Window function dependence of the novel mass function of primordial black holes

DOI10.1088/1475-7516/2020/12/038zbMath1484.83073arXiv2005.07153OpenAlexW3117432123MaRDI QIDQ5027102

Keisuke Inomata, Koki Tokeshi, Jun'ichi Yokoyama

Publication date: 3 February 2022

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

Full work available at URL: https://arxiv.org/abs/2005.07153

zbMATH Keywords

inflationprimordial black holes

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Reasoning under uncertainty in the context of artificial intelligence (68T37) Geometrodynamics and the holographic principle (83E05)

Related Items (4)

Statistics of coarse-grained cosmological fields in stochastic inflation ⋮ Amplification of primordial perturbations from the rise or fall of the inflaton ⋮ Implications of stochastic effects for primordial black hole production in ultra-slow-roll inflation ⋮ Effects of the modification of gravity on the production of primordial black holes

Cites Work

• On the primordial black hole mass function for broad spectra
• Primordial Black Holes as Dark Matter and Generators of Cosmic Structure
• Primordial black holes—perspectives in gravitational wave astronomy
• The ineludible non-Gaussianity of the primordial black hole abundance
• From primordial black holes abundance to primordial curvature power spectrum (and back)
• Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation
• A novel formulation of the primordial black hole mass function
• Primordial black hole abundance from random Gaussian curvature perturbations and a local density threshold

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