Simulation of primordial black holes with large negative non-Gaussianity

DOI10.1088/1475-7516/2022/05/012zbMath1505.83016arXiv2202.01028OpenAlexW4229371985MaRDI QIDQ5099288

Shuichiro Yokoyama, Yuichiro Tada, Chul-Moon Yoo, Albert Escrivà

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/2202.01028

zbMATH Keywords

primordial black holesGR black holes

Mathematics Subject Classification ID

Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) 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) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (6)

Squeezed bispectrum and one-loop corrections in transient constant-roll inflation ⋮ Galileon inflation evades the no-go for PBH formation in the single-field framework ⋮ Primordial black holes and stochastic inflation beyond slow roll. Part I. Noise matrix elements ⋮ Primordial black holes and gravitational waves induced by exponential-tailed perturbations ⋮ Uphill inflation ⋮ Primordial non-Gaussianity f_NLand anisotropies in scalar-induced gravitational waves

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