A 1 k g bead slides from rest under the pull of gravity from the point ( − 1 m , 0 m ) to the point ( 0 m , − 1 m ) along a wire in the shape of a circle centered on the origin, as shown above.
The wire is rough, and exerts a retarding tangential friction force F f = μ F normal on the bead, with μ = 2 1 .
Find the speed of the bead ( in m/s ) when it arrives at ( 0 m , − 1 m ) .
Note:
g
=
1
0
m
/
s
2
.
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I'm impressed. How complex do you think the path can get before purely analytical solutions become impossible? Or perhaps infeasible, if not strictly impossible.
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If you look at my further note, I set out a fairly general case. Obtaining the first integral of the equations explicitly - basically, the energy equation - requires us to perform an integral that could be seriously difficult, if not impossible.
I just have a question, if the path would have been say a Sine wave instead of a circle how would we have dealt with that ?
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Friction F would act tangentially to the curve, and the normal reaction N would act along the principal normal. If the curve was the shape y = f ( x ) , then the position vector of the particle would be r = ( x , f ( x ) ) and we can differentiate this twice to obtain the equation m r ¨ = N + F + m g ( 0 , − 1 ) The only unknown on the RHS is the modulus of N (all the vector directions can be expressed in terms of f ( x ) ). We could take components and thereby eliminate this, obtaining a differential equation for x .
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Actually I am a bit confused about the last equation. How differentiating twice we obtain that. It would be very helpful for me if you please explain it a bit if you have time.
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@Aditya Narayan Sharma – Suppose that the wire has shape given by the equation y = f ( x ) , where f has a minimum at x = 0 . The position vector of the particle is r r ˙ r ¨ = ( f ( x ) x ) = ( f ′ ( x ) 1 ) x ˙ = ( f ′ ( x ) 1 ) x ¨ + ( f ′ ′ ( x ) 0 ) x ˙ 2 and we must have N = λ ( 1 − f ′ ( x ) ) F = μ λ ( f ′ ( x ) 1 ) for some function λ . Recall that F has to be tangential to the curve, while N has to be normal to the curve and upward-pointing. The equation of motion is m r ¨ m ( f ′ ( x ) 1 ) x ¨ + m ( f ′ ′ ( x ) 0 ) x ˙ 2 = N + F + m g ( − 1 0 ) = λ ( 1 − f ′ ( x ) ) + μ λ ( f ′ ( x ) 1 ) + m g ( − 1 0 ) Taking the scalar product of this equation with ( f ′ ( x ) 1 ) and ( 1 − f ′ ( x ) ) , we obtain m ( 1 + f ′ ( x ) 2 ) 2 x ¨ + m f ′ ( x ) f ′ ′ ( x ) x ˙ 2 m f ′ ′ ( x ) x ˙ 2 = μ λ ( 1 + f ′ ( x ) 2 ) − m g f ′ ( x ) = λ ( 1 + f ′ ( x ) 2 ) − m g Eliminating λ yields ( 1 + f ′ ( x ) 2 ) x ¨ + ( f ′ ( x ) f ′ ′ ( x ) − μ f ′ ′ ( x ) ) x ˙ 2 d x d [ 2 1 ( 1 + f ′ ( x ) 2 ) e − 2 μ tan − 1 f ′ ( x ) x ˙ 2 ] = g ( μ − f ′ ( x ) ) = g ( μ − f ′ ( x ) ) e − 2 μ tan − 1 f ′ ( x ) At this point, we would need to know the explicit form of f ( x ) to proceed further...
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@Mark Hennings – Thanks a lot, This was an awesome explanation.
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@Aditya Narayan Sharma – How do you move from step 3 to step 4? How does e − 2 μ θ appear in the step 4?
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@Rohit Gupta – It is a matter of looking for an integrating factor. Since d θ d ( 2 1 θ ˙ 2 ) = θ ¨ , multiplying by e − 2 μ θ is what it takes to make the LHS of the equation exact.
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@Mark Hennings – Well, this is a very clever adjustment. Is there a method to follow to find such integrating factors or one has to do the hit and trail approach to reach to it?
Moreover, in the second equation, μ N − m g sin θ = m r θ ¨ , should it be m g sin θ − μ N = m r θ ¨ ? This is because the speed is increasing, thus the forces in the direction of the speed must be greater.
