Primordial black holes and gravitational waves induced by exponential-tailed perturbations
DOI10.1088/1475-7516/2023/05/044zbMath1528.83063arXiv2209.13891OpenAlexW4377990725MaRDI QIDQ6172967
Yuichiro Tada, Unnamed Author, Shuichiro Yokoyama, Katsuya T. Abe
Publication date: 20 July 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2209.13891
Unified quantum theories (81V22) Black holes (83C57) Signal detection and filtering (aspects of stochastic processes) (60G35) Geometrodynamics and the holographic principle (83E05) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Gravitational waves (83C35) Dark matter and dark energy (83C56)
Related Items (2)
Cites Work
- Rare events are nonperturbative: primordial black holes from heavy-tailed distributions
- One small step for an inflaton, one giant leap for inflation: \textit{a novel non-Gaussian tail and primordial black holes}
- Gravitational waves induced by the local-type non-Gaussian curvature perturbations
- The dynamics of primordial black-hole formation
- Gravitational-Wave Constraints on the Abundance of Primordial Black Holes
- THE GLOBAL STRUCTURE OF THE INFLATIONARY UNIVERSE
- Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond
- Quantum diffusion during inflation and primordial black holes
- A cosmological signature of the SM Higgs instability: gravitational waves
- Revisiting non-Gaussianity from non-attractor inflation models
- Analytical thresholds for black hole formation in general cosmological backgrounds
- Probing non-Gaussianities with the high frequency tail of induced gravitational waves
- Cosmology of strongly interacting fermions in the early universe
- Numerical simulations of stochastic inflation using importance sampling
- Non-Gaussianity and the induced gravitational wave background
- Primordial black holes in peak theory with a non-Gaussian tail
- Statistics of coarse-grained cosmological fields in stochastic inflation
- The exponential tail of inflationary fluctuations: consequences for primordial black holes
- PBH in single field inflation: the effect of shape dispersion and non-Gaussianities
- Gravitational waves from dark matter isocurvature
- Simulation of primordial black holes with large negative non-Gaussianity
- The third order scalar induced gravitational waves
- Implications of stochastic effects for primordial black hole production in ultra-slow-roll inflation
- Quantum diffusion in sharp transition to non-slow-roll phase
- Primordial black hole abundance from random Gaussian curvature perturbations and a local density threshold
- Abundance of primordial black holes in peak theory for an arbitrary power spectrum
- A general proof of the conservation of the curvature perturbation
- Primordial black hole formation in the radiative era: investigation of the critical nature of the collapse
- Abundance of primordial black holes with local non-Gaussianity in peak theory
- 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
- No-go theorem for scalar-trispectrum-induced gravitational waves
This page was built for publication: Primordial black holes and gravitational waves induced by exponential-tailed perturbations
