LISA double black holes: Dynamics in gaseous nuclear discs
arXiv:astro-ph/0509813 · doi:10.1111/j.1365-2966.2005.09956.x
Abstract
We study the inspiral of double black holes, with masses in the LISA window of detectability, orbiting inside a massive circum-nuclear disc. Using high-resolution SPH simulations, we follow the black hole dynamics in the early phase when gas-dynamical friction acts on the black holes individually, and continue our simulation until they form a close binary. We find that in the early sinking the black holes lose memory of their initial orbital eccentricity if they co-rotate with the gaseous disc, forming a binary with a low eccentricity, consistent with zero within our numerical resolution limit. The cause of circularization resides in the rotation present in the gaseous background where dynamical friction operates. Circularization may hinder gravitational waves from taking over and leading the binary to coalescence. In the case of counter-rotating orbits the initial eccentricity does not decrease, and the black holes may bind forming an eccentric binary. When dynamical friction has subsided, for equal mass black holes and regardless their initial eccentricity, angular momentum loss, driven by the gravitational torque exerted on the binary by surrounding gas, is nevertheless observable down to the smallest scale probed. In the case of unequal masses, dynamical friction remains efficient down to our resolution limit, and there is no sign of formation of any ellipsoidal gas distribution that may further harden the binary. During inspiral, gravitational capture of gas by the black holes occurs mainly along circular orbits: eccentric orbits imply high relative velocities and weak gravitational focusing. Thus, AGN activity may be excited during the black hole pairing process and double active nuclei may form when circularization is completed, on distance-scales of tens of pcs.
Minor changes, accepted to MNRAS (11 pags, 14 figs). Movies (.avi) are available at http://pitto.mib.infn.it/~haardt/MOVIES/
References in corpus (33)
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- The Demography of Massive Dark Objects in Galaxy Centres
- GADGET: A code for collisionless and gasdynamical cosmological simulations
- On the Black Hole Mass - Bulge Mass Relation
- Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies
- The Assembly and Merging History of Supermassive Black Holes in Hierarchical Models of Galaxy Formation
- Discovery of a binary AGN in the ultraluminous infrared galaxy NGC 6240 using Chandra
- Formation of Galactic Nuclei
- Dynamical Friction in a Gaseous Medium
- Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries
- Evolution of massive binary black holes
- Accretion during the merger of supermassive black holes
- The Role of Gas in the Merging of Massive Black Holes in Galactic Nuclei. II. Black Hole Merging in a Clumpy Disk
- The Afterglow of Massive Black Hole Coalescence
- An Intermediate-Mass Black Hole in the Globular Cluster G1: Improved Significance from New Keck and Hubble Space Telescope Observations
- Axisymmetric, 3-Integral Models of Galaxies: A Massive Black Hole in NGC3379
- Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15: II. Kinematical Analysis and Dynamical Modeling
- The Role of Gas in the Merging of Massive Black Holes in Galactic Nuclei. I. Black Hole Merging in a Spherical Gas Cloud
- A 20 Thousand Solar Mass Black Hole in the Stellar Cluster G1
- Dynamical friction and the evolution of satellites in virialized halos: the theory of linear response
- Eccentricity of supermassive black hole binaries coalescing from gas rich mergers
- The gravitational wave signal from massive black hole binaries and its contribution to the LISA data stream
- Substructure in Dark Halos: Orbital Eccentricities and Dynamical Friction
- Low-frequency gravitational waves from supermassive black holes
- Arp 299: a second merging system with two active nuclei?
- Fate of Supermassive Black Holes and Evolution of the M(BH)-sigma Relation in Merging Galaxies: The Effect of Gaseous Dissipation
- Long-Term Evolution of Massive Black Hole Binaries. II. Binary Evolution in Low-Density Galaxies
- Evolution of Massive Black Hole Binaries
- The time-scale for core collapse in spherical star clusters
- Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15: I. STIS Spectroscopy and WFPC2 Photometry
- The fate of central black holes in merging galaxies
- Dynamical friction of bodies orbiting in a gaseous sphere
- The case of PSR J1911-5958A in the outskirts of NGC 6752: signature of a black hole binary in the cluster core?
