Quantum Seesaw Cosmology: A Heating Phase from Pauli Blocking

In Seesaw Cosmology, a scalar field reheats the Standard Model (SM) through right-handed neutrinos (RHNs), which generate tiny neutrino masses through the seesaw mechanism. When RHNs rapidly fill a restricted momentum-space region, expansion continually opens new fermionic states that are refilled by subsequent scalar decays, maintaining an approximately constant physical RHN density. This gives rise to a novel heating regime in which the SM temperature increases with the scale factor as $T\propto a^{+3\mathrm{/}8}$, in sharp contrast to the conventional $T\propto a^{-3\mathrm{/}8}$ scaling during matter-dominated reheating.