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Particle A makes a perfectly elastic col...

Particle A makes a perfectly elastic collision with anther particle B at rest. They fly apart in opposite direction with equal speeds. If the masses are `m_(A)&m_(B)` respectively, then

A

`2m_(A)=m_(B)`

B

`3m_(A)=m_(B)`

C

`4m_(A)=m_(B)`

D

`sqrt3m_(A)=m_(B)`

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To solve the problem of a perfectly elastic collision between particle A and particle B, we can follow these steps: ### Step 1: Understand the Initial Conditions - Particle A has mass \( m_A \) and is moving with an initial velocity \( u \). - Particle B has mass \( m_B \) and is initially at rest (velocity = 0). ### Step 2: Apply the Concept of Elastic Collision In a perfectly elastic collision, both momentum and kinetic energy are conserved. The coefficient of restitution \( e \) for a perfectly elastic collision is equal to 1. ### Step 3: Write the Equation for Coefficient of Restitution The coefficient of restitution \( e \) is defined as: \[ e = \frac{\text{Velocity of separation}}{\text{Velocity of approach}} \] For our case: \[ 1 = \frac{v + v}{u} \] Where \( v \) is the speed of both particles A and B after the collision (they fly apart with equal speeds in opposite directions). ### Step 4: Simplify the Coefficient of Restitution Equation From the equation above, we can simplify: \[ 1 = \frac{2v}{u} \] This leads to: \[ 2v = u \quad \Rightarrow \quad v = \frac{u}{2} \] ### Step 5: Apply Conservation of Momentum The total momentum before and after the collision must be equal. Thus, we have: \[ \text{Initial Momentum} = \text{Final Momentum} \] Before the collision: \[ \text{Initial Momentum} = m_A \cdot u + m_B \cdot 0 = m_A \cdot u \] After the collision: \[ \text{Final Momentum} = -m_A \cdot v + m_B \cdot v \] Setting the initial momentum equal to the final momentum: \[ m_A \cdot u = -m_A \cdot v + m_B \cdot v \] ### Step 6: Substitute \( v \) in the Momentum Equation Substituting \( v = \frac{u}{2} \) into the momentum equation: \[ m_A \cdot u = -m_A \cdot \left(\frac{u}{2}\right) + m_B \cdot \left(\frac{u}{2}\right) \] This simplifies to: \[ m_A \cdot u = -\frac{m_A \cdot u}{2} + \frac{m_B \cdot u}{2} \] ### Step 7: Rearranging the Equation Multiply through by 2 to eliminate the fraction: \[ 2m_A \cdot u = -m_A \cdot u + m_B \cdot u \] Rearranging gives: \[ 2m_A \cdot u + m_A \cdot u = m_B \cdot u \] \[ 3m_A \cdot u = m_B \cdot u \] ### Step 8: Solve for the Mass Relationship Dividing both sides by \( u \) (assuming \( u \neq 0 \)): \[ 3m_A = m_B \] ### Conclusion Thus, the relationship between the masses of particles A and B is: \[ m_B = 3m_A \]
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