Inflaton accretion onto primordial black holes during reheating
astro-ph.CO, gr-qc, hep-ph
Submitted: 2026-05-19
Updated: 2026-09-10
Comments: 41 pages, 14 figures, Published in Physical Review D
Journal ref: Phys. Rev. D 114, 063517 (2026)
DOI: 10.1103/cgll-c5kh
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Constraints on Primordial Black Holes From Big Bang Nucleosynthesis Revisited
- Constraints on Primordial Black Holes
- Primordial Black Holes as Dark Matter
- Primordial Black Holes as Dark Matter: Recent Developments
- Primordial Black Holes as a dark matter candidate
- Could supermassive black holes be quintessential primordial black holes?
- Primordial Black Holes as Generators of Cosmic Structures
- Primordial Black Holes - Perspectives in Gravitational Wave Astronomy -
- Did LIGO detect dark matter?
- The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO
- Near-Critical Gravitational Collapse and the Initial Mass Function of Primordial Black Holes
- Computations of primordial black hole formation
- Threshold of primordial black hole formation
- Towards the Theory of Reheating After Inflation
- Inflation Dynamics and Reheating
- Reheating in Inflationary Cosmology: Theory and Applications
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- Dynamical and Gravitational Instability of Oscillating-Field Dark Energy and Dark Matter
- Inflaton Oscillations and Post-Inflationary Reheating
- Primordial Black Holes for the LIGO Events in the Axion-like Curvaton Model
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation