Abundance of primordial black holes in peak theory for an arbitrary power spectrum

DOI10.1093/ptep/ptaa155OpenAlexW3093639803MaRDI QIDQ5158140

Tomohiro Harada, Chul-Moon Yoo, Kazunori Kohri, Shin'ichi Hirano

Publication date: 21 October 2021

Published in: Progress of Theoretical and Experimental Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2008.02425

Mathematics Subject Classification ID

Astronomy and astrophysics (85-XX) Relativity and gravitational theory (83-XX)

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The inflaton that could: primordial black holes and second order gravitational waves from tachyonic instability induced in Higgs-R²inflation ⋮ Primordial black holes in peak theory with a non-Gaussian tail ⋮ Statistics of coarse-grained cosmological fields in stochastic inflation ⋮ 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 ⋮ Implications of stochastic effects for primordial black hole production in ultra-slow-roll inflation ⋮ Peaks and primordial black holes: the effect of non-Gaussianity ⋮ Primordial black holes and gravitational waves induced by exponential-tailed perturbations ⋮ Reconstruction of primordial power spectrum of curvature perturbation from the merger rate of primordial black hole binaries ⋮ The power spectrum on small scales: robust constraints and comparing PBH methodologies

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