Review Article

Non-Gaussianity from Particle Production during Inflation

Table 3

Constraints on the standard β€œvanilla” cosmological parameters for the multiple-bump model. All error bars are 95.4% confidence level.

Ξ© 𝑏 β„Ž 2 0 . 0 2 2 7 + 0 . 0 0 0 9 βˆ’ 0 . 0 0 0 9

Ξ© 𝑐 β„Ž 2 0 . 1 1 2 6 + 0 . 0 0 4 9 βˆ’ 0 . 0 0 4 4
πœƒ 1 . 0 4 2 4 + 0 . 0 0 3 9 βˆ’ 0 . 0 0 4 3
𝜏 0 . 0 7 8 + 0 . 0 3 1 βˆ’ 0 . 0 2 6
𝑛 𝑠 0 . 9 3 + 0 . 0 4 βˆ’ 0 . 1 7
l n [ 1 0 1 0 𝐴 𝑠 ] 2 . 8 + 0 . 4 βˆ’ 0 . 9
𝐴 𝑆 𝑍 1 . 6 0 + 0 . 7 7 βˆ’ 0 . 7 6
Ξ© π‘š 0 . 2 6 5 + 0 . 0 2 6 βˆ’ 0 . 0 2 1
𝜎 8 0 . 8 0 7 + 0 . 0 3 4 βˆ’ 0 . 0 3 0
𝑧 π‘Ÿ 𝑒 1 0 . 3 + 2 . 6 βˆ’ 2 . 5
𝐻 0 7 1 . 4 + 2 . 2 βˆ’ 2 . 4