Normal force in rotational motion

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Discussion Overview

The discussion revolves around the behavior of the normal force in a rotational motion scenario involving a uniform disk. Participants explore how the normal force changes when the disk is hinged at its rim and experiences angular acceleration, particularly when released from a horizontal position.

Discussion Character

  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Chris questions whether the normal force remains equal to mg when the disk is hinged at its rim and experiences angular acceleration, or if it decreases due to the center of mass accelerating downwards.
  • Some participants propose that the normal force will initially be lower than mg as the disk accelerates downwards, and will increase as the disk rotates, reaching a maximum value greater than mg at the lowest position due to the effects of rotation.
  • Clarifications are made regarding the relationship between the hinge force and the gravitational force, with some suggesting that the hinge force must exceed mg during rotation due to the need for centripetal force.
  • One participant mentions that the variation of the hinge force can be described as a function of the angle, although it may not be the simplest function.

Areas of Agreement / Disagreement

Participants generally agree that the normal force varies during the disk's motion, but there is no consensus on the exact nature of this variation or the complexity of the forces involved.

Contextual Notes

The discussion includes assumptions about the system being frictionless and the nature of the forces acting on the disk, which may not be fully resolved.

cavis
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Hi there,
I've got a conceptual question about the normal force as applied to rotational motion. Suppose you have an object like a uniform disk. If the disk were set up so that its axis of rotation were about its centre of mass, it would just sit there and the normal force would be equal to +mg.

What happens if the disk is instead hinged so that its axis of rotation is at its rim (see attached image)? Here if the disk is held horizontally and then released, it'll experience an angular acceleration and start to rotate. Ultimately were it frictionless, it would oscillate back and forth.

My question is what happens to the normal force in this situation? Does it remain equal to mg since ultimately the hinge isn't accelerating? Or, does the normal force decrease since the centre of mass of the disk is accelerating downwards. Or am I totally confused?

Thanks!

Chris.
 

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The normal force is the force due to axis rod which supports the disk? If so,
this will be initially lower than mg, since the disk accelerates downwards. Continually, as the disk rotates and falls down, the acceleration decreases and so the normal force increases. When the disk is at its lowest position, the normal force will be at its maximum value, which is greater than mg (due to rotation of the disk).
 
Jano L. said:
The normal force is the force due to axis rod which supports the disk? If so,
this will be initially lower than mg, since the disk accelerates downwards. Continually, as the disk rotates and falls down, the acceleration decreases and so the normal force increases. When the disk is at its lowest position, the normal force will be at its maximum value, which is greater than mg (due to rotation of the disk).

Thanks, Jano. This helps. Just to clarify, if the disk we just suspended at its lowest point without rotating, the hinge force would be equal to mg? But, since it's rotating and a radially directed centripetal force is required, the hinge force must exceed mg? Do I have that correct? If I interpret your response correctly, then, the force at the hinge will have a magnitude that varies in quite a complicated manner as the disk undergoes its rotational motion?

Thanks for your help, again.

Chris.
 
cavis said:
the force at the hinge will have a magnitude that varies in quite a complicated manner as the disk undergoes its rotational motion?
Not too complicated: just the force needed to balance the radial component of the gravitational force, + centripetal force. What will make it complicated for large perturbations is the 'circular error', i.e. the extent to which it is not SHM. For small perturbations, taking the SHM approximation, the hinge force will be something like A-Bθ2.
 
Just to clarify, if the disk we just suspended at its lowest point without rotating, the hinge force would be equal to mg? But, since it's rotating and a radially directed centripetal force is required, the hinge force must exceed mg? Do I have that correct?
That's right. Exact variation can be found as a function of the angle, but probably it won't be the simplest function possible.
 

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