Preheating after modular inflation

被引:36
作者
Barnaby, Neil [1 ]
Bond, J. Richard [1 ]
Huang, Zhiqi [1 ]
Kofman, Lev [1 ]
机构
[1] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
string theory and cosmology; physics of the early universe; NATURAL INFLATION;
D O I
10.1088/1475-7516/2009/12/021
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study (p) reheating in modular (closed string) inflationary scenarios, with a special emphasis on Kahler moduli/Roulette models. It is usually assumed that reheating in such models occurs through perturbative decays. However, we find that there are very strong non-perturbative preheating decay channels related to the particular shape of the inflaton potential (which is highly nonlinear and has a very steep minimum). Preheating after modular inflation, proceeding through a combination of tachyonic instability and broad-band parametric resonance, is perhaps the most violent example of preheating after inflation known in the literature. Further, we consider the subsequent transfer of energy to the standard model sector in scenarios where the standard model particles are confined to a D7-brane wrapping the inflationary blow-up cycle of the compactification manifold or, more interestingly, a non-inflationary blow-up cycle. We explicitly identify the decay channels of the inflaton in these two scenarios. We also consider the case where the inflationary cycle shrinks to the string scale at the end of inflation; here a field theoretical treatment of reheating is insufficient and one must turn instead to a stringy description. We estimate the decay rate of the inflaton and the reheat temperature for various scenarios.
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页数:31
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