Highly asymmetric probability distribution from a finite-width upward step during inflation
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Publication:6121242
DOI10.1088/1475-7516/2023/11/021arXiv2305.18140OpenAlexW4388487790MaRDI QIDQ6121242
Unnamed Author, Tomohiro Fujita, Misao Sasaki
Publication date: 26 February 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2305.18140
Cites Work
- Superconformal inflationary \(\alpha\)-attractors
- Gauge-invariant second-order perturbations and non-Gaussianity from inflation
- One small step for an inflaton, one giant leap for inflation: \textit{a novel non-Gaussian tail and primordial black holes}
- A note on the abundance of primordial black holes: use and misuse of the metric curvature perturbation
- A new type of isotropic cosmological models without singularity
- Primordial black holes—perspectives in gravitational wave astronomy
- Quantum diffusion during inflation and primordial black holes
- Single field double inflation and primordial black holes
- Primordial black holes from inflation and non-Gaussianity
- Primordial black holes from inflation and quantum diffusion
- Revisiting non-Gaussianity from non-attractor inflation models
- The ineludible non-Gaussianity of the primordial black hole abundance
- Non-Gaussianity effects on the primordial black hole abundance for sharply-peaked primordial spectrum
- Primordial black holes in peak theory with a non-Gaussian tail
- Amplification of primordial perturbations from the rise or fall of the inflaton
- The exponential tail of inflationary fluctuations: consequences for primordial black holes
- Primordial black holes from a tiny bump/dip in the inflaton potential
- 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
- Inflationary universe: A possible solution to the horizon and flatness problems
- 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
- Highly non-Gaussian tails and primordial black holes from single-field inflation
- Questions on calculation of primordial power spectrum with large spikes: the resonance model case
- 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
- PBH formation in EFT of single field inflation with sharp transition
- One-loop corrections in power spectrum in single field inflation
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