The Beauty of Collisions and Rotations
Imagine a pristine, horizontal frictionless surface. A uniform bar is resting peacefully, pivoted at one of its ends.
Suddenly, a small mass comes hurtling towards it, moving perpendicular to the bar. This isn't just a simple collision; it's a beautiful interplay of linear motion transforming into rotational motion.
When the mass strikes the bar exactly at its midpoint, it transfers energy and momentum. But because the bar is pinned at one end, it can't just slide away. It must rotate.
This problem is a classic test of your understanding of Conservation of Angular Momentum and the kinematics of Elastic Collisions. Let's break it down step by step.
Analyzing the Setup
Before we dive into the equations, let's establish our physical parameters. We have a bar of mass M=1.00 kg and length L=0.20 m.
The small mass m=0.10 kg approaches with an initial speed u=5.00 m/s. It strikes the bar at a distance of L/2 from the pivot.
After the collision, the particle bounces back with a speed v, and the bar begins to swing with an angular velocity ω.
Our goal is to find the exact values of ω and v. To do this, we need two independent equations.
The Master Equation
Angular Momentum
Why can't we use linear momentum conservation here? The answer lies at the pivot.
During the impact, the pivot exerts a massive, unknown impulsive force on the rod to keep it anchored. This external force destroys the conservation of linear momentum for the system.
However, if we calculate the torque about the pivot point itself, the lever arm for this pivot force is zero. Thus, the net external torque about the pivot is zero.
This is our golden ticket: Angular momentum about the pivot is conserved.
Let's write down the initial angular momentum. It's entirely due to the incoming particle:
After the collision, the particle bounces back, so its angular momentum reverses direction. The rod also gains angular momentum as it rotates:
Equating the two gives us our master equation:
Calculating the Moment of Inertia
Before we plug in the numbers, we need the moment of inertia I of the rod.
Since the rod is rotating about its end, we use the standard formula:
Substituting the given values M=1.00 kg and L=0.20 m:
I=31.00×(0.20)2=30.04 kg m2
Now, let's substitute everything into our angular momentum equation:
0.10×5.00×0.10=−0.10×v×0.10+30.04ω
Simplifying this yields:
Multiplying the entire equation by 100 to clear the decimals:
And multiplying by 3 gives us a clean, linear equation:
This is our first crucial relationship between v and ω.
The Geometry of the Bounce
Coefficient of Restitution
We have two unknowns, so we need a second equation. The problem states that the collision is elastic.
This means kinetic energy is conserved, but using the energy equation leads to messy quadratics. Instead, we use the Coefficient of Restitution (e), which is exactly 1 for an elastic collision.
The restitution equation relates the relative velocities before and after the impact:
e=vapproachvseparation=1
The velocity of approach is simply the initial speed of the particle, u=5.00 m/s.
The velocity of separation requires careful thought. After the hit, the point on the rod at L/2 moves forward with a tangential speed of ω(L/2).
Simultaneously, the particle bounces backward with speed v. Since they are moving in opposite directions, their relative speed of separation is the sum of their individual speeds:
vseparation=ω2L−(−v)=ω2L+v
Setting up the restitution equation:
Rearranging for v, we get our second equation:
Final Calculation
Bringing It All Together
We now have a simple system of two linear equations. Let's substitute the expression for v into our first equation:
Expanding the bracket:
Moving the constants to one side:
Solving for ω:
Rounding to three significant figures, we get ω=6.98 rad/s.
Finally, let's find the rebound speed v by plugging ω back into our second equation:
v=5.00−0.69767≈4.3023 m/s
Rounding again, we get v=4.30 m/s.
And there we have it! The physics perfectly predicts the aftermath of the collision, matching option (A).