Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2003-12-04
Class.Quant.Grav. 21 (2004) L11-L16
Physics
High Energy Physics
High Energy Physics - Phenomenology
9pages, no figure, references added, final version
Scientific paper
10.1088/0264-9381/21/4/L02
Recent arguments show that some curvaton field may generate the cosmological curvature perturbation. As the curvaton is independent of the inflaton field, there is a hope that the fine-tunings of inflation models can be cured by the curvaton scenario. More recently, however, D.H.Lyth discussed that there is a strong bound for the Hubble parameter during inflation even if one assumes the curvaton scenario. Although the most serious constraint was evaded, the bound seems rather crucial for many models of a low inflation scale. In this paper we try to remove this constraint. We show that the bound is drastically modified if there were multiple stages of inflation.
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