Two-Stage Inflation as a Solution of the Initial Condition Problem of Hybrid Inflation
arXiv:hep-ph/9710526 · doi:10.1103/PhysRevD.59.083502
Abstract
We address the issue of fine-tuning of the initial field configuration that can lead to hybrid inflation in the context of global supersymmetry. This problem is generated by the difference between the energy scale at which the Universe emerges from the Planck era and the inflationary scale implied by the COBE observations: V^{1/4} \sim 10^{-3} m_{Pl}. We propose a scenario with two stages of inflation. The first stage, with a typical scale not far from m_{Pl}, occurs ``naturally'' and provides the necessary homogeneity for the second stage. The latter generates the density perturbations that result in the cosmic microwave background anisotropy observed by COBE.
12 pages, LaTeX, uses equation.sty, 4 figures in eps format
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Cited by in corpus (22)
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- Double inflation in supergravity and the primordial black hole formation
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- Basics of inflationary cosmology
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- Supersymmetry breaking and loop corrections at the end of inflation
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- Large Field Inflation in Supergravity
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