The Beauty of Blended Motion
This problem is a masterpiece of classical mechanics, seamlessly blending two fundamental concepts: vertical circular motion and projectile motion. When a particle is given an initial velocity at the bottom of a suspended string, its fate depends entirely on that initial kinetic energy. If the energy is too low, it oscillates. If it's very high, it completes the circle. But in this specific scenario, the energy is just enough to carry it above the horizontal, but not enough to reach the top.
This causes the string to slack, and the particle transitions from a constrained circular path into a free-falling parabolic trajectory. Let's break down this beautiful transition step by step.
Phase 1
The Circular Journey
Let the particle start at the lowest point P with an initial velocity u. It travels in a circular arc of radius L. As it climbs, it loses kinetic energy and gains gravitational potential energy. At some point Q, located at an angle θ above the horizontal, the tension in the string drops exactly to zero.
At this critical instant, the string slacks. The only force providing the necessary centripetal acceleration is the component of gravity acting along the radial direction. We can write the dynamic equation as:
This simplifies to a direct relationship between the velocity at Q and the angle θ:
Simultaneously, we must respect the Conservation of Mechanical Energy. The particle has climbed a total vertical height of h=L+Lsinθ from its starting point. Applying the work-energy theorem between P and Q:
21mu2=21mv2+mgL(1+sinθ)
Rearranging this gives us our master energy equation:
Phase 2
The Parabolic Arc
Once the string slacks at Q, the particle is no longer constrained by the string. It becomes a projectile launched with velocity v. Since the string was at an angle θ to the horizontal, the velocity vector (which is tangential to the circle) is launched at an angle of 90∘−θ to the horizontal.
The problem provides a crucial geometric constraint: the particle crosses the vertical line AB (located at x=L/8) with a horizontal velocity. In projectile motion, the velocity is purely horizontal only at the highest point (the vertex) of the parabolic trajectory.
This means the horizontal distance from the launch point Q to the line AB is exactly half the range of the projectile.
Let's calculate this geometric distance. The x-coordinate of Q is Lcosθ, and the x-coordinate of the line AB is L/8. Therefore, the horizontal distance traveled is:
Now, we use the standard formula for the range of a projectile. Since the launch angle is 90∘−θ, the range is gv2sin(2(90∘−θ))=gv2sin(180∘−2θ)=gv2sin(2θ). Equating our geometric distance to half the range:
The Mathematical Resolution
We now have a system of equations. We can elegantly eliminate v2 by substituting v2=gLsinθ from our centripetal equation into the range equation:
Lcosθ−8L=2g(gLsinθ)(2sinθcosθ)
Canceling g and L, and simplifying the right side:
Using the identity sin2θ=1−cos2θ, we get:
The cosθ terms cancel out beautifully, leaving:
Taking the cube root yields cosθ=21, which means the string slacks exactly at θ=60∘ above the horizontal!
Final Calculation
With θ=60∘ unlocked, the rest of the problem collapses easily. First, we find the velocity squared at Q:
Finally, we substitute v2 and θ back into our master energy equation to find the initial velocity u:
Taking the square root gives us our final, elegant answer: