A First Principles Warm Inflation Model that Solves the Cosmological Horizon/Flatness Problems

Details A First Principles Warm Inflation Model that Solves the Cosmological Horizon/Flatness Problems A First Principles Warm Inflation Model that Solves the Cosmological Horizon/Flatness Problems

1998-09-29

arxiv.org/abs/hep-ph/9809583v3

Phys.Rev.Lett.83:264-267,1999

Physics

High Energy Physics

High Energy Physics - Phenomenology

In Press Physical Review Letters 1999, 5 pgs, 1 fig., latex

Scientific paper

10.1103/PhysRevLett.83.264

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.

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