Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models

Abstract

We study the merger rate of primordial black holes (PBHs) in self-interacting dark matter (SIDM) halo models. To explore a numerical description for the density profile of SIDM halo models, we use the result of a previously performed simulation for SIDM halo models with $\sigma /m=10\mathrm{c}{\mathrm{m}}^2{\mathrm{g}}^{-1}$. We also propose a concentration-mass-time relation that can explain the evolution of the halo density profile related to SIDM models. Furthermore, we investigate the encounter condition of PBHs that may have been randomly distributed in the medium of dark matter halos. Under these assumptions, we calculate the merger rate of PBHs within each halo considering SIDM halo models and compare the results with that obtained for cold dark matter (CDM) halo models. To do this, we employ the definition of the time after halo virialization as a function of halo mass. We indicate that SIDM halo models for $f_{\mathrm{PBH}}>0.32$ can generate sufficient PBH mergers in such a way that those exceed the one resulted from CDM halo models. By considering the spherical-collapse halo mass function, we obtain similar results for the cumulative merger rate of PBHs. Moreover, we calculate the redshift evolution of the PBH total merger rate. To determine a constraint on the PBH abundance, we study the merger rate of PBHs in terms of their fraction and masses and compare those with the black hole merger rate estimated by the Advanced LIGO (aLIGO)-Advanced Virgo (aVirgo) detectors during the third observing run. The results demonstrate that within the context of SIDM halo models, the merger rate of $10M_{\odot }-10M_{\odot }$ events can potentially fall within the aLIGO-aVirgo window. We also estimate a relation between the fraction of PBHs and their masses, which is well consistent with our findings.

arXiv comment17 pages, 9 figures, refs. added, fixed some typos

References in corpus (79)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• A Universal Density Profile from Hierarchical Clustering
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
• Dark Matter Substructure in Galactic Halos
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
• Observational evidence for self-interacting cold dark matter
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• Tests of general relativity with GW150914
• Mass function of dark matter halos
• GW190521: A Binary Black Hole Merger with a Total Mass of $150M_{\odot }$
• Did LIGO detect dark matter?
• Constraints on Primordial Black Holes
• Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles
• Primordial Black Hole Scenario for the Gravitational-Wave Event GW150914
• Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• Primordial Black Holes - Perspectives in Gravitational Wave Astronomy -
• Primordial Black Holes as Dark Matter: Recent Developments
• Concentration, Spin and Shape of Dark Matter Haloes as a Function of the Cosmological Model: WMAP1, WMAP3 and WMAP5 results
• Halo concentrations in the standard LCDM cosmology
• The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO
• Subhaloes in Self-Interacting Galactic Dark Matter Haloes
• Precision Determination of the Mass Function of Dark Matter Halos
• Gravitational waves from scattering of stellar-mass black holes in galactic nuclei
• Cosmological Simulations with Self-Interacting Dark Matter II: Halo Shapes vs. Observations
• Cosmic microwave background limits on accreting primordial black holes
• The merger rate of primordial-black-hole binaries
• Primordial black hole constraints for extended mass functions
• Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential
• The halo mass function from the dark ages through the present day
• Dynamics of Primordial Black Hole Formation
• Black hole formation in the Friedmann universe: Formulation and computation in numerical relativity
• The Mass-Concentration-Redshift Relation of Cold and Warm Dark Matter Halos
• Constraints on MACHO Dark Matter from Compact Stellar Systems in Ultra-Faint Dwarf Galaxies
• Formation and Evolution of Primordial Black Hole Binaries in the Early Universe
• Primordial black hole formation in the early universe: critical behaviour and self-similarity
• The Mass-Concentration-Redshift Relation of Cold Dark Matter Halos
• Cosmic microwave background bounds on primordial black holes including dark matter halo accretion
• Femtolensing by Dark Matter Revisited
• Limits on stellar-mass compact objects as dark matter from gravitational lensing of type Ia supernovae
• The Halo Mass Function: High-Redshift Evolution and Universality
• Calculating the mass spectrum of primordial black holes
• Evolution of the Mass Function of Dark Matter Haloes
• Revisiting constraints on asteroid-mass primordial black holes as dark matter candidates
• Lower bound on the primordial black hole merger rate
• A Test of the Collisional Dark Matter Hypothesis from Cluster Lensing
• Updated Constraints on Asteroid-Mass Primordial Black Holes as Dark Matter
• Black Holes' Dark Dress: On the merger rate of a subdominant population of primordial black holes
• Black Hole Binary Formation in the Expanding Universe --- Three Body Problem Approximation ---
• Dynamics of dwarf galaxies disfavor stellar-mass black hole dark matter
• Curvature profiles as initial conditions for primordial black hole formation
• Supermassive Black Holes from Ultra-Strongly Self-Interacting Dark Matter
• Direct Detection of Hawking Radiation from Asteroid-Mass Primordial Black Holes
• Stochastic Gravitational-Wave Background due to Primordial Binary Black Hole Mergers
• Runaway Merging of Black Holes: Analytical Constraint on the Timescale
• Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons
• Limits on Collisional Dark Matter from Elliptical Galaxies in Clusters
• New X-ray bound on density of primordial black holes
• Near future MeV telescopes can discover asteroid-mass primordial black hole dark matter
• Velocity-dependent Self-interacting Dark Matter from Groups and Clusters of Galaxies
• Galactic Substructure and Direct Detection of Dark Matter
• Astrophysical uncertainties on the local dark matter distribution and direct detection experiments
• Primordial black hole merger rates: distributions for multiple LIGO observables
• When are LIGO/Virgo's Big Black-Hole Mergers?
• Self-interacting Dark Matter from Primordial Black Holes
• Primordial-black-hole mergers in dark-matter spikes
• The structure and assembly history of cluster-size haloes in Self-Interacting Dark Matter
• How well do we know the Halo Mass Function?
• The Observed Rate of Binary Black Hole Mergers can be Entirely Explained by Globular Clusters
• Concentration, Ellipsoidal Collapse, and the Densest Dark Matter haloes
• The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology
• The Maximal-Density Mass Function for Primordial Black Hole Dark Matter
• N-body simulations of dark matter with frequent self-interactions
• Constraining self-interacting dark matter with scaling laws of observed halo surface densities
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• Primordial black holes in linear and non-linear regimes
• Model-independent discovery prospects for primordial black holes at LIGO

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• Compact Binary Merger Rate in Dark-Matter Spikes
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Primordial Black Hole Merger Rate in $f(R)$ Gravity
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Gravitational Lensing in More Realistic Dark Matter Halo Models
• Toward More Realistic Mass Functions For Ultradense Dark Matter Halos
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Matching JWST UV Luminosity Functions with Refined $\Lambda$CDM Halo Models
• High-redshift Galaxies from JWST Observations in More Realistic Dark Matter Halo Models
• Merger History of Clustered Primordial Black Holes
• Ultradense Dark Matter Halos with Poisson Noise from Stellar-Mass Primordial Black Holes
• Toward Gravitational Lensing in Modified Theories of Gravity
• Chameleon Gravity as an Alternative to Dark Matter