Massive black hole remnants of the first stars in galactic haloes

Abstract

We investigate the possibility that present-day galactic haloes contain a population of massive black holes (MBHs) that form by hierarchical merging of the black hole remnants of the first stars. Some of the MBHs may be large enough or close enough to the centre of the galactic host that they merge within a Hubble time. We estimate to what extent this process could contribute to the mass of the super-massive black holes (SMBHs) observed in galactic centres today. Many MBHs will not reach the centre of the main halo, however, but continue to orbit within satellite subhaloes. Using a semi-analytical approach that explicitly accounts for dynamical friction, tidal disruption and encounters with the galactic disk, we follow the dynamics of the satellites and their MBHs and determine the abundance and distribution of MBHs in present-day haloes of various masses. Considering two different accretion scenarios we also compute the bolometric luminosity function for the MBHs.

Accepted for publication in MNRAS, 11 pages, 11 figures

References in corpus (34)

• The Demography of Massive Dark Objects in Galaxy Centres
• The Formation of the First Stars. I. The Primordial Star Forming Cloud
• The Assembly and Merging History of Supermassive Black Holes in Hierarchical Models of Galaxy Formation
• Massive Black Holes as Population III Remnants
• Observational constraints on growth of massive black holes
• How small were the first cosmological objects?
• Formation of Galactic Nuclei
• Beyond the Bulge: a Fundamental Relation Between Supermassive Black Holes and Dark Matter Halos
• The Formation and Fragmentation of Primordial Molecular Clouds
• The dynamical evolution of massive black hole binaries - I. Hardening in a fixed stellar background
• First stars, very massive black holes and metals
• The Power Spectrum Dependence of Dark Matter Halo Concentrations
• Black Hole Mass Estimates from Reverberation Mapping and from Spatially Resolved Kinematics
• Evolution of massive binary black holes
• Formation of gas disks in merging galaxies
• Simulations of Pregalactic Structure Formation with Radiative Feedback
• How to Plant a Merger Tree
• A Correlation between Galaxy Light Concentration and Supermassive Black Hole Mass
• Black Hole Demographics from the M(BH)-sigma Relation
• Chandra High-Resolution Camera Observations of the Luminous X-Ray Source in the Starburst Galaxy M82
• The correlation between black hole mass and bulge velocity dispersion in hierarchical galaxy formation models
• Spectrum of Optically Thin Advection Dominated Accretion Flow around a Black Hole: Application to Sgr A*
• The Dynamics of Sinking Satellites Around Disk Galaxies: A Poor Man's Alternative to High-Resolution Numerical Simulations
• Binary Black Hole Mergers from Planet-like Migrations
• The Merger History of Supermassive Black Holes in Galaxies
• Low-frequency gravitational waves from supermassive black holes
• On The Linearity of The Black Hole - Bulge Mass Relation in Active and in Nearby Galaxies
• Simulation of primordial object formation
• Radiation from the first forming stars
• A Theoretical Model for the $M_{\mathrm{bh}}-\sigma$ Relation for Supermassive Black Holes in Galaxies
• Chandra Observations of "The Antennae" Galaxies (NGC 4038/39): II. Detection and Analysis of Galaxian X-ray source
• Spectral Models of Convection-Dominated Accretion Flows
• Emission from Isolated Black Holes and MACHOs Accreting from the Interstellar Medium
• How big were the first cosmological objects?

Cited by in corpus (71)

