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Spin, Pressure and the Paraboloid

Irodov 1.330DifficultyDifficulty 3 of 5UniquenessUniqueness 3 of 5

Problem Irodov 1.330

A cylindrical vessel containing water is spun about its own vertical axis at a constant angular velocity ω\omega. Find:

  1. the shape taken up by the free surface of the water;

  2. how the water pressure along the bottom of the vessel varies with distance from the axis, given that the pressure at the central point of the bottom is p0p_0.

The cylindrical vessel of water, turning steadily about its own vertical axis at angular velocity ω.

The cylindrical vessel of water, turning steadily about its own vertical axis at angular velocity ω\omega.

Given
  • ω\omega (angular velocity)
  • p0p_0 (pressure on the axis at the bottom)
Find
Find (a) z(r)z(r), the shape of the free surface, and (b) p(r)p(r), the pressure along the bottom

Solution

Step 1Radial pressure balance in the rotating vessel

Once the water rotates rigidly with the vessel, every fluid ring at radius rr needs a net inward (centripetal) force ρω2r\rho\omega^2r per unit volume, supplied by the radial pressure gradient:

∂p∂r=ρω2r.(1) \frac{\partial p}{\partial r} = \rho\omega^2 r. \tag{1}

Vertically the fluid is in ordinary hydrostatic equilibrium, with ∂p/∂z=−ρg\partial p/\partial z = -\rho g as usual.

Step 2Shape of the free surface

Along the free surface the pressure is everywhere atmospheric, so pp is constant there and dp=0dp=0; substituting the radial gradient (1) together with ∂p/∂z=−ρg\partial p/\partial z=-\rho g relates drdr and dzdz along the surface.

0=∂p∂rdr+∂p∂zdz=ρω2r dr−ρg dz.0 = \frac{\partial p}{\partial r}dr + \frac{\partial p}{\partial z}dz = \rho\omega^2 r\,dr - \rho g\,dz.

Solving for the slope dz/drdz/dr and integrating from the vertex (r=0r=0, taken as z=0z=0) out to radius rr gives the surface height there.

dzdr=ω2gr⟹∫0zdz′=ω2g∫0rr′ dr′=ω2g[r′22]0r.\frac{dz}{dr} = \frac{\omega^2}{g}r \quad\Longrightarrow\quad \int_0^{z} dz' = \frac{\omega^2}{g}\int_0^{r} r'\,dr' = \frac{\omega^2}{g}\left[\frac{r'^2}{2}\right]_0^{r}.
z=ω22gr2z = \dfrac{\omega^2}{2g}r^2
(2)
The free surface in cross section: a parabola in section and a paraboloid of revolution in the vessel. Here z is measured from the lowest point of the surface, on the axis, and R is the vessel's own radius.

The free surface in cross section: a parabola in section and a paraboloid of revolution in the vessel. Here zz is measured from the lowest point of the surface, on the axis, and RR is the vessel’s own radius.

Step 3Pressure along the bottom

At any fixed height, in particular the vessel’s bottom, integrate (1) from the axis (r=0r=0, where p=p0p=p_0) outward:

p(r)−p0=∫0rρω2r′ dr′=12ρω2r2.p(r) - p_0 = \int_0^r \rho\omega^2 r'\,dr' = \frac{1}{2}\rho\omega^2r^2.
z=ω22gr2,p=p0+12ρω2r2z = \dfrac{\omega^2}{2g}r^2, \qquad p = p_0+\dfrac{1}{2}\rho\omega^2r^2
(3)
Check

Both results collapse to the stationary case (z=0z=0 everywhere, p=p0p=p_0 everywhere) as ω→0\omega\to0, and both grow without bound as rr increases, exactly as expected for a paraboloid whose curvature is set by ω\omega: a faster spin lifts the rim higher and raises the bottom pressure faster with radius.

Remark

The surface shape and the bottom pressure share coefficients matching up to the factor ρg\rho g, ω2/(2g)\omega^2/(2g) and ρω2/2\rho\omega^2/2 respectively, both traceable to the same radial balance (1): the extra height the surface must climb at radius rr to keep the pressure atmospheric there is exactly the height of water whose weight would supply that radius’s own centripetal pressure. Rotation converts a spatial pressure gradient into a tilted free surface precisely because gravity is what converts pressure into height in the first place.