Why do masses on a disk move differently than masses on a string?

  • Thread starter Thread starter PFuser1232
  • Start date Start date
  • Tags Tags
    Disk
Click For Summary

Homework Help Overview

The discussion revolves around a problem involving a rotating disk with two masses connected by a string. The masses slide in a groove on the disk and are initially held in place before being released. The participants are exploring the dynamics of the system, particularly the motion of the masses after the catch is removed and the implications of the forces acting on them.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss the equations of motion for the masses and the role of tension in the string. There is an exploration of the relationship between the radial distances of the masses and the length of the string. Questions are raised about the forces acting on the masses before the catch is released and the implications of the polar coordinate system on their motion.

Discussion Status

The discussion is ongoing, with participants providing feedback on the correctness of the original poster's attempts. There is a focus on understanding the dynamics of the system, particularly why the masses do not remain at a fixed distance from the center of the disk. Some participants are questioning the assumptions made regarding the forces and the nature of the motion (spiral vs. circular).

Contextual Notes

Participants are considering the constraints of the problem, such as the massless nature of the string and the implications of the polar coordinate system on the motion of the masses. There is also uncertainty regarding the initial conditions of the system before the catch is released.

PFuser1232
Messages
479
Reaction score
20

Homework Statement



A disk rotates with constant angular velocity ##ω##, as shown (attached image). Two masses, ##m_A## and ##m_B##, slide without friction in a groove passing through the center of the disk. They are connected by a light string of length ##l##, and are initially held in position by a catch, with mass ##m_A## at distance ##r_A## from the center. Neglect gravity. At ##t = 0## the catch is removed and the masses are free to slide.

Find ##\ddot{r}_A## immediately after the catch is removed, in terms of ##m_A##, ##m_B##, ##l##, ##r_A##, and ##ω##.

Homework Equations



$$\sum_{}^{} \vec{F}_r = m(\ddot{r} - r \dot{\theta}^2) \hat{r}$$

3. The Attempt at a Solution


The particles are constrained to move according to ##r_A + r_B = l##. Differentiating twice with respect to time, we get ##\ddot{r}_A = -\ddot{r}_B##. Each particle experiences a force of magnitude ##T## where ##T## is the tension in the string. Writing down the equations of motion:
$$-T = -m_A(\ddot{r}_A - r_A \omega^2)$$
$$-T = -m_B(\ddot{r}_B - r_B \omega^2)$$
Eliminating ##T## and substituting ##r_B = l - r_A## and ##\ddot{r}_B = -\ddot{r}_A## we get:
$$\ddot{r}_A = \omega^2 \frac{m_A r_A + m_B r_A - m_B l}{m_A + m_B}$$
Is this answer correct?
Also, before ##t = 0##, were ##m_A## and ##m_B## acted upon by an additional force ##F## such that ##|F - T| = mr\omega^2##? Or was the string fixed?
It seems to me that my physical intuition was wrong (again). I don't understand why the ##\ddot{r}## terms appear in the equations of motion. Why can't the masses remain at a fixed distance from the circle?
My last question is really about the polar coordinate system and the constraint I used above, namely ##l = r_A + r_B##.
If the disk was big enough, and the string was entirely on one side of the circle (the origin no longer lies on the string), then we would be forced to interpret the radial coordinate of the particle closer to the pole as negative, otherwise the sum of the radial coordinates would not equal the length of the string, right?
Sometimes, I find the non-uniqueness of polar coordinates really frustrating
 

Attachments

  • image.jpg
    image.jpg
    15.7 KB · Views: 580
Physics news on Phys.org
MohammedRady97 said:
Is this answer correct?
Looks correct.

We don't know how the system was hold in place before t=0, I don't see how this would matter.

MohammedRady97 said:
Why can't the masses remain at a fixed distance from the circle?
They can, if their forces are in equilibrium?

MohammedRady97 said:
If the disk was big enough, and the string was entirely on one side of the circle (the origin no longer lies on the string), then we would be forced to interpret the radial coordinate of the particle closer to the pole as negative, otherwise the sum of the radial coordinates would not equal the length of the string, right?
That, or change the equation for l (and for the force balances) to keep two positive radial distances.
 
mfb said:
Looks correct.

We don't know how the system was hold in place before t=0, I don't see how this would matter.

They can, if their forces are in equilibrium?

That, or change the equation for l (and for the force balances) to keep two positive radial distances.

Why do the particles move around in a spiral, rather than a circle?
 
MohammedRady97 said:
Why do the particles move around in a spiral, rather than a circle?
Assuming they move in a circle, you can consider the forces on one and deduce the tension in the string. Likewise the other. If the two tensions are not the same then your assumption must be false.
 
haruspex said:
Assuming they move in a circle, you can consider the forces on one and deduce the tension in the string. Likewise the other. If the two tensions are not the same then your assumption must be false.

The two tensions are the same, since the string is massless. What I'm asking is: why are there ##\ddot{r}## terms in the equations of motion in the first place?
 
MohammedRady97 said:
The two tensions are the same, since the string is massless. What I'm asking is: why are there ##\ddot{r}## terms in the equations of motion in the first place?
You seem to be saying you want an explanation for the ##\ddot r## term in ##|\Sigma F_r| = m(\ddot r - r {\dot \theta}^2)##. Is that right? You should be able to find a derivation online.
 
haruspex said:
You seem to be saying you want an explanation for the ##\ddot r## term in ##|\Sigma F_r| = m(\ddot r - r {\dot \theta}^2)##. Is that right? You should be able to find a derivation online.

I'm quite familiar with the derivation of acceleration in polar coordinates.
I'm just wondering why it appears in some cases, but not others.
 
MohammedRady97 said:
I'm quite familiar with the derivation of acceleration in polar coordinates.
I'm just wondering why it appears in some cases, but not others.
Well, it will be zero for circular motion of course. Can you list some other case?
 

Similar threads

Replies
6
Views
2K
Replies
5
Views
3K
Replies
5
Views
4K
Replies
13
Views
6K
  • · Replies 2 ·
Replies
2
Views
9K
Replies
1
Views
1K
  • · Replies 11 ·
Replies
11
Views
8K
  • · Replies 1 ·
Replies
1
Views
1K
Replies
6
Views
7K
  • · Replies 14 ·
Replies
14
Views
5K