The discussion centers on the comparison of energy density in modern particle accelerators to that of the early universe post-Big Bang. It highlights that while energy density and temperature are related, they are not the same; energy density refers to the number of particles per volume, while temperature indicates energy per particle. The conversation references a phase diagram that illustrates the conditions of the early universe and experimental results. Proton-proton collisions can achieve higher energy levels but do not reach thermal equilibrium, complicating the definitions of temperature and density. Ultimately, the distinction between energy per particle and energy density is clarified, emphasizing their different roles in physics.