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@Rohit Gupta – Look up solving first order differential equations for the technique for finding integrating factors. In brief, the integrating factor for the equation d x d y + a ( x ) y = b ( x ) is e ∫ a ( x ) d x
My equation is correct, Firstly, my θ is not the θ that Steven used. It is the angle with the downward vertical. Thus, while θ is positive, θ ˙ and θ ¨ are negative. The tangential component of gravity acts in the direction of negative θ , and the friction force acts in the opposite direction.
@Mark Hennings – the theta' term disappeared because the derivative is wrt theta right? clever!
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@Dhruv G – If you prefer, multiply the whole equation by θ ˙ and then integrate with respect to t .
See @Mark Hennings for a purely analytical approach. I will provide a hybrid analytical-computational solution which eases the mathematical burden, with a computer taking up the slack.
Split the gravitational force into two parts. The tangential component is:
F g t = m g c o s θ
The normal component is (referenced toward the origin):
F g n = − m g s i n θ
Write an expression for the centripetal force in relation to the normal reaction force and the normal component of the gravity force. Let the variable v refer to the bead's speed.
F c = R m v 2 = − m g s i n θ + F n r ⟹ F n r = m g s i n θ + R m v 2
The net tangential force with friction is therefore:
F t = m g c o s θ − μ [ m g s i n θ + R m v 2 ] = m d t d v d t d v = v ˙ = g c o s θ − μ [ g s i n θ + R v 2 ]
Then we can solve iteratively in the following way (I used a time step Δ t = 1 0 − 6 s e c ):
v k = v k − 1 + v ˙ k − 1 Δ t θ k = θ k − 1 + θ ˙ k − 1 Δ t v ˙ k = g c o s θ k − μ [ g s i n θ k + R v k 2 ] θ ˙ k = R v k
Run the algorithm until θ = 2 π . The resulting final velocity comes out to be approximately 1 . 3 7 m / s .
The potential energy at rest at elevation R is dissipated as friction heat energy and is used to speed up the particle's speed (kinetic energy,) and the net difference is the work exhibited by the tangential force displaced R units. The centripetal force is only for changing direction and generates no work as it is normal on displacement.
Potential energy - Friction heat - Kinetic energy = Work of tangential force
cos(a)×PE - u sin(a)×PE - (2u/R)×KE = Ft×R
PE = potential E = m g R KE = Kinetic E = 0.5 m v^2 Fc = centripetal force R = radius of circle a = angle between radius & horizontal axis u = coefficient of friction m = mass Ac = centripetal acceleration = v^2/R v' = dv/dt = At = tangential acceleration Ft = tangential force = m At = m v'
Substitution:
cos(a) m g R - u sin(a) m g R - 2 u 0.5 m v^2 / R = m v' R
(Devide by R)
mg cos(a) - u mg sin(a) - u m Ac = m v'
mg cos(a) - u [mg sin(a) + m Ac] = m v'
Radial forces Fn = normal force = mg sin(a) + m Ac
Ff = frictional force = u Fn Fg = gravitational force = mg
Tangential forces Fg cos(a) - Ff = m At
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Let θ be the angle that the radius to the particle makes with the downward vertical, r the radius and m the mass of the particle. If N is the normal reaction, and F = μ N the friction force on the particle, then the radial and transverse equations of motion are: N − m g cos θ = m r θ ˙ 2 μ N − m g sin θ = m r θ ¨ Eliminating N yields m r θ ¨ − μ m r θ ˙ 2 θ ¨ − μ θ ˙ 2 d θ d [ 2 1 θ ˙ 2 e − 2 μ θ ] = m g ( μ cos θ − sin θ ) = r g ( μ cos θ − sin θ ) = r g ( μ cos θ − sin θ ) e − 2 μ θ Since the particle starts at rest when θ = 2 1 π , the particle's speed at angle θ is v ( θ ) 2 = 2 r g e 2 μ θ ∫ θ 2 1 π ( sin θ − μ cos θ ) e − 2 μ θ d θ With r = 1 , g = 1 0 , μ = 2 1 , the particle's speed at the bottom is v ( 0 ) , where v ( 0 ) 2 = 1 0 ∫ 0 2 1 π ( 2 sin θ − cos θ ) e − θ d θ = 5 ( 1 − 3 e − 2 1 π ) and hence the answer is v ( 0 ) = 1 . 3 7 1 7 9 .