A First Principles Warm Inflation Model that Solves the Cosmological Horizon/Flatness Problems
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A quantum field theory warm inflation model is presented that solves the horizon/flatness problems. The model obtains, from the elementary dynamics of particle physics, cosmological scale factor trajectories that begin in a radiation dominated regime, enter an inflationary regime and then smoothly exit back into a radiation dominated regime, with nonnegligible radiation throughout the evolution.
In Press Physical Review Letters 1999, 5 pgs, 1 fig., latex
In Press Physical Review Letters 1999, 5 pgs, 1 fig., latex