• The First Stars
• Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
• Formation of the First Supermassive Black Holes
• Intermediate-Mass Black Holes
• Consequences of gravitational radiation recoil
• The First Cosmic Structures and their Effects
• Active Galactic Nuclei with Candidate Intermediate-Mass Black Holes
• Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors
• Massive black hole seeds from low angular momentum material
• Early reionization by miniquasars
• How Mergers May Affect The Mass Scaling Relations Between Black Holes, Galaxies, and Other Gravitationally Bound Systems
• The First Galaxies: Assembly, Cooling and the Onset of Turbulence
• Blossoms from black hole seeds: properties and early growth regulated by supernova feedback
• Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time
• A New Signature of Dark Matter Annihilations: Gamma-Rays from Intermediate-Mass Black Holes
• Low-mass black holes as the remnants of primordial black hole formation
• Off the Beaten Path: A New Approach to Realistically Model The Orbital Decay of Supermassive Black Holes in Galaxy Formation Simulations
• Accretion onto Seed Black Holes in the First Galaxies
• The Low End of the Supermassive Black Hole Mass Function: Constraining the Mass of a Nuclear Black Hole in NGC 205 via Stellar Kinematics
• The Era of Massive Population III Stars: Cosmological Implications and Self-Termination
• Gravitational waves as a probe of dark matter mini-spikes
• Black Hole Growth in Hierarchical Galaxy Formation
• Constraints from Gravitational Recoil on the Growth of Supermassive Black Holes at High Redshift
• Detecting dark matter WIMPs in the Draco dwarf: a multi-wavelength perspective
• Pregalactic Black Hole Formation with an Atomic Hydrogen Equation of State
• Dynamical evolution of intermediate mass black holes and their observable signatures in the nearby Universe
• Gravitational Wave Recoil and the Retention of Intermediate Mass Black Holes
• Supermassive Seeds for Supermassive Black Holes
• Constraining the primordial initial mass function with stellar archaeology
• Population III and the Near-Infrared Background Excess
• The Formation of the First Massive Black Holes
• Secondary anisotropies of the CMB
• Gravitational waves and stalled satellites from massive galaxy mergers at z <= 1
• The Millennium Galaxy Catalogue: The local supermassive black hole mass function in early- and late-type galaxies
• Can Supersymmetry Naturally Explain the Positron Excess?
• Supermassive Black Hole Growth and Merger Rates from Cosmological N-body Simulations
• The Early Growth of the First Black Holes
• A Unique Multi-Messenger Signal of QCD Axion Dark Matter
• Hyper-Eddington mass accretion onto a black hole with super-Eddington luminosity
• Star Clusters Around Recoiled Black Holes in the Milky Way Halo
• Massive black hole remnants of the first stars I: abundance in present-day galactic haloes
• Have Atmospheric Cerenkov Telescopes Observed Dark Matter?
• A Population of Relic Intermediate-Mass Black Holes in the Halo of the Milky Way
• Constraints on Galactic Intermediate Mass Black Holes
• Intermediate Mass-Ratio Inspirals with Dark Matter Minispikes
• Binary Disruption by Massive Black Holes in Globular Clusters
• Growing Massive Black Holes in a Local Group Environment: the Central Supermassive, Slowly Sinking, and Ejected Populations
• Ultrahigh-energy cosmic rays from tidally-ignited white dwarfs
• Dark matter annihilation from intermediate-mass black holes: Contribution to the extragalactic gamma-ray background
• Search for Gamma-rays from Dark Matter annihilations around Intermediate Mass Black Holes with the H.E.S.S. experiment
• A variable ultra-luminous X-ray source in the colliding galaxy NGC 7714
• Radiation from early black holes - I: effects on the neutral inter-galactic medium
• Disk Assembly and the M_BH-sigma Relation of Supermassive Black Holes
• Are Ultra-Luminous X-ray Sources Intermediate Mass Black Holes Accreting from Molecular Clouds?
• On the dynamics of the satellite galaxies in NGC 5044
• The Role of Primordial Kicks on Black Hole Merger Rates
• Discovery of the Candidate Off-nuclear Ultrasoft Hyper-luminous X-ray Source 3XMM J141711.1+522541
• Gravitational Wave Signal from Assembling the Lightest Supermassive Black Holes
• The Formation and Evolution of the First Massive Black Holes
• The concentration-velocity dispersion relation in galaxy groups
• The imprint of the cosmic supermassive black hole growth history on the 21 cm background radiation
• Detection of Gravitational Waves from the Coalescence of Population-III Remnants with Advanced LIGO
• Mechanism for the Suppression of Intermediate-Mass Black Holes
• Gamma-Rays from Dark Matter Mini-Spikes in M31
• The black hole mass versus velocity dispersion relation in QSOs/Active Galactic Nuclei: observational appearance and black hole growth
• SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
• Growth of massive black holes at high-z via accretion predominantly driven by magnetic outflows
• Can gas dynamics in centres of galaxies reveal orbiting massive black holes?
• Kickstarting Reionization with the First Black Holes: the effects of second-order perturbation theory in pre-reionization volumes
• Metal Enrichment of the Intergalactic Medium and Production of Massive Black Holes
• Formation and Evolution of Supermassive Black Holes