PBH formation in EFT of single field inflation with sharp transition

DOI10.1016/j.physletb.2023.138123arXiv2302.05655MaRDI QIDQ6055949

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Publication date: 29 September 2023

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2302.05655

Mathematics Subject Classification ID

Unified quantum theories (81V22) Black holes (83C57) Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Models and methods for concurrent and distributed computing (process algebras, bisimulation, transition nets, etc.) (68Q85) Loops, quasigroups (20N05) Causal inference from observational studies (62D20) Effective quantum field theories (81T12)

Related Items (12)

PBHs and GWs from 𝕋²-inflation and NANOGrav 15-year data ⋮ 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 ⋮ Multi-field inflation with large scalar fluctuations: non-Gaussianity and perturbativity ⋮ Primordial black holes and stochastic inflation beyond slow roll. Part I. Noise matrix elements ⋮ One-loop corrections in power spectrum in single field inflation ⋮ Gravitational capture of magnetic monopoles by primordial black holes in the early universe ⋮ Thermalization in quenched open quantum cosmology ⋮ Cancellation of quantum corrections on the soft curvature perturbations ⋮ The cosmological tree theorem ⋮ Highly asymmetric probability distribution from a finite-width upward step during inflation ⋮ Quantum loop effects on the power spectrum and constraints on primordial black holes

Cites Work

• Dynamical renormalization group approach to relaxation in quantum field theory.
• Loop corrections to standard model fields in inflation
• Dynamical constraints on RG flows and cosmology
• Primordial black holes—perspectives in gravitational wave astronomy
• The ineludible non-Gaussianity of the primordial black hole abundance
• Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation
• Primordial black holes from a tiny bump/dip in the inflaton potential
• Black hole explosions?
• Loop corrections in Minkowski spacetime away from equilibrium. I: Late-time resummations
• Loop corrections in Minkowski spacetime away from equilibrium. II: Finite-time results
• 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
• One-loop corrections in power spectrum in single field inflation

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