How Primordial Black Holes Change BBN
astro-ph.CO, astro-ph.HE, hep-ph
Submitted: 2025-11-23
Updated: 2026-08-31
Terminology
Sources
- Constraints on Primordial Black Holes
- Primordial black holes as a tool for constraining non-Gaussianity
- Effects of Critical Collapse on Primordial Black-Hole Mass Spectra
- Primordial black hole formation by vacuum bubbles
- Primordial black hole and wormhole formation by domain walls
- Primordial black hole formation in the matter-dominated phase of the Universe
- PBH abundance from random Gaussian curvature perturbations and a local density threshold
- Spins of primordial black holes formed in the matter-dominated phase of the Universe
- Analytic Description of Primordial Black Hole Formation from Scalar Field Fragmentation
- Primordial black holes from supersymmetry in the early universe
- Primordial Black Holes as Dark Matter
- Primordial Black Holes as a dark matter candidate
- Primordial Black Holes as Dark Matter: Recent Developments
- Did LIGO detect dark matter?
- Inflationary Primordial Black Holes as All Dark Matter
- The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO
- Primordial Black Holes and $r$-Process Nucleosynthesis
- Constraining the primordial black hole abundance through Big-Bang nucleosynthesis
- Primordial Black Holes as Generators of Cosmic Structures
- Illuminating the dark ages: Cosmic backgrounds from accretion onto primordial black hole dark matter
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