Published on:
14 July 2023
Primary Category:
Cosmology and Nongalactic Astrophysics
Paper Authors:
A. Esteban-Gutiérrez,
E. Mediavilla,
J. Jiménez-Vicente,
J. A. Muñoz
Microlensing of lensed quasars is a powerful probe of dark matter in the form of compact objects like black holes
X-ray observations are sensitive to microlensing by lower mass black holes than optical data
Bayesian analysis used to calculate probability of different black hole populations based on microlensing data
Abundance of substellar to planetary mass black holes is negligible based on microlensing constraints
New limits set on fraction of dark matter composed of black holes from 0.005 to 100 solar masses
Unveiling the hidden population of black holes in the dark matter halos of galaxies
This paper uses gravitational microlensing of distant quasars to search for primordial black holes of substellar to planetary mass in the dark matter halos of lensing galaxies. The results indicate the abundance of these black holes is negligible, providing stringent constraints on their contribution to dark matter in the mass range from 0.005 to 100 solar masses.
LIGO constrains primordial black holes down to planetary masses
Gravitational lensing of black holes reveals dark matter in galaxies
Open questions around primordial black holes
A General Audience Guide to Probing Black Holes with Submillimeter Light
Primordial black holes remain viable dark matter candidates despite extended mass distribution
Constraining quasar host halo mass with circumgalactic medium kinematics
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