A Cosmological Model Based on a Quadratic Equation of State Unifying Vacuum Energy, Radiation, and Dark Energy
Figure 6
Evolution of the temperature with the time in linear scales. The dashed line corresponds to the standard radiation model of Section 3.2 exhibiting a finite time singularity at . Quantum mechanics limits the rise of the temperature to about half the Planck value . In the vacuum energy era, the temperature drops to zero exponentially rapidly for .
