Increased normal force due to rotation

Click For Summary

Discussion Overview

The discussion revolves around the dynamics of a small sphere rolling inside a hemispherical bowl, specifically focusing on the calculation of the normal force exerted by the sphere on the bowl as it rolls towards the center. Participants explore the implications of energy conservation, the effects of the sphere's radius, and the conditions under which the analysis holds true.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant calculates the normal force exerted by the sphere at the bottom of the bowl, finding it to be greater than the gravitational force due to radial acceleration from rotation.
  • Another participant clarifies the rolling condition, emphasizing that the sphere's contact point has zero velocity relative to the bowl, leading to conservation of mechanical energy.
  • Energy conservation is discussed, with calculations showing the relationship between potential and kinetic energy as the sphere rolls down.
  • Newton's second law is applied to derive the normal force, confirming the earlier calculation of the normal force being 17/7 times the gravitational force.
  • Some participants speculate on the relevance of the assumption regarding the sphere's small radius, questioning whether it was intended to simplify the problem or if it has implications for larger spheres.
  • Concerns are raised about the initial conditions affecting the analysis, particularly if the sphere is as large as the bowl, which could complicate the dynamics.
  • One participant points out that if the sphere starts at the lip of the bowl, it must tip in, while starting from a central position would lead to a direct fall, affecting the normal force calculation.
  • Another participant discusses potential complications arising from the sphere's initial contact conditions, suggesting that energy conservation may not hold in certain scenarios.

Areas of Agreement / Disagreement

Participants express a mix of agreement and disagreement regarding the implications of the sphere's size and initial conditions. While some calculations and principles are accepted, there is no consensus on the relevance of the sphere's radius or the effects of different starting positions.

Contextual Notes

The discussion highlights limitations related to assumptions about the sphere's size and initial conditions, which may affect the validity of energy conservation and the normal force calculations. The dependency on precise definitions and conditions is noted but remains unresolved.

Who May Find This Useful

This discussion may be useful for graduate students studying dynamics, particularly those interested in rotational motion and energy conservation principles in constrained systems.

quarkman
Messages
40
Reaction score
0
I am studying for my graduate exam in physics and came across a strange phenomenon and I would like to make sure I am reasoning it correctly:

Start with a hemispherical bowl and place a small sphere (relatively) at the edge. Let the sphere roll towards the center of the bowl, thus gaining kinetic energy. At the bottom of the bowl, I have calculated the normal force the small sphere exerts on the hemispherical bowl, allowing the radius of the sphere be much less than the radius of the bowl. This force is much greater (by 17/7) than just (mass sphere) x (gravitational acceleration)!

Through my calculations I have reasoned the sphere has both translational and kinetic energy at the bottom of the bowl. From the angular speed of the sphere, I have calculated the required radial acceleration of a point on the edge of the sphere. Now I let the radius of the sphere become very small compared to the radius of the bowl it is in. Now there is a force on the bowl due to this acceleration of the sphere. From Newton's second law I finally determine that the normal force the sphere exerts on the bowl is the sum of the gravitatonal force on the sphere plus this radial acceleration due to the rotation of the sphere:
i.e. Fext = N - mg = ma
with:
a = radial acceleration of sphere
N = normal force
g = gravitational acceleration
m = mass of sphere

This analysis appears sketchy to me and I may not be explaining myself correctly, but I get the answer I am supposed to get for the normal force. Could anyone help clarify this for me? Thanks. :confused:
 
Physics news on Phys.org
Perhaps you think this analysis is clearer:
1. Rolling condition:
This means that the sphere's contact point's velocity is zero (i.e., equal to the velocity of the bowl's contact point)
Two important implications:
a) The frictional force acting on the contact point is static, hence, it does no work, and the mechanical energy of the system is conserved.
b)The angular velocity is related to the velocity of C.M (assuming C.M to be the center of the sphere) by:
[tex]\omega=\frac{v_{c.m}}{r_{s}}[/tex]

2. Energy conservation:
We place the sphere initially at the rim of the bowl, so that it's potential value relative to the bottom of the bowl is mgR
The sphere's potential value when it is at the bottom is [tex]mgr_{s}[/tex]
Hence, we have:
[tex]\frac{m}{2}v^{2}_{c.m}+\frac{m}{2}(\frac{2}{5})v_{c.m}^{2}=mg(R-r_{s})[/tex]
Or:
[tex]v_{c.m}^{2}=\frac{10}{7}g(R-r_{s})[/tex]

3. Newton's 2.law:
Since the C.M is traversing a circle, the net sum of forces must give the centripetal acceleration of C.M:
[tex]N-mg=m\frac{v_{c.m}^{2}}{R-r_{s}}[/tex]
Or, as you found:
[tex]N=\frac{17}{7}mg[/tex]

Note that your assumption of a small sphere radius is irrelevant.
 
Great answer. You have clarified things very well. Thank you very much for your time with this problem. I am interested in any speculation you may have for the reasons why the original problem would have told me to assume a small sphere radius. Was this information there to lead me astray, or is there some implication when the radius of the sphere approaches the radius of the bowl? Thanks again for your help.
 
I think it was included to make the problem "easier"
For example, some might have forgotten that the centripetal acceleration is calculated with respect to the actual radius, R-r; others might forget that the potential difference is mg(R-r), and so on..

Welcome to PF, BTW.
 
To AR
Not querying your maths , but I'm having a puzzling time thinking about a sphere which is as large as the bowl (i.e. it just fits inside) --can you resolve this ?
 
rayjohn:
In that case, the initial potential energy will be equal to the "final" potential energy, which means that the kinetic energies must be equal as well (i.e, zero, since the initial kinetic energy is given as zero)
 
To AR
it's a quibble but it appears to depend on the exact starting assumptions -- if the ball starts on top of the lip it has to tip-in. If it starts inside but central to the lip it will fall in directly, if it's top is at the lip it cannot move hence Fn = mg. his comes as a result of having a finite ball without stating the precise initial conditions.
 
Certainly, rayjohn:
But I solved it explicitly under the assumption that the C.M. of the sphere is only horizontally displaced from the contact point on the rim.
It is certainly true that the initial potential energy will be different if we allow the contact point on the edge to be in contact with a contact point on the sphere that does not have a horizontal normal; however, in that case, there will be an initial, highly problematic phase where energy conservation only can be assumed if the sphere can rotate on the sharp edge with no contact point velocity.
In my view, it is more probable that in such a case, there will be an initial slip; i.e, either loss of contact with the bowl's surface, or a (disssipative) sliding phase along the bowl's surface.
Either of these scenarios would bring in complications not envisaged by the problem maker; in particular, one ought to assume that the accuracy level of simple energy maths is rather poor.
 

Similar threads

  • · Replies 20 ·
Replies
20
Views
3K
  • · Replies 28 ·
Replies
28
Views
3K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 138 ·
5
Replies
138
Views
9K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 10 ·
Replies
10
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 12 ·
Replies
12
Views
2K