The discussion addresses the concept of temperature in relation to the Big Bang, questioning how the early universe could possess immense temperature without elementary particles. It clarifies that temperature is not solely linked to the kinetic energy of particles; rather, it is defined by the relationship between energy and entropy. The temperature of electromagnetic radiation, such as that observed in cosmic microwave background maps, demonstrates that temperature can exist independently of conventional matter. Additionally, it highlights that classical models fail as one approaches the moment of the Big Bang, necessitating the use of quantum cosmology to understand these conditions. This indicates a need for advanced theoretical frameworks to accurately describe the early universe's temperature.