The discussion centers on the potential for a high-energy particle, like the OMG particle, to impact a neutron star and initiate the formation of a black hole. Participants argue that a single high-energy proton is unlikely to provide the necessary mass for this transformation, emphasizing that sufficient total mass is required rather than just energy density. The idea of a neutron star being on the brink of becoming a black hole is considered, but it is noted that neutron stars are constantly accumulating mass, making such a scenario improbable. Misconceptions about black holes "gobbling" matter are clarified, with the consensus that black holes do not actively consume surrounding material but rather attract it due to their gravitational pull. Ultimately, the conversation highlights the complexities of mass, density, and the conditions necessary for black hole formation.