Highly non-Gaussian tails and primordial black holes from single-field inflation
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Publication:5878858
DOI10.1088/1475-7516/2022/12/034OpenAlexW4312226339MaRDI QIDQ5878858
Misao Sasaki, Zihan Zhou, Dong-Gang Wang, Yi-Fu Cai, Xiao-Han Ma
Publication date: 23 February 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2207.11910
Related Items (6)
Enhance primordial black hole abundance through the non-linear processes around bounce point ⋮ Tail diversity from inflation ⋮ Primordial black holes and stochastic inflation beyond slow roll. Part I. Noise matrix elements ⋮ Highly asymmetric probability distribution from a finite-width upward step during inflation ⋮ Primordial black holes and gravitational waves induced by exponential-tailed perturbations ⋮ Uphill inflation
Cites Work
- One small step for an inflaton, one giant leap for inflation: \textit{a novel non-Gaussian tail and primordial black holes}
- The hand-made tail: non-perturbative tails from multifield inflation
- A note on the abundance of primordial black holes: use and misuse of the metric curvature perturbation
- Creation of Wormholes by First Order Phase Transition of a Vacuum in the Early Universe
- Primordial black holes—perspectives in gravitational wave astronomy
- Quantum diffusion during inflation and primordial black holes
- Primordial black hole formation by vacuum bubbles
- Primordial black holes from inflation and non-Gaussianity
- Primordial black holes from inflation and quantum diffusion
- Revisiting non-Gaussianity from non-attractor inflation models
- A generalized non-Gaussian consistency relation for single field inflation
- Matter bounce cosmology with a generalized single field: non-Gaussianity and an extended no-go theorem
- Stochastic inflation beyond slow roll
- On primordial black holes from rapid turns in two-field models
- Beyond perturbation theory in inflation
- Numerical simulations of stochastic inflation using importance sampling
- Gravitational waves from resonant amplification of curvature perturbations during inflation
- Statistics of coarse-grained cosmological fields in stochastic inflation
- Amplification of primordial perturbations from the rise or fall of the inflaton
- Primordial black holes dark matter from inflection point models of inflation and the effects of reheating
- The exponential tail of inflationary fluctuations: consequences for primordial black holes
- On the slope of the curvature power spectrum in non-attractor inflation
- PBH in single field inflation: the effect of shape dispersion and non-Gaussianities
- Non-gaussianities for primordial black hole formation
- Non-Gaussianity in inflationary scenarios for primordial black holes
- Quantum diffusion in sharp transition to non-slow-roll phase
- Revisiting non-Gaussianity in non-attractor inflation models in the light of the cosmological soft theorem
- A general proof of the conservation of the curvature perturbation
- Primordial black hole formation with non-Gaussian curvature perturbations
- Ultra-slow-roll inflation with quantum diffusion
- Stochastic ultra slow roll inflation
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