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arxiv: hep-ph/9804453 · v4 · submitted 1998-04-30 · ✦ hep-ph · astro-ph· gr-qc· hep-th

Inflationary Reheating in Grand Unified Theories

classification ✦ hep-ph astro-phgr-qchep-th
keywords reheatingtheoriesgrandnon-thermalunifiedanswercaseschaotic
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Grand unified theories may display multiply interacting fields with strong coupling dynamics. This poses two new problems: (1) What is the nature of chaotic reheating after inflation, and (2) How is reheating sensitive to the mass spectrum of these theories ? We answer these questions in two interesting limiting cases and demonstrate an increased efficiency of reheating which strongly enhances non-thermal topological defect formation, including monopoles and domain walls. Nevertheless, the large fluctuations may resolve this monopole problem via a modified Dvali-Liu-Vachaspati mechanism in which non-thermal destabilsation of discrete symmetries occurs at reheating.

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