Prospects of Indirect Detection of Dark Matter via Primordial Black Hole Induced Gravitational Waves
astro-ph.CO, hep-ph
Submitted: 2026-02-16
Updated: 2026-08-25
Terminology
Sources
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
- GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
- GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Single-field inflation, anomalous enhancement of superhorizon fluctuations, and non-Gaussianity in primordial black hole formation
- Primordial black holes from single field models of inflation
- Scalaron from $R^2$-gravity as a Heavy Field
- Cosmic String Loop Collapse in Full General Relativity
- Primordial black holes from cusp collapse on cosmic strings
- String Necklaces and Primordial Black Holes from Type IIB Strings
- Black Holes from Fermi Ball Collapse
- Direct-collapse supermassive black holes from relic particle decay
- Revisiting formation of primordial black holes in a supercooled first-order phase transition
- Structure Formation after Reheating: Supermassive Primordial Black Holes and Fermi Ball Dark Matter
- Primordial black hole formation from self-resonant preheating?
- Unification models with reheating via primordial black holes
- Primordial black holes from the preheating instability
- Dark Radiation and Superheavy Dark Matter from Black Hole Domination
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