The discussion centers on whether a black hole has a radius or if it is effectively zero, focusing on the distinction between the singularity and the event horizon. While classical General Relativity (GR) suggests a singularity with zero radius, the complexities of gravity at such extreme scales lead to uncertainties about the nature of mass and area. The conversation highlights the challenge of reconciling GR with Quantum Mechanics (QM), particularly at the singularity where traditional concepts of mass and area may not apply. Participants emphasize that assumptions based on classical mechanics do not hold true at quantum scales, complicating the understanding of black holes. Ultimately, the nature of mass and area in black holes remains a profound question in modern physics.