Non-Gaussianity in inflationary scenarios for primordial black holes

DOI10.1088/1475-7516/2022/06/019zbMath1505.83026arXiv2110.08189OpenAlexW3204982142MaRDI QIDQ5099329

Pedro Carrilho, David J. Mulryne, Matthew W. Davies

Publication date: 31 August 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2110.08189

zbMATH Keywords

inflationnon-Gaussianityprimordial black holes

Mathematics Subject Classification ID

Black holes (83C57) Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Set functions and measures and integrals in infinite-dimensional spaces (Wiener measure, Gaussian measure, etc.) (28C20)

Related Items (4)

Multi-field inflation with large scalar fluctuations: non-Gaussianity and perturbativity ⋮ Highly asymmetric probability distribution from a finite-width upward step during inflation ⋮ Scalar induced gravitational waves from Chern-Simons gravity during inflation era ⋮ Highly non-Gaussian tails and primordial black holes from single-field inflation

Cites Work

• Gravitational waves induced by the local-type non-Gaussian curvature perturbations
• Primordial black holes from inflation and non-Gaussianity
• Revisiting non-Gaussianity from non-attractor inflation models
• The ineludible non-Gaussianity of the primordial black hole abundance
• Probing non-Gaussianities with the high frequency tail of induced gravitational waves
• Non-Gaussianity and the induced gravitational wave background
• On the slope of the curvature power spectrum in non-attractor inflation
• Non-gaussianities for primordial black hole formation

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