Primordial black hole formation with non-Gaussian curvature perturbations

DOI10.1088/1475-7516/2019/09/073OpenAlexW2947928126MaRDI QIDQ5861874

Airam Marcos-Caballero, Vicente Atal, Jaume Garriga

Publication date: 2 March 2022

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

Full work available at URL: https://arxiv.org/abs/1905.13202

zbMATH Keywords

inflationcosmological perturbation theoryprimordial black holes

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (21)

Non-Gaussianity effects on the primordial black hole abundance for sharply-peaked primordial spectrum ⋮ Primordial black holes in peak theory with a non-Gaussian tail ⋮ Statistics of coarse-grained cosmological fields in stochastic inflation ⋮ Amplification of primordial perturbations from the rise or fall of the inflaton ⋮ Non-Gaussian formation of primordial black holes: effects on the threshold ⋮ Primordial black holes from broad spectra: abundance and clustering ⋮ Primordial black holes from a tiny bump/dip in the inflaton potential ⋮ PBH in single field inflation: the effect of shape dispersion and non-Gaussianities ⋮ Detuning primordial black hole dark matter with early matter domination and axion monodromy ⋮ Non-gaussianities for primordial black hole formation ⋮ Solving peak theory in the presence of local non-gaussianities ⋮ Simulation of primordial black holes with large negative non-Gaussianity ⋮ Peaks and primordial black holes: the effect of non-Gaussianity ⋮ Squeezed bispectrum and one-loop corrections in transient constant-roll inflation ⋮ Highly asymmetric probability distribution from a finite-width upward step during inflation ⋮ Primordial black holes and gravitational waves induced by exponential-tailed perturbations ⋮ Uphill inflation ⋮ Primordial non-Gaussianity f_NLand anisotropies in scalar-induced gravitational waves ⋮ Could PBHs and secondary GWs have originated from squeezed initial states? ⋮ Probing non-Gaussianities with the high frequency tail of induced gravitational waves ⋮ Highly non-Gaussian tails and primordial black holes from single-field inflation

Cites Work

• A new type of isotropic cosmological models without singularity
• Primordial black holes—perspectives in gravitational wave astronomy
• Quantum diffusion during inflation and primordial black holes
• Single field double inflation and primordial black holes
• Primordial black holes from inflation and non-Gaussianity
• Mechanisms for primordial black hole production in string theory
• A generalized non-Gaussian consistency relation for single field inflation
• Primordial black hole and wormhole formation by domain walls
• The ineludible non-Gaussianity of the primordial black hole abundance
• Primordial black hole abundance from random Gaussian curvature perturbations and a local density threshold
• Primordial black holes from α-attractors

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