Advances in Astronomy

Review Article

Non-Gaussianity from Particle Production during Inflation

Table 2

Constraints on the standard β€œvanilla” cosmological parameters for the single-bump model. All errors are 95.4% confidence level.
Ξ© 𝑏 β„Ž 2 0 . 0 2 2 7 + 0 . 0 0 1 0 βˆ’ 0 . 0 0 1 0
Ξ© 𝑐 β„Ž 2 0 . 1 1 2 2 + 0 . 0 0 5 0 βˆ’ 0 . 0 0 4 4
πœƒ 1 . 0 4 2 4 + 0 . 0 0 4 2 βˆ’ 0 . 0 0 4 3
𝜏 0 . 0 8 + 0 . 0 3 βˆ’ 0 . 0 3
𝑛 𝑠 0 . 9 5 6 + 0 . 0 2 4 βˆ’ 0 . 0 2 4
l n [ 1 0 1 0 𝐴 𝑠 ] 3 . 2 0 6 + 0 . 0 7 4 βˆ’ 0 . 0 6 8
𝐴 𝑆 𝑍 1 . 6 2 + 0 . 7 6 βˆ’ 0 . 7 4
Ξ© π‘š 0 . 2 6 4 + 0 . 0 2 6 βˆ’ 0 . 0 2 2
𝜎 8 0 . 8 0 7 + 0 . 0 3 4 βˆ’ 0 . 0 3 0
𝑧 π‘Ÿ 𝑒 1 0 . 5 + 2 . 5 βˆ’ 2 . 7
𝐻 0 7 1 . 6 + 2 . 3 βˆ’ 2 . 4