Inflation in random Gaussian landscapes

被引:20
|
作者
Masoumi, Ali [1 ]
Vilenkin, Alexander [1 ]
Yamada, Masaki [1 ,2 ]
机构
[1] Tufts Univ, Dept Phys & Astron, Inst Cosmol, Medford, MA 02155 USA
[2] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan
基金
美国国家科学基金会;
关键词
inflation; initial conditions and eternal universe;
D O I
10.1088/1475-7516/2017/05/053
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We develop analytic and numerical techniques for studying the statistics of slow-roll inflation in random Gaussian landscapes. As an illustration of these techniques, we analyze small-field inflation in a one-dimensional landscape. We calculate the probability distributions for the maximal number of e-folds and for the spectral index of density fluctuations n(s) and its running alpha(s). These distributions have a universal form, insensitive to the correlation function of the Gaussian ensemble. We outline possible extensions of our methods to a large number of fields and to models of large-field inflation. These methods do not suffer from potential inconsistencies inherent in the Brownian motion technique, which has been used in most of the earlier treatments.
引用
收藏
页数:25
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