Solving Centrifugal Forces in a Rotating Coordinate System

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The discussion focuses on resolving equations related to centrifugal forces in a rotating coordinate system, specifically addressing the relationship between two points, A and B. The user presents equations derived from constraints, but struggles with sign conventions and the correctness of their calculations. There is an emphasis on the importance of using a consistent sign convention, particularly that radially outwards is positive. The user acknowledges confusion regarding the application of forces and tension in the context of a non-inertial frame of reference. Clarifications are provided to help the user understand the correct approach to the problem.
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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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