Ring with beads

A light ring of radius r r wearing two identical beads A A and B B each of mass m m is hinged at its top point O O in such a way that it can rotate freely in its plane about a horizontal axis through the hinge O O . The bead A A is affixed on the ring and the bead B B is held so that they occupy position of the ends of the horizontal diameter of the ring and the system stays system stays motionless. The ring is well lubricated so that the bead B B can slide with negligible friction on the ring.

Determine acceleration of the beads immediately after the bead B B is released and final angle of rotation of the ring when all motion ceases after a long time due to the little viscous friction between the bead B B and the ring.

Acceleration due to the gravity is g g .

Answer will come in the form of

Acceleration of bead A : α g \alpha g
Acceleration of bead B : β g \beta g
Final angle of rotation : t a n 1 γ tan^{-1} \gamma

Type your answer as α + β + γ = ? \large \alpha+ \beta+\gamma=?

Thanks in advance, if you are going to post a solution.


The answer is 2.025.

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1 solution

Karan Chatrath
Sep 19, 2020

I have used the Lagrangian formulation to solve this. Any other fundamental approach would be too tedious, in my opinion.

Say at a general time t t the ring has rotated anticlockwise about O O by θ \theta . At the same time, B has rotated along the ring clockwise by an angle ϕ \phi . Based on this, the coordinates of points A and B are:

x A = R sin θ R cos θ x_A = R\sin{\theta} - R \cos{\theta} y A = R cos θ R sin θ y_A = -R\cos{\theta} - R \sin{\theta}

x B = R sin θ + R cos ( ϕ θ ) x_B = R\sin{\theta} + R \cos(\phi-\theta) y B = R cos θ R sin ( ϕ θ ) y_B = -R\cos{\theta} - R \sin(\phi-\theta)

I request the reader to try visualising the geometry and deriving the above coordinates by him/her self.

Having done the above, the kinetic energy of the system can be derived as such:

T = m 2 ( x ˙ A 2 + y ˙ A 2 ) + m 2 ( x ˙ B 2 + y ˙ B 2 ) \mathcal{T} = \frac{m}{2}(\dot{x}_A^2 + \dot{y}_A^2) + \frac{m}{2}(\dot{x}_B^2 + \dot{y}_B^2)

The potential energy of the system is:

V = m g y A + m g y B \mathcal{V} = mgy_A + mgy_B

After simplification, the expression turn out to be:

T = m 2 ( 4 R 2 θ ˙ 2 + R 2 ϕ ˙ 2 2 R 2 ϕ ˙ θ ˙ + 2 R 2 θ ˙ 2 sin ϕ 2 R 2 ϕ ˙ θ ˙ sin ϕ ) \mathcal{T} = \frac{m}{2}\left(4R^2 \dot{\theta}^2 +R^2 \dot{\phi}^2 -2R^2\dot{\phi}\dot{\theta} +2R^2\dot{\theta} ^2\sin{\phi} - 2R^2\dot{\phi}\dot{\theta}\sin{\phi}\right)

V = m g ( 2 R cos θ + R sin θ + R sin ( ϕ θ ) ) \mathcal{V} = -mg(2R\cos{\theta} + R\sin{\theta} + R\sin(\phi-\theta ))

Lagrange's equations read:

d d t ( T θ ˙ ) T θ + V θ = 0 \frac{d}{dt}\left(\frac{\partial \mathcal{T}}{\partial \dot{\theta}}\right) - \frac{\partial \mathcal{T}}{\partial \theta} + \frac{\partial \mathcal{V}}{\partial \theta}=0

d d t ( T ϕ ˙ ) T ϕ + V ϕ = 0 \frac{d}{dt}\left(\frac{\partial \mathcal{T}}{\partial \dot{\phi}}\right) - \frac{\partial \mathcal{T}}{\partial \phi} + \frac{\partial \mathcal{V}}{\partial \phi}=0

Doing this entire derivative crunching gives the required equations of motion which are:

