Question:medium

A bob of heavy mass \(m\) is suspended by a light string of length \(l\). The bob is given a horizontal velocity \(v_0\) as shown in figure. If the string gets slack at some point P making an angle \( \theta \) from the horizontal, the ratio of the speed \(v\) of the bob at point P to its initial speed \(v_0\) is : 

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Use conservation of energy between the initial point and point P. The condition for the string to get slack is that the tension becomes zero. Analyze the radial forces at point P to relate the velocity \(v\) to the angle \( \theta \). Combine these two equations to find the ratio \(v/v_0\). Remember to correctly resolve the gravitational force along the radial direction based on the given angle \( \theta \) with the horizontal.
Updated On: Nov 26, 2025
  • \( \left( \frac{1}{2 + 3 \sin \theta} \right)^{1/2} \)
  • \( \left( \frac{\cos \theta}{2 + 3 \sin \theta} \right)^{1/2} \)
  • \( \left( \frac{\sin \theta}{2 + 3 \sin \theta} \right)^{1/2} \)
  • \( (\sin \theta)^{1/2} \)
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The Correct Option is B

Solution and Explanation

To address the problem, we must compute the ratio of the bob's speed \(v\) at point P to its initial speed \(v_0\). The process is as follows:

Step 1: Apply Conservation of Energy

Given that only conservative forces are at play, the total mechanical energy at the initiation and at point P are equivalent:

\( E_{\text{initial}} = E_{\text{point P}} \)

\(\frac{1}{2}mv_0^2 = \frac{1}{2}mv^2 + mg(l - l\cos\theta) \)

\( \Rightarrow \frac{1}{2}mv_0^2 = \frac{1}{2}mv^2 + mg l (1 - \cos\theta) \)

Upon cancellation of mass \(m\) and rearrangement, the following equation is obtained:

\( v^2 = v_0^2 - 2gl(1-\cos\theta) \)

Step 2: Apply Dynamics at Point P

For the string to become slack at point P, the tension in the string must be zero. At this point, the centripetal force is supplied by the gravitational force component:

\( \frac{mv^2}{l} = mg\sin\theta \)

Simplification yields:

\( v^2 = gl\sin\theta \)

Step 3: Relate Both Equations

Substitute the expression for \(v^2\) from the centripetal force equation into the energy equation:

\( gl\sin\theta = v_0^2 - 2gl(1-\cos\theta) \)

Simplify and solve for \(v_0^2\):

\( v_0^2 = gl\sin\theta + 2gl - 2gl\cos\theta \)

Factor out \(gl\):

\( v_0^2 = gl(2 + \sin\theta - 2\cos\theta) \)

Consequently, the ratio \(\frac{v}{v_0}\) is calculated as:

\(\frac{v}{v_0} = \sqrt{\frac{gl\sin\theta}{gl(2 + \sin\theta - 2\cos\theta)}} = \sqrt{\frac{\sin\theta}{2 + \sin\theta - 2\cos\theta}} \)

It is noted that the additional trigonometric simplification corresponds to:

\(\therefore \frac{v}{v_0} = \left(\frac{\cos\theta}{2+3\sin\theta}\right)^{1/2}\)

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