Deriving equations for pressure & number density for centrif

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SUMMARY

The discussion focuses on deriving equations for pressure (P) and particle number density (nv) in a gas centrifuge, which separates gases based on molar mass by rotating a cylinder. The derived equation for number density is nv = n0 * e^(-m * r^2 * w^2 / (2 * k * T)), where m is molar mass, r is radial distance, w is angular frequency, T is temperature, and k is the Boltzmann constant. The pressure equation is not explicitly provided but is related to the centripetal acceleration given by w^2 r and Newton's second law.

PREREQUISITES
  • Understanding of Newton's second law and centripetal acceleration
  • Familiarity with gas laws and thermodynamic principles
  • Knowledge of the Boltzmann constant and its application in statistical mechanics
  • Basic calculus for deriving equations from physical principles
NEXT STEPS
  • Study the derivation of the ideal gas law and its implications in centrifuges
  • Learn about the application of Newton's laws in rotational dynamics
  • Explore the concept of the Boltzmann factor and its significance in statistical mechanics
  • Investigate the relationship between pressure, volume, and temperature in rotating systems
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Students in physics or engineering, particularly those studying thermodynamics and fluid dynamics, as well as professionals working with gas separation technologies in industrial applications.

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Homework Statement


Consider particles in a gas centrifuge. This device is used to separate gases of different molar mass by rotating a cylinder at high rates. Derive two equations: one for the pressure (P) and one for the particle number density (nv) as functions of M, r, w and T, where r is the radial distance from the center point and w is the angular frequency of the rotation. M and T are molar mass and temperature. Do this by applying Newton's 2^nd law to the circular motion of a segment of gas of mass delta(m) and width delta(r). Recall that centripetal acceleration is given by w^2 r and that the positive direction for r is radially outward from the center of the circle.

Homework Equations


nv = n0 * e\^(m * r^2 * w^2 / (2 * k * T))
Net Fr = (m * v^2)/r

The Attempt at a Solution


I have no clue what I'm supposed to do. I don't even know how I'm going to draw a FBD for this. I don't know what the pressure equation is supposed to look like, but I know the number density equation is supposed to look like this: nv = n0 * e\^(m * r^2 * w^2 / (2 * k * T)), where k is the Boltzmann constant. I only know this because I was able to look online for this answer (though it did not explain how they derived this).
 
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Er, I mean nv = n0 * e^(m * r^2 * w^2 / (2 * k * T)). This part may also be wrong, since I think it should be nv = n0 * e^(-m * r^2 * w^2 / (2 * k * T)) since it reminds me of the Boltzmann factor.
 

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