Fluid in rotating tube with different initial levels

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The discussion centers on determining the constant C in the pressure equation for fluid in a rotating tube with differing initial fluid heights. The main challenge is establishing the condition to calculate C as a function of the angular velocity ω. Participants note that Bernoulli's principle cannot be applied due to the rotation of the tube. Instead, they suggest considering the total centripetal force required for equilibrium when the pressure at one point is given. Understanding how this force is generated is crucial for solving the problem.
Soren4
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Homework Statement


ddddddd.png


Homework Equations


Fluid in rotation

The Attempt at a Solution


This exercise is quite different from the classic one of fluidi in rotation. Before rotation starts the height in one branch is bigger than in the other, so I do not really know how to approach the problem.

My main difficulty is: how can I determine the constant ##C## in the following expression in this case?

$$p(r,z)=-\rho g z+\frac{1}{2} \rho \omega^2 r^2+C$$

(The frame of reference considered has the ##z## axis towards up and placed on axis of rotation, ##r## is the radial coordinate)

The fact is that I do not really know how to impose the condition for determinimg ##C## as a function of ##\omega## (which is what I want to determine). I think that, once ##C## is determined the rest of exercise is straightforward.

So how can I determine ##C##?
 
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Soren4 said:

Homework Statement


View attachment 103167

Homework Equations


Fluid in rotation

The Attempt at a Solution


This exercise is quite different from the classic one of fluidi in rotation. Before rotation starts the height in one branch is bigger than in the other, so I do not really know how to approach the problem.

My main difficulty is: how can I determine the constant ##C## in the following expression in this case?

$$p(r,z)=-\rho g z+\frac{1}{2} \rho \omega^2 r^2+C$$

(The frame of reference considered has the ##z## axis towards up and placed on axis of rotation, ##r## is the radial coordinate)

The fact is that I do not really know how to impose the condition for determinimg ##C## as a function of ##\omega## (which is what I want to determine). I think that, once ##C## is determined the rest of exercise is straightforward.

So how can I determine ##C##?
In condition a), what is the height of the fluid in the open section? What is the pressure at its top?
 
Soren4 said:
The fact is that I do not really know how to impose the condition for determinimg ##C## as a function of ##\omega## (which is what I want to determine). I think that, once ##C## is determined the rest of exercise is straightforward.
You can't use Bernoulli when the tube is rotated.
Instead:
What total centripetal force is needed to maintain the system in equilibrium when pA = 0.8e5 Pa?
How is this force going to be provided?
 
The book claims the answer is that all the magnitudes are the same because "the gravitational force on the penguin is the same". I'm having trouble understanding this. I thought the buoyant force was equal to the weight of the fluid displaced. Weight depends on mass which depends on density. Therefore, due to the differing densities the buoyant force will be different in each case? Is this incorrect?

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