Abundance of primordial black holes with local non-Gaussianity in peak theory
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Publication:5861840
DOI10.1088/1475-7516/2019/09/033OpenAlexW2973988606MaRDI QIDQ5861840
Chul-Moon Yoo, Shuichiro Yokoyama, Jinn-Ouk Gong
Publication date: 2 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1906.06790
Related Items (21)
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Cites Work
- Primordial black hole formation in the early universe: critical behaviour and self-similarity
- Curvature profiles as initial conditions for primordial black hole formation
- Primordial black holes—perspectives in gravitational wave astronomy
- Computations of primordial black-hole formation
- Primordial black holes from inflation and non-Gaussianity
- Quantum diffusion beyond slow-roll: implications for primordial black-hole production
- The ineludible non-Gaussianity of the primordial black hole abundance
- Primordial black hole abundance from random Gaussian curvature perturbations and a local density threshold
- 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
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