Published on:
5 March 2024
Primary Category:
Cosmology and Nongalactic Astrophysics
Paper Authors:
Antonio Riotto,
Joe Silk
What is the abundance of primordial black holes across the mass spectrum
How significantly do primordial black holes cluster and affect their merger rates
What fraction of current gravitational wave events are primordial black hole binaries
Are primordial black holes the dark matter, especially in the unconstrained asteroid mass range
Future gravitational wave detectors and multimessenger experiments provide smoking gun probes of primordial black holes to high redshifts and low masses
Open questions around primordial black holes
This paper discusses key open questions and future research directions related to primordial black holes (PBHs). PBHs are hypothetical black holes that may have formed in the early universe. Though not confirmed, they are an intriguing dark matter candidate and could play various roles in astrophysics and cosmology. The paper summarizes open theoretical and observational issues around constraining PBH abundance across the mass spectrum, assessing their clustering properties and merger rates, evaluating their contribution to detected gravitational wave events, and testing whether they make up all dark matter. It then outlines a detailed roadmap spanning gravitational wave detectors, microlensing surveys, 21cm experiments, and more, that can provide definitive tests for PBHs in the coming years through smoking gun signatures like high redshift mergers and sub-solar mass detections.
Primordial black hole formation and detection
Quantum effects extend primordial black hole lifetimes as dark matter candidates
Gravitational waves reveal primordial black hole origins
Unveiling the hidden population of black holes in the dark matter halos of galaxies
Link between primordial black hole formation and properties of unstable null geodesics
Primordial black holes remain viable dark matter candidates despite extended mass distribution
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