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- W4310374865 abstract "We present a non-perturbative method for calculating the abundance of primordial black holes given an arbitrary one-point probability distribution function for the primordial curvature perturbation, $P(zeta)$. A non-perturbative method is essential when considering non-Gaussianities that cannot be treated using a conventional perturbative expansion. To determine the full statistics of the density field, we relate $zeta$ to a Gaussian field by equating the cumulative distribution functions. We consider two examples: a specific local-type non-Gaussian distribution arising from ultra slow roll models, and a general piecewise model for $P(zeta)$ with an exponential tail. We demonstrate that the enhancement of primordial black hole formation is due to the intermediate regime, rather than the far tail. We also show that non-Gaussianity can have a significant impact on the shape of the primordial black hole mass distribution." @default.
- W4310374865 created "2022-12-10" @default.
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- W4310374865 date "2023-05-01" @default.
- W4310374865 modified "2023-10-18" @default.
- W4310374865 title "Non-perturbative non-Gaussianity and primordial black holes" @default.
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- W4310374865 doi "https://doi.org/10.1209/0295-5075/acd417" @default.
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