Setting L to zero in the effective potential energy equation indicates zero angular momentum, leading to a scenario of radial infall. This situation can be analyzed in both Newtonian and general relativity contexts. In Newtonian physics, the Kepler problem provides a foundational understanding, allowing for analytical solutions. Understanding this framework simplifies the transition to general relativity, particularly in the context of a test particle in Schwarzschild spacetime. A thorough study of these concepts is essential for grasping the implications of L=0.