Decoherence from isocurvature perturbations in inflation

被引:33
|
作者
Prokopec, Tomislav [1 ]
Rigopoulos, Gerasimos I. [1 ]
机构
[1] Univ Utrecht, Inst Theoret Phys, NL-3508 TD Utrecht, Netherlands
关键词
cosmological perturbation theory; inflation; physics of the early universe;
D O I
10.1088/1475-7516/2007/11/029
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the possible role of isocurvature perturbations for the quantum decoherence of the curvature perturbation during inflation. We point out that if the inflaton trajectory in field space is curved, the adiabatic mode is generically coupled to the isocurvature mode and thus tracing out the latter can cause the curvature perturbation to decohere. We explicitly investigate this suggestion in a model of inflation with two decoupled massive fields and find that decoherence is effective for a wide range of mass ratios. In particular, we calculate the entanglement entropy for this model and show that it grows after horizon exit, providing a quantitative measure for decoherence.
引用
收藏
页数:16
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