4 m R 2 θ ¨ m R 2 ϕ ¨ + 2 m R 2 θ ¨ sin ϕ + 2 m R 2 θ ˙ ϕ ˙ cos ϕ m R 2 ϕ ¨ sin ϕ m R 2 ϕ ˙ 2 cos ϕ + 2 m g R sin θ m g R cos θ + m g R cos ( ϕ θ ) = 0 4mR^2 \ddot{\theta} - mR^2 \ddot{\phi} + 2mR^2\ddot{\theta}\sin{\phi} + 2mR^2\dot{\theta}\dot{\phi}\cos{\phi}- mR^2\ddot{\phi}\sin{\phi} - mR^2\dot{\phi}^2\cos{\phi} + 2mgR\sin{\theta} -mgR\cos{\theta} + mgR\cos(\phi - \theta)=0

m R 2 ϕ ¨ m R 2 θ ¨ m R 2 θ ¨ sin ϕ m R 2 θ ˙ 2 cos ϕ m g R cos ( ϕ θ ) = 0 mR^2 \ddot{\phi} - mR^2\ddot{\theta} - mR^2\ddot{\theta}\sin{\phi} - mR^2\dot{\theta}^2\cos{\phi} -mgR\cos(\phi - \theta)=0

Note that the system is at rest at the beginning so the initial conditions are:

θ ( 0 ) = ϕ ( 0 ) = θ ˙ ( 0 ) = ϕ ˙ ( 0 ) = 0 \theta(0) = \phi(0) = \dot{\theta}(0) = \dot{\phi}(0)=0

At t = 0 t=0 applying the initial conditions in the above equations and simplifying, gives the following two equations:

ϕ ¨ = 4 θ ¨ \ddot{\phi} = 4\ddot{\theta} ϕ ¨ θ ¨ = g R \ddot{\phi} - \ddot{\theta} = \frac{g}{R}

Solving gives:

ϕ ¨ = 4 g 3 R \ddot{\phi} = \frac{4g}{3R} θ ¨ = g 3 R \ddot{\theta} = \frac{g}{3R}

Finally, the acceleration of A and B at t = 0 t=0 is computed as follows:

a A = x ¨ A ( 0 ) 2 + y ¨ A ( 0 ) 2 a_A = \sqrt{\ddot{x}_A(0)^2 + \ddot{y}_A(0)^2} a B = x ¨ B ( 0 ) 2 + y ¨ B ( 0 ) 2 a_B = \sqrt{\ddot{x}_B(0)^2 + \ddot{y}_B(0)^2}

Crunching out all derivatives and substituting all initial conditions are derived earlier gives:

a A = g 2 3 a_A = \frac{g\sqrt{2}}{3} a B = g 10 3 a_B = \frac{g\sqrt{10}}{3}

Now, when the system finally comes to rest due to viscous friction, the system will be in its state of stable equilibrium. At this stage:

ϕ ˙ = θ ˙ = ϕ ¨ = θ ¨ = 0 \dot{\phi} = \dot{\theta} = \ddot{\phi} = \ddot{\theta}=0

Substituting in Lagrange's equations gives:

2 sin θ cos θ + cos ( ϕ θ ) = 0 2\sin{\theta} -\cos{\theta} + \cos(\phi - \theta)=0 cos ( ϕ θ ) = 0 \cos(\phi - \theta)=0 tan θ = 1 2 \implies \tan{\theta} = \frac{1}{2} Finally:

α = 2 3 \boxed{\alpha = \frac{\sqrt{2}}{3}} β = 10 3 \boxed{\beta = \frac{\sqrt{10}}{3}} γ = 1 2 \boxed{\gamma = \frac{1}{2}}

I have left out intermediate steps, as typing all of it would be tedious. You can try to work them out by yourself

Karan Chatrath - 8 months, 3 weeks ago

This problem should be marked as level 5.

Karan Chatrath - 8 months, 3 weeks ago

Log in to reply

I don't care for that because Brilliant gives any level to any problem by closing his eyes :)

Talulah Riley - 8 months, 3 weeks ago

@Karan Chatrath Thank you so much.

Talulah Riley - 8 months, 3 weeks ago

@Karan Chatrath By the way, sir i will upload a attempt of a problem within 1 hour in notes.

Talulah Riley - 8 months, 3 weeks ago

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