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A body of mass m moving with a constant velocity collides head on with another stationary body of same mass if the coefficient of restitution between the bodies is `(1)/(2)` then ratio of velocities of two bodies after collision with be

A

`(1)/(3)`

B

`(1)/(2)`

C

`(1)/(4)`

D

`1`

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To solve the problem of finding the ratio of velocities of two bodies after a collision, we can follow these steps: ### Step 1: Understand the Problem We have two bodies of equal mass \( m \). One body is moving with a velocity \( v \) and the other is stationary. After the collision, we need to find the velocities \( v_1 \) and \( v_2 \) of the two bodies, and then determine the ratio \( \frac{v_1}{v_2} \). ### Step 2: Apply Conservation of Momentum The law of conservation of momentum states that the total momentum before the collision is equal to the total momentum after the collision. Before the collision: - Momentum of the first body = \( mv \) - Momentum of the second body = \( 0 \) Total initial momentum \( P_{initial} = mv + 0 = mv \) After the collision: - Momentum of the first body = \( mv_1 \) - Momentum of the second body = \( mv_2 \) Total final momentum \( P_{final} = mv_1 + mv_2 \) Setting these equal gives us: \[ mv = mv_1 + mv_2 \] Dividing through by \( m \) (assuming \( m \neq 0 \)): \[ v = v_1 + v_2 \quad \text{(Equation 1)} \] ### Step 3: Apply the Coefficient of Restitution The coefficient of restitution \( e \) is defined as the ratio of the relative velocity of separation to the relative velocity of approach. Given \( e = \frac{1}{2} \), we can write: \[ e = \frac{v_2 - v_1}{v - 0} \] Substituting the value of \( e \): \[ \frac{1}{2} = \frac{v_2 - v_1}{v} \] Cross-multiplying gives: \[ v_2 - v_1 = \frac{v}{2} \quad \text{(Equation 2)} \] ### Step 4: Solve the Equations Now we have two equations: 1. \( v = v_1 + v_2 \) (Equation 1) 2. \( v_2 - v_1 = \frac{v}{2} \) (Equation 2) From Equation 2, we can express \( v_2 \) in terms of \( v_1 \): \[ v_2 = v_1 + \frac{v}{2} \] Substituting \( v_2 \) into Equation 1: \[ v = v_1 + \left(v_1 + \frac{v}{2}\right) \] Simplifying this gives: \[ v = 2v_1 + \frac{v}{2} \] Rearranging: \[ 2v_1 = v - \frac{v}{2} = \frac{v}{2} \] Thus: \[ v_1 = \frac{v}{4} \] Now substituting \( v_1 \) back into Equation 2 to find \( v_2 \): \[ v_2 = v_1 + \frac{v}{2} = \frac{v}{4} + \frac{v}{2} = \frac{v}{4} + \frac{2v}{4} = \frac{3v}{4} \] ### Step 5: Find the Ratio of Velocities Now we have: - \( v_1 = \frac{v}{4} \) - \( v_2 = \frac{3v}{4} \) The ratio \( \frac{v_1}{v_2} \) is: \[ \frac{v_1}{v_2} = \frac{\frac{v}{4}}{\frac{3v}{4}} = \frac{1}{3} \] ### Conclusion The ratio of the velocities of the two bodies after the collision is \( \frac{1}{3} \).
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