Solving peak theory in the presence of local non-gaussianities

DOI10.1088/1475-7516/2021/08/060zbMath1492.83108arXiv2102.04084OpenAlexW3195322517MaRDI QIDQ5070254

Flavio Riccardi, Alfredo Urbano, Marco Taoso

Publication date: 11 April 2022

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

Full work available at URL: https://arxiv.org/abs/2102.04084

zbMATH Keywords

inflationprimordial black holesdark matter theory

Mathematics Subject Classification ID

Black holes (83C57) Geometrodynamics and the holographic principle (83E05) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Set functions and measures and integrals in infinite-dimensional spaces (Wiener measure, Gaussian measure, etc.) (28C20) Peak functions (32T40) Dark matter and dark energy (83C56)

Related Items (8)

Enhance primordial black hole abundance through the non-linear processes around bounce point ⋮ Non-Gaussianity effects on the primordial black hole abundance for sharply-peaked primordial spectrum ⋮ Non-Gaussianity and the induced gravitational wave background ⋮ Non-gaussianities for primordial black hole formation ⋮ Simulation of primordial black holes with large negative non-Gaussianity ⋮ Peaks and primordial black holes: the effect of non-Gaussianity ⋮ Dark photon stars: formation and role as dark matter substructure ⋮ Probing non-Gaussianities with the high frequency tail of induced gravitational waves

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