Solving Centrifugal Forces in a Rotating Coordinate System

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Homework Help Overview

The discussion revolves around analyzing centrifugal forces in a rotating coordinate system, specifically focusing on the dynamics of two masses, A and B, connected by a tension force. Participants are exploring the implications of their chosen sign conventions and the resulting equations of motion.

Discussion Character

  • Conceptual clarification, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants are attempting to derive equations based on the forces acting on the masses and are questioning the correctness of their sign conventions. There is a focus on the relationship between the radial distances and the forces involved.

Discussion Status

The discussion is active, with participants providing feedback on each other's reasoning and questioning the application of sign conventions. Some guidance has been offered regarding the typical sign conventions used in radially symmetric problems, but no consensus has been reached on the specific equations or their interpretations.

Contextual Notes

Participants are working within the constraints of a rotating frame of reference and are grappling with the implications of using fictitious forces. There is an acknowledgment of the complexity of the problem, particularly for those new to the topic.

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Homework Statement
A disk rotates with constant angular velocity ω. Two masses A & B slide without friction in a groove passing through center of disk. They are connected by string of length 'l' and are initially held in position by catch with mass A at a distance r(A) from the center. Neglect gravity. At t=0 the catch is removed and masses are free to slide. Find r''(A) immediately after catch is removed in terms of A,B,l,r(A) & ω.
Relevant Equations
F(A)-T=m(A)*r''(A)

T-F(B)=m(B)*r''(B)

r(A)+r(B)=l
I am also attaching picture of the figure as well as my diagram to showcase the forces.

I have devised these equations because as per the question, r(A) is acting like a reference.

The constraint r(A)+r(B)=l--------(i) transforms to r''(B)= - r''(A) ------- (ii)

Using-

F(A)-T=m(A)*r''(A)

T-F(B)=m(B)*r''(B)

Adding both & using (i) & (ii), F(A)-F(B)= r''(A) {m(A)-m(B)}

r(A)*ω^2 [m(A)+m(B)] - m(B)*l*ω^2= r''(A) {m(A)-m(B)}

{ r(A)*ω^2 [m(A)+m(B)] - m(B)*l*ω^2} /{m(A)-m(B)}

This answer is not coming out to be correct. I sense I have taken force directions wrong but unable to understand why.
 

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warhammer said:
T-F(B)=m(B)*r''(B)
Can you see the sign error there?
 
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haruspex said:
Can you see the sign error there?

I used this sign convention because r(A) would increase if A tended to move away from the center. Since I used that as reference, I also applied the similar convention for B, T is 'towards' A and F(B) away from it. Can I not do that?
 
warhammer said:
I used this sign convention because r(A) would increase if A tended to move away from the center. Since I used that as reference, I also applied the similar convention for B, T is 'towards' A and F(B) away from it. Can I not do that?
But elsewhere you used r(B) for B's distance from the centre. The tension tends to reduce that and the centrifugal force to increase it.
 
haruspex said:
But elsewhere you used r(B) for B's distance from the centre. The tension tends to reduce that and the centrifugal force to increase it.

I replaced it with (l-r(A)) and r''(A).

(I'm sorry if my questions seem silly sir. It's all new to me and I've hit an understanding block).
 
EDIT: Changed answer to reflect working in the rotating coordinate system.

Looks like F(A) and F(B) are the (fictitious) centrifugal forces. So you are working in the non-inertial rotating frame-of-reference of the disc.

The usual sign-convention for these radially symmetric problems is 'radially outwards is positive'.

Using this sign convention:
F(A) - T = m(A)*r''(A) is fine because F(A) is outwards and T in inwards
So you need to address the equation T - F(B) = m(B)*r''(B).
 
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Steve4Physics said:
EDIT: Changed answer to reflect working in the rotating coordinate system.

Looks like F(A) and F(B) are the (fictitious) centrifugal forces. So you are working in the non-inertial rotating frame-of-reference of the disc.

The usual sign-convention for these radially symmetric problems is 'radially outwards is positive'.

Using this sign convention:
F(A) - T = m(A)*r''(A) is fine because F(A) is outwards and T in inwards
So you need to address the equation T - F(B) = m(B)*r''(B).

Thank you so much for your help sir.
 

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