The discussion centers on the concept of energy in the expanding universe, questioning whether the internal energy (U) is decreasing as work (W) increases while total energy (Q) remains constant. It highlights that the total energy of the universe is not well-defined, as it depends on coordinate choices and is not necessarily conserved. An integral called PQ, defined as energy density multiplied by volume, is introduced but noted to not represent the universe's true energy. In standard isotropic cosmologies, PQ is conserved in "dust" universes but not in those with pressure, which applies to our current matter-dominated universe. The conversation references MTW for further insights, emphasizing that PQ should not be mistaken for the universe's energy.