A. Berera et al., A first principles warm inflation model that solves the cosmological horizon and flatness problems, PHYS REV L, 83(2), 1999, pp. 264-267
A quantum field theory warm inflation model is presented that solves the ho
rizon and flatness problems. The model obtains, from the elementary dynamic
s of particle physics, cosmological scale factor trajectories that begin in
a radiation dominated regime, enter an inflationary regime, and then smoot
hly exit back into a radiation dominated regime, with non-negligible radiat
ion throughout the evolution.