Primordial black holes as a natural consequence of scale-invariance
astro-ph.CO, hep-ph
Submitted: 2026-10-07
Updated: 2026-10-07
Terminology
Sources
- Planck 2018 results. X. Constraints on inflation
- Higgs-Dilaton Cosmology: From the Early to the Late Universe
- Higgs-Dilaton Cosmology: an effective field theory approach
- Agravity
- Scale-Independent Inflation and Hierarchy Generation
- Weyl Current, Scale-Invariant Inflation and Planck Scale Generation
- Cosmology with a TeV mass GUT Higgs
- Thermal Inflation and the Moduli Problem
- Primordial Black Holes from Thermal Inflation
- Escape from supercooling with or without bubbles: gravitational wave signatures
- The NANOGrav 11-year Data Set: Pulsar-timing Constraints On The Stochastic Gravitational-wave Background
- Significance of soft-scale breaking on primordial black hole production in Coleman-Weinberg type supercooling-phase transition
- Spontaneous breaking of the Peccei-Quinn symmetry during warm inflation
- Large-scale Perturbations from the Waterfall Field in Hybrid Inflation
- Spinodal Inflation
- Smearing Formula for Higher-Order Effective Classical Potentials
- Spinodal Decomposition and Inflation: Dynamics and Metric Perturbations
- Spinodal Backreaction During Inflation and Initial Conditions
- Waterfall field in hybrid inflation and curvature perturbation
- Calculating the mass spectrum of primordial black holes
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