Graduate Model the pressure of a zero-gravity simple fluid system

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SUMMARY

This discussion centers on modeling the pressure of a zero-gravity simple fluid system contained within a circular cylinder. The equilibrium free surface of the inviscid liquid is described as a spherical cap, with pressure governed by the Young-Laplace equation, leading to the relationship P ∼ σ/R². When the base of the cylinder is open, the pressure in the liquid domain incorporates reservoir pressure from inflow, complicating the model. The contact angle significantly influences the shape of the interface, determining whether it is concave or convex based on the hydrophilic or hydrophobic nature of the liquid.

PREREQUISITES
  • Understanding of potential flow theory
  • Familiarity with the Young-Laplace equation
  • Knowledge of contact angle effects in fluid dynamics
  • Basic principles of inviscid fluid mechanics
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  • Research contact angle effects on fluid behavior in various materials
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Fluid dynamicists, mechanical engineers, and researchers in materials science focusing on fluid behavior in zero-gravity environments.

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Hi PF!

A circular cylinder contains an inviscid liquid, which is softly disturbed (i.e. velocities are small). There are no body forces, which implies the equilibrium free surface is that of a spherical cap with radius ##R## (see figure A). Inviscid implies we can assume potential flow, such that the liquid velocity ##V## can be expressed in terms of it's potential such that ##V = \nabla \psi##. The pressure throughout the liquid domain is ##P = -\nabla \psi## (recall velocities are small, so the non-linear term drops). The pressure at the free surface is governed by the Young-Laplace equation, which implies ##P \sim \sigma/R^2## there (actually this pressure term turns out to be VERY mathematically complicated, which is why I simply use the proportional notation). So the pressure balance at the free surface can be expressed by equating the two pressures at the interface.

Now let's assume the base of the cylinder is open such that flow can enter, shown in B). What is the pressure now in the liquid domain? I believe it is no longer ##P = -\nabla \psi##, but may also include a reservoir pressure from the inflow. How would you model this, given the small disturbance of the transient interface from equilibrium is some function ##\xi(x,y,z,t)##? There's a way I've been shown, but it doesn't intuitively make sense to me. Any help? Seems like @Chestermiller might know this one?
IMG_5153.jpg
 
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What makes you think that, without gravity, the equilibrium shape will be as you have drawn it?
 
Without body forces surface tension dictates the displacement. According to the Young-Laplace equation the radii of curvature will be equal to minimize energy. I drew it this way for some contact angle, which looks hydrophilic, but for sure it could be anything which changes the shape of the interface but maintains the spherical cap shape.
 
It seems to me the cap should be convex. After all, the liquid will form a sphere if it is small.
 
Chestermiller said:
It seems to me the cap should be convex. After all, the liquid will form a sphere if it is small.
The liquid forms a sphere if it's in a pool of gas, but gas would also form a sphere if in a pool of liquid.

Ultimately this comes down to contact angle. If the liquid is hydrophilic (silicone oil on glass) we'd expect concave; if it's hydrophobic (mercury on glass) we expect convex. I assume the open flow scenario of B) is occurring slow enough that the shape remains spherical.
 
joshmccraney said:
The liquid forms a sphere if it's in a pool of gas, but gas would also form a sphere if in a pool of liquid.

Ultimately this comes down to contact angle. If the liquid is hydrophilic (silicone oil on glass) we'd expect concave; if it's hydrophobic (mercury on glass) we expect convex. I assume the open flow scenario of B) is occurring slow enough that the shape remains spherical.
I think the contact angle is an effect localized to the region near the wall. If there were no wall, the glob of fluid would be a sphere.
 
Chestermiller said:
I think the contact angle is an effect localized to the region near the wall. If there were no wall, the glob of fluid would be a sphere.
Without body forces, equilibrium is only achieved when all free surfaces have the same radius of curvature. Otherwise there will be a force imbalance according to the Young-Laplace equation. But for large scales (say well beyond the capillary length scale) in gravity, I agree with your statement, and in fact the interface will be approximately flat everywhere.

But here we consider no body forces, so the equilibrium interface will always be curved according to the contact-angle.
 

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