Bead on Circular Wire: Related Rates Reloaded

The following question is inspired by this problem.

The diagram depicts a bead sliding on a rough circular wire (due to the influence of gravity) as shown below:

The circular arc is of unit radius centred at the origin. The bead is of unit mass and slides down the surface starting from the point ( 1 , 0 ) (-1,0) . Initially, the downward speed of the bead is 0.5 m / s 0.5 m/s . The coefficient of friction of the wire is μ = 0.5 \mu = 0.5 .

The goal of this question is to find the value of A A at time t = 0.5 s t = 0.5 s where:

A = d θ ˙ d θ A = \frac{d\dot{\theta}}{d\theta}

Enter your answer as 1000 A \lfloor\mid 1000A \mid \rfloor

Take g = 10 m / s 2 g = 10 m/s^2


The answer is 1054.

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3 solutions

Mark Hennings
May 27, 2019

The differential equation of the particle is m ( sin θ cos θ ) θ ¨ + m ( cos θ sin θ ) θ ˙ 2 = N ( cos θ sin θ ) + μ N ( sin θ cos θ ) + m g ( 0 1 ) m\binom{\sin\theta}{-\cos\theta} \ddot{\theta} + m\binom{\cos\theta}{\sin\theta}\dot{\theta}^2 \; = \; N\binom{\cos\theta}{\sin\theta} + \mu N\binom{-\sin\theta}{\cos\theta} + mg\binom{0}{-1} where N N is the magnitude of the normal reaction. Thus m θ ¨ = μ N + m g cos θ m θ ˙ 2 = N m g sin θ m\ddot{\theta} \; = \; -\mu N + mg\cos\theta \hspace{2cm} m\dot{\theta}^2 \; = \; N - mg\sin\theta and hence, eliminating N N , θ ¨ + μ θ ˙ 2 = g ( cos θ μ sin θ ) d d θ [ 1 2 θ ˙ 2 e 2 μ θ ] = g ( cos θ μ sin θ ) e 2 μ θ 1 2 θ ˙ 2 e 2 μ θ = g 4 μ 2 + 1 [ 3 μ e 2 μ θ cos θ + ( 1 2 μ 2 ) e 2 μ θ sin θ 3 μ ] + 1 8 θ ˙ 2 = 2 g 4 μ 2 + 1 [ 3 μ cos θ + ( 1 2 μ 2 ) sin θ 3 μ e 2 μ θ ] + 1 4 e 2 μ θ ( ) \begin{aligned} \ddot{\theta} + \mu\dot{\theta}^2 & = \; g(\cos\theta - \mu\sin\theta)\\ \frac{d}{d\theta}\left[\tfrac12\dot{\theta}^2e^{2\mu\theta}\right] & = \; g(\cos\theta - \mu\sin\theta)e^{2\mu\theta} \\ \tfrac12\dot{\theta}^2e^{2\mu\theta} & = \; \frac{g}{4\mu^2+1}\left[3\mu e^{2\mu\theta}\cos\theta + (1 - 2\mu^2)e^{2\mu\theta}\sin\theta -3\mu\right] + \tfrac18\\ \dot{\theta}^2 & = \; \frac{2g}{4\mu^2+1}\left[3\mu\cos\theta + (1 - 2\mu^2)\sin\theta - 3\mu e^{-2\mu\theta}\right] + \tfrac14e^{-2\mu\theta} \hspace{2cm} (\star) \end{aligned} With g = 10 g=10 and μ = 1 2 \mu=\tfrac12 we want to find the value of θ \theta attained at time t = 1 2 t=\tfrac12 . Thus we need to solve the equation 1 2 = 0 θ 2 d u 60 cos u + 20 sin u 59 e u \tfrac12 \; = \; \int_0^\theta \frac{2 du}{\sqrt{60\cos u + 20\sin u - 59e^{-u}}} and this can be done numerically, obtaining θ = θ 0 = 1.0537654 \theta = \theta_0 = 1.0537654 . We can now calculate θ ˙ ( θ 0 ) \dot{\theta}(\theta_0) and θ ¨ ( θ 0 ) \ddot{\theta}(\theta_0) , using ( ) (\star) and the fact that θ ¨ = 10 cos θ 5 sin θ 1 2 θ ˙ 2 \ddot{\theta} = 10\cos\theta - 5\sin\theta - \tfrac12\dot{\theta}^2 , obtaining A = θ ¨ ( θ 0 ) θ ˙ ( θ 0 ) = 1.05447 A \; = \; \frac{\ddot{\theta}(\theta_0)}{\dot{\theta}(\theta_0)} \; = \; -1.05447 making the required answer equal to 1054 \boxed{1054} .

Steven Chase
May 26, 2019

This was a fun problem. Here are my two cents. Let ( x , v , a ) (x,v,a) be the tangential position, velocity, and acceleration, respectively.

A = d θ ˙ d θ = d θ ˙ / d t d θ / d t = θ ¨ θ ˙ = a v \large{A = \frac{d \dot{\theta}}{d \theta} = \frac{d \dot{\theta} / dt}{d \theta / dt} = \frac{\ddot{\theta}}{\dot{\theta}} = \frac{a}{v}}

The rest is just number crunching. Code below:

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import math

R = 1.0   # Radius
m = 1.0   # Mass
u = 0.5   # Friction coefficient
g = 10.0  # Gravity

##################################################

t = 0.0            # Time
dt = 10.0**(-6.0)  # Time step

x = 0.0   # Tangential position
v = 0.5   # Tangential velocity
a = 0.0   # Tangential acceleration

while t <= 0.5:         

    x = x + v * dt    # Euler integration
    v = v + a * dt

    theta = x/R       # Angle

    N = (m/R)*(v**2.0) + m*g*math.sin(theta)  # Normal force

    F = m*g*math.cos(theta) - u*N  # Force in tangential direction

    a = F/m   # Tangential acceleration

    t = t + dt

##################################################

A = a/v
q1 = math.fabs(1000.0*A)
q2 = math.floor(q1)

print q2  # Answer is 1054

Karan Chatrath
May 26, 2019

I will lay out a few brief steps for the approach to this question. I encourage the solvers to post more detailed solutions.

Using the laws of motion, the equation of motion is: θ ¨ = 10 cos ( θ ) 5 sin ( θ ) θ ˙ 2 2 \ddot{\theta} = 10\cos(\theta) - 5\sin(\theta) - \frac{\dot{\theta}^2}{2}

Now comes the important step: d 2 θ d t 2 = d θ ˙ d t = d θ ˙ d θ d θ d t = d θ ˙ d θ θ ˙ \frac{d^2\theta}{dt^2} = \frac{d\dot{\theta}}{dt} = \frac{d\dot{\theta}}{d\theta}\frac{d\theta}{dt} = \frac{d\dot{\theta}}{d\theta} \dot{\theta}

Replacing this in the EOM, we get: d θ ˙ d θ θ ˙ = 10 cos ( θ ) 5 sin ( θ ) θ ˙ 2 2 \frac{d\dot{\theta}}{d\theta} \dot{\theta} = 10\cos(\theta) - 5\sin(\theta) - \frac{\dot{\theta}^2}{2}

This differential equation can be solved to obtain a closed form solution where θ ˙ \dot{\theta} is a function of θ \theta . Solving for θ \theta as a function of time would require numerical approaches. Recall that the initial conditions are:

θ ˙ ( 0 ) = 0.5 \dot{\theta}(0) = 0.5 and θ ( 0 ) = 0 \theta(0) = 0

Looking forward to seeing more elaborate solutions which demonstrate how to obtain the equation of motion and its solution.

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