Analyzing the Setup
Imagine you are standing next to a U-shaped tube filled with a liquid of density ρ.
When the tube is at rest, the liquid levels in both vertical limbs are perfectly equal due to hydrostatic equilibrium.
But what happens when we spin the tube about the vertical axis of its left limb with a constant angular velocity ω?
As the tube rotates, the liquid in the horizontal connecting tube is thrown outward due to the centrifugal effect.
This causes the liquid level in the right limb to rise and the level in the left limb to fall, creating a height difference H.
Our goal is to find this height difference H at equilibrium.
The Master Equation
Horizontal Pressure Variation
To understand how the pressure varies horizontally, let us analyze a small horizontal element of liquid of length dx at a distance x from the axis of rotation.
Let A be the cross-sectional area of the tube. The mass dm of this tiny element is:
Now, let's look at the forces acting on this element in the horizontal direction.
The pressure on the left side of the element is p, and the pressure on the right side is slightly higher, p+dp.
This pressure difference creates a net force pointing towards the left (towards the axis of rotation):
This net force must provide the necessary centripetal force for the circular motion of the element:
Substituting the mass dm=ρAdx into this equation:
Notice how the cross-sectional area A beautifully cancels out from both sides! We are left with:
Integrating the Pressure Difference
To find the total pressure difference between the left limb (x=0) and the right limb (x=L), we integrate this differential equation:
This equation tells us that the pressure at the bottom of the right limb is higher than the pressure at the bottom of the left limb by 2ρω2L2 due to the rotation.
Vertical Hydrostatic Equilibrium
Now, let's relate this pressure difference to the heights of the liquid columns in the vertical limbs.
The pressure at the bottom of the left limb (p1) and the right limb (p2) are given by hydrostatic pressure:
Subtracting these two equations gives:
where H=h2−h1 is the height difference between the two liquid columns.
Final Calculation
Now, we equate our two independent expressions for the pressure difference p2−p1:
Notice that the density ρ cancels out completely! This means the height difference is independent of the liquid used.
Solving for H, we get the final elegant result:
This is a classic result in fluid dynamics, showing how rotational motion and gravity cooperate to shape the liquid surface.