should not they be stressing pressure on each other?)

ISTR this problem is discussed in the Feynman lectures, where it is stated that the density in equilibrium is proportional to the Boltzmann probability, i.e. exp(-m*g*h/T), where m is the molecular mass (T is in energy units; use kB for unit conversion). (This is assuming an isothermal atmosphere, which is not in mechanical equilibrium.) There will be a normalization factor that depends on the total amount of has. The higher molecular weight gas has a higher rate of density change with height.

BBB
 

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