CONSTRAINTS ON THE THREE-FLUID MODEL OF CURVATON DECAY

被引:2
|
作者
Multamaki, T. [1 ]
Sainio, J. [1 ]
Vilja, I. [1 ]
机构
[1] Univ Turku, Dept Phys & Astron, FIN-20014 Turku, Finland
来源
基金
芬兰科学院;
关键词
Curvaton; reheating; cosmological perturbations; DOUBLE INFLATION; PERTURBATIONS;
D O I
10.1142/S0218271809015801
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A three-fluid system describing the decay of the curvaton is studied by numerical and analytical means. We place constraints on the allowed interaction strengths between the fluids and initial curvaton density by requiring that the curvaton should decay before nucleosynthesis while nucleosynthesis, radiation-matter equality and decoupling occur at correct temperatures. We find that with a continuous, time-independent interaction, a small initial curvaton density is naturally preferred along with a low reheating temperature. Allowing for a time-dependent interaction, this constraint can be relaxed. In both cases, a purely adiabatic final state can be generated, but not without fine-tuning. Unlike in the two-fluid system, the time-dependent interactions are found to have a small effect on the curvature perturbation itself, due to the different nature of the system.
引用
收藏
页码:2047 / 2059
页数:13
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