Cited by in corpus (102)
- Rapid Formation of Supermassive Black Hole Binaries in Galaxy Mergers with Gas
- Alignment of the spins of supermassive black holes prior to coalescence
- Efficient Merger of Binary Supermassive Black Holes in Non-Axisymmetric Galaxies
- Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays
- Supermassive black hole binaries in gaseous and stellar circumnuclear discs: orbital dynamics and gas accretion
- The evolution of massive black holes and their spins in their galactic hosts
- The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
- Journey to the M_BH -sigma relation: the fate of low mass black holes in the Universe
- Quasars at z=6: the survival of the fittest
- Gravitational wave background from binary systems
- Gravitational Recoil From Accretion-Aligned Black-Hole Binaries
- Post-Circular Expansion of Eccentric Binary Inspirals: Fourier-Domain Waveforms in the Stationary Phase Approximation
- The imprint of massive black hole formation models on the LISA data stream
- Massive binary black holes in galactic nuclei and their path to coalescence
- Dual black holes in merger remnants. II: spin evolution and gravitational recoil
- Massive black hole binaries: dynamical evolution and observational signatures
- Self consistent model for the evolution of eccentric massive black hole binaries in stellar environments: implications for gravitational wave observations
- Observable Signatures of a Black Hole Ejected by Gravitational Radiation Recoil in a Galaxy Merger
- Hydrodynamics of galaxy mergers with supermassive black holes: is there a last parsec problem ?
- Identifying Supermassive Black Hole Binaries with Broad Emission Line Diagnosis
- An eccentric binary black hole inspiral-merger-ringdown gravitational waveform model from numerical relativity and post-Newtonian theory
- Dynamical Friction of a Circular-Orbit Perturber in a Gaseous Medium
- Comparisons of eccentric binary black hole simulations with post-Newtonian models
- Electromagnetic Counterparts to Massive Black Hole Mergers
- eLISA: Astrophysics and cosmology in the millihertz regime
- Eccentric binary black-hole mergers: The transition from inspiral to plunge in general relativity
- Insights on the astrophysics of supermassive black hole binaries from pulsar timing observations
- Constraining sub-Parsec Binary Supermassive Black Holes in Quasars with Multi-Epoch Spectroscopy. I. The General Quasar Population
- SDSSJ092712.65+294344.0: a candidate massive black hole binary
- Interaction of massive black hole binaries with their stellar environment: II. Loss-cone depletion and binary orbital decay
- Mass and spin coevolution during the alignment of a black hole in a warped accretion disc
- Massive Black Hole binaries in gas-rich galaxy mergers; multiple regimes of orbital decay and interplay with gas inflows
- Constraining Sub-Parsec Binary Supermassive Black Holes in Quasars with Multi-Epoch Spectroscopy. II. The Population with Kinematically Offset Broad Balmer Emission Lines
- Triplets of supermassive black holes: Astrophysics, Gravitational Waves and Detection
- A Large Systematic Search for Close Supermassive Binary and Rapidly Recoiling Black Holes - III. Radial Velocity Variations
- Dual black holes in merger remnants. I: linking accretion to dynamics
- Modeling of Emission Signatures of Massive Black Hole Binaries: I Methods
- Stellar and Gaseous Nuclear Disks Observed in Nearby (U)LIRGs
- The Current Status of Binary Black Hole Simulations in Numerical Relativity
- Gravitational recoil velocities from eccentric binary black hole mergers
- Sub-parsec supermassive Binary Quasars: expectations at z<1
- Dynamical Friction of Double Perturbers in a Gaseous Medium
- On the search of electromagnetic cosmological counterparts to coalescences of massive black hole binaries
- Towards a Comprehensive Fueling-Controlled Theory on the Growth of Massive Black Holes and Host Spheroids
- Nonlinear Dynamical Friction in a Gaseous Medium
- Search of sub-parsec massive binary black holes through line diagnosis
- Gaseous Dynamical Friction in Presence of Black Hole Radiative Feedback
- Compact massive objects in Virgo galaxies: the black hole population
- LISA observations of massive black hole mergers: event rates and issues in waveform modelling
- Dynamical Evolution and Merger Time-scales of LISA Massive Black Hole Binaries in Disk Galaxy Mergers
- The competing effect of gas and stars in massive black hole binaries evolution
- Emission Signatures from Sub-parsec Binary Supermassive Black Holes I: Diagnostic Power of Broad Emission Lines
- Dynamical Friction in a Gas: The Subsonic Case
- Supermassive Black Hole Binaries: The Search Continues
- