Heavy primordial black holes from strongly clustered light black holes
arXiv:2210.14171 · doi:10.1103/PhysRevLett.130.171401
Abstract
We show that heavy primordial black holes may originate from much lighter ones if the latter are strongly clustered at the time of their formation. While this population is subject to the usual constraints from late-time universe observations, its relation to the initial conditions is different from the standard scenario and provides a new mechanism to generate massive primordial black holes even in the absence of efficient accretion, opening new scenarios, e.g. for the generation of supermassive black holes.
arXiv comment6 pages, 2 figures. v2: matching version published in PRL
References in corpus (47)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- Did LIGO detect dark matter?
- Constraints on Primordial Black Holes
- Observational constraints on growth of massive black holes
- Primordial Black Hole Scenario for the Gravitational-Wave Event GW150914
- Primordial Black Holes - Perspectives in Gravitational Wave Astronomy -
- Formation of Supermassive Black Holes
- Primordial Black Holes as a dark matter candidate
- The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO
- Self-Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative Efficiency
- The merger rate of primordial-black-hole binaries
- Axion Miniclusters and Bose Stars
- Eddington-limited accretion and the black hole mass function at redshift 6
- Steepest growth of the power spectrum and primordial black holes
- The origins of massive black holes
- Gravitational Wave signatures of inflationary models from Primordial Black Hole Dark Matter
- Cosmic microwave background bounds on primordial black holes including dark matter halo accretion
- Two populations of LIGO-Virgo black holes
- Primordial Black Holes Confront LIGO/Virgo data: Current situation
- Large-amplitude isothermal fluctuations and high-density dark-matter clumps
- Searching for a subpopulation of primordial black holes in LIGO/Virgo gravitational-wave data
- Early Structure Formation in PBH Cosmologies
- From inflation to black hole mergers and back again: Gravitational-wave data-driven constraints on inflationary scenarios with a first-principle model of primordial black holes across the QCD epoch
- Limits on primordial black holes from distortions in cosmic microwave background
- Accelerating early massive galaxy formation with primordial black holes
- Distinguishing Primordial Black Holes from Astrophysical Black Holes by Einstein Telescope and Cosmic Explorer
- The Clustering Evolution of Primordial Black Holes
- The Spatial Clustering of Primordial Black Holes
- Bayesian Evidence for Both Astrophysical and Primordial Black Holes: Mapping the GWTC-2 Catalog to Third-Generation Detectors
- Signatures of non-gaussianity in the isocurvature modes of primordial black hole dark matter
- On the merger rate of primordial black holes: effects of nearest neighbours distribution and clustering
- Correlation function of high-threshold regions and application to the initial small-scale clustering of primordial black holes
- Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
- Primordial black holes from long-range scalar forces and scalar radiative cooling
- Stochastic gravitational-wave background as a tool to investigate multi-channel astrophysical and primordial black-hole mergers
- Assessing the redshift evolution of massive black holes and their hosts
- Gravitational waves from dark matter isocurvature
- Prospects for probing gravitational waves from primordial black hole binaries
- The Minimum Testable Abundance of Primordial Black Holes at Future Gravitational-Wave Detectors
- Primordial Black Holes from Broad Spectra: Abundance and Clustering
- Gravitational Waves from Density Perturbations in an Early Matter Domination Era
- Ruling out Initially Clustered Primordial Black Holes as Dark Matter
- LIGO/Virgo black holes and dark matter: The effect of spatial clustering
- Constraining the Initial Primordial Black Hole Clustering with CMB-distortion
- Gravitational Waves from Peaks
Cited by in corpus (11)
- The Science of the Einstein Telescope
- Primordial black holes from null energy condition violation during inflation
- Pinning down the primordial black hole formation mechanism with gamma-rays and gravitational waves
- Distinguishing the impact and signature of black holes from different origins in early cosmic history
- The Irrelevance of Primordial Black Hole Clustering in the LVK mass range
- Primordial Black-Hole-Based Pathways to Little Red Dots
- Revisiting primordial black holes formation from preheating instabilities: the case of Starobinsky inflation
- Clustering and Runaway Merging in a Primordial Black Hole Dominated Universe
- What happens when supercooling is terminated by curvature flipping of the effective potential?
- Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters
- The Dark Side of the Moon: Listening to Scalar-Induced Gravitational Waves