Question icon
Grade 12th passMechanics

A U-tube of a very small bore, with its limbs in a vertical plane and filled with a liquid of density ρ, up to a height of h, is rotated about a vertical axis, with an angular velocity of ω, as shown in the Figure. The radius of each limb from the axis of rotation is R. Let pa be the atmospheric pressure and g, the gravitational acceleration. The angular velocity at which the pressure at the point O becomes half of the atmospheric pressure is given by

Question image for A U-tube of a very small bore, with its limbs in
Profile image of Vivek S
6 Years agoGrade 12th pass
Answers icon

1 Answer

Profile image of ROSHAN MUJEEB
6 Years ago

To find the angular velocity at which the pressure at point O in the U-tube becomes half of the atmospheric pressure, we can analyze the situation using the principles of fluid mechanics and centrifugal force. Let’s break it down step-by-step.

Understanding the Problem

The U-tube is filled with a liquid of density ρ and has its limbs in a vertical plane. When it is rotated about a vertical axis with an angular velocity ω, the pressure at any point within the liquid will change due to the effects of rotation. We need to determine the condition where the pressure at point O, which is located at the bottom of the U-tube, becomes half of atmospheric pressure (pa/2).

The Pressure Equation

In a rotating system, the pressure at a point can be given by the following equation:

  • P = pa + ρgh - ρ(Rω²)

Here:

  • P is the pressure at point O.
  • pa is the atmospheric pressure.
  • ρ is the liquid density.
  • g is the acceleration due to gravity.
  • h is the height of the liquid column above point O.
  • R is the radius of the U-tube limb from the axis of rotation.
  • ω is the angular velocity.

Setting Up the Condition

We need to find the angular velocity ω such that the pressure P at point O equals half of the atmospheric pressure:

  • P = pa / 2

Substituting this into our pressure equation gives:

  • pa / 2 = pa + ρgh - ρ(Rω²)

Rearranging this equation leads to:

  • ρ(Rω²) = pa + ρgh - (pa / 2)
  • ρ(Rω²) = (pa / 2) + ρgh

Solving for Angular Velocity

Now we can isolate ω:

  • Rω² = (pa / (2ρ)) + h g
  • ω² = [(pa / (2ρ)) + hg] / R
  • ω = sqrt{[(pa / (2ρ)) + hg] / R}

Final Expression

Thus, the angular velocity ω at which the pressure at point O becomes half of the atmospheric pressure can be expressed as:

  • ω = sqrt{(pa / (2ρR)) + (hg / R)}

Real-World Application

This principle has practical implications in various fields such as engineering and meteorology, where understanding fluid behavior under rotational forces is crucial. For example, in designing centrifuges or understanding atmospheric pressure changes in rotating systems, this knowledge can be applied effectively.

By analyzing the pressures exerted within the U-tube based on the centrifugal effects, we gain critical insights into fluid dynamics in rotational systems.