Pressure and the Young-Laplace Equation

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SUMMARY

The discussion centers on the application of the Young-Laplace equation in determining pressure profiles in a fluid contained within a rotating cylinder under the influence of gravity. The participants derived a parabolic meniscus profile and explored the conditions under which surface tension can be neglected, specifically referencing the Bond number and the newly introduced McCraney number. The conversation emphasizes the importance of understanding the balance of forces acting on the free surface and the implications of curvature on pressure distribution. The final derived equation for meniscus height is given as z = z0 + (ω²/2g)r².

PREREQUISITES
  • Understanding of fluid dynamics principles, particularly the Navier-Stokes equations.
  • Familiarity with the Young-Laplace equation and its application in fluid mechanics.
  • Knowledge of dimensionless numbers, specifically the Bond number and Capillary number.
  • Basic calculus for deriving equations and performing integrations.
NEXT STEPS
  • Study the derivation and implications of the Young-Laplace equation in fluid mechanics.
  • Learn about dimensionless analysis and its application in fluid systems, focusing on the Bond and McCraney numbers.
  • Investigate the Navier-Stokes equations and their application in free surface flows.
  • Explore numerical methods for simulating fluid dynamics in rotating systems.
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Fluid dynamics engineers, researchers in mechanical engineering, and students studying advanced fluid mechanics who are interested in the effects of surface tension and pressure distribution in rotating fluid systems.

  • #31
joshmccraney said:
$$-\sigma\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)+s_0^2\rho g Z(S)+\sigma\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)_{S=0}=s_0^3\frac{\rho \omega^2R^2(S)}{2}$$
Is this what you had in mind?
Yes. Now divide the equation by ##\rho \omega^2 s^3_0##. What do you get?
 
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  • #32
Chestermiller said:
Yes. Now divide the equation by ##\rho \omega^2 s^3_0##. What do you get?
$$\frac{\sigma}{\rho \omega^2 s^3_0}\left[\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)_{S=0}-\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)\right]+\frac{g }{\omega^2 s_0}Z(S)=\frac{R^2(S)}{2}$$ Starting to look like the "McCraney number".
 
  • #33
joshmccraney said:
$$\frac{\sigma}{\rho \omega^2 s^3_0}\left[\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)_{S=0}-\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)\right]+\frac{g }{\omega^2 s_0}Z(S)=\frac{R^2(S)}{2}$$ Starting to look like the "McCraney number".
Good. Now, there are a couple of ways to proceed further with the dimensional analysis. One way is to now set ##s_0=g/\omega^2##, so that the coefficient of Z is unity. What does this give you?
 
  • #34
Chestermiller said:
Good. Now, there are a couple of ways to proceed further with the dimensional analysis. One way is to now set ##s_0=g/\omega^2##, so that the coefficient of Z is unity. What does this give you?
Awesome, this is perfect. Thanks so much!
$$M\left[\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)_{S=0}-\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)\right]+Z(S)=\frac{R^2(S)}{2}$$
 
  • #35
joshmccraney said:
Awesome, this is perfect. Thanks so much!
$$M\left[\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)_{S=0}-\left(\frac{\sin\phi}{R}+\frac{d\phi}{dS}\right)\right]+Z(S)=\frac{R^2(S)}{2}$$
The important thing is to assimilate this kind of methodology for reducing the equations for a system to dimensionless form.
 
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  • #36
Chestermiller said:
Good. Now, there are a couple of ways to proceed further with the dimensional analysis. One way is to now set ##s_0=g/\omega^2##, so that the coefficient of Z is unity. What does this give you?

Chestermiller said:
The important thing is to assimilate this kind of methodology for reducing the equations for a system to dimensionless form.
I couldn't agree more. How did you know to scale ##Z## with ##R^2##, which is to say what to set as ##O(1)##?
 
  • #37
joshmccraney said:
I couldn't agree more. How did you know to scale ##Z## with ##R^2##, which is to say what to set as ##O(1)##?
I wanted the terms for the case of zero surface tension to be preserved in the limit of zero surface tension.
 
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