Formation of primordial black holes from warm inflation
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Publication:5070954
DOI10.1088/1475-7516/2020/09/042zbMath1493.83012arXiv1910.05238OpenAlexW3105254649MaRDI QIDQ5070954
Publication date: 14 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1910.05238
Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Classical and relativistic thermodynamics (80A10) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Dark matter and dark energy (83C56)
Related Items (6)
Gravity waves and primordial black holes in scalar warm little inflation ⋮ Galileon inflation evades the no-go for PBH formation in the single-field framework ⋮ Quantum loop effects on the power spectrum and constraints on primordial black holes ⋮ Primordial black-hole dark matter via warm natural inflation ⋮ Feasibility of primordial black hole Remnants as dark matter in view of Hawking radiation recoil ⋮ Primordial black holes and gravitational waves from dissipation during inflation
Cites Work
- Particle creation by black holes
- The importance of being warm (during inflation)
- Towards a reliable effective field theory of inflation
- Gravitino production by primordial black hole evaporation and constraints on the inhomogeneity of the early universe
- Pregalactic black hole accretion and the thermal history of the Universe
- Primordial black holes—perspectives in gravitational wave astronomy
- Primordial black holes from thermal inflation
- From primordial black holes abundance to primordial curvature power spectrum (and back)
- Black hole explosions?
- Moduli constraints on primordial black holes
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