Failure of the stochastic approach to inflation beyond slow-roll

被引:55
作者
Cruces, Diego [1 ]
Germani, Cristiano [1 ,2 ]
Prokopec, Tomislav [3 ,4 ]
机构
[1] Univ Barcelona, Inst Ciencies Cosmos ICCUB, Marti i Franques 1, E-08028 Barcelona, Spain
[2] Univ Barcelona, Dept Fis Quant & Astrofis, Marti i Franques 1, E-08028 Barcelona, Spain
[3] Univ Utrecht, Inst Theoret Phys, Spinoza Inst, Postbus 80-195, NL-3508 TD Utrecht, Netherlands
[4] Univ Utrecht, EMMEO, Postbus 80-195, NL-3508 TD Utrecht, Netherlands
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2019年 / 03期
关键词
cosmological perturbation theory; inflation; primordial black holes; FLUCTUATIONS;
D O I
10.1088/1475-7516/2019/03/048
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
After giving a pedagogical review we clarify that the stochastic approach to inflation is generically reliable only at zeroth order in the (geometrical) slow-roll parameter epsilon(l) if and only if epsilon(2)(2) << 6/epsilon(1), with the notable exception of slow-roll. This is due to the failure of the stochastic Delta N formalism in its standard formulation. However, by keeping the formalism in its regime of validity, we showed that, in ultra-slow-roll, the stochastic approach to inflation reproduces the power spectrum calculated from the linear theory approach.
引用
收藏
页数:16
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