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- W2804070879 abstract "Primordial black-holes (PBH) can be produced in single-field models of inflation with a quasi-inflection point in the potential. In these models, a large production of PBHs requires a deviation from the slow-roll (SR) trajectory. In turn, this SR violation can produce an exponential growth of quantum fluctuations. We study the back-reaction of these quantum modes on the inflationary dynamics using stochastic inflation in the Hamilton-Jacobi formalism. We develop a methodology to solve quantum diffusion beyond SR in terms of the statistical moments of the probability distribution. We apply these techniques to a toy model potential with a quasi-inflection point. We find that there is an enhancement of the power spectrum due to the dominance of the stochastic noise in the phase beyond SR. Moreover, non-Gaussian corrections become as well relevant with a large positive kurtosis. Altogether, this produces a significant boost of PBH production. We discuss how our results extend to other single-field models with similar dynamics. We conclude that the abundance of PBHs in this class of models should be revisited including quantum diffusion." @default.
- W2804070879 created "2018-06-01" @default.
- W2804070879 creator A5011635269 @default.
- W2804070879 creator A5051228162 @default.
- W2804070879 date "2018-08-13" @default.
- W2804070879 modified "2023-10-18" @default.
- W2804070879 title "Quantum diffusion beyond slow-roll: implications for primordial black-hole production" @default.
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- W2804070879 doi "https://doi.org/10.1088/1475-7516/2018/08/018" @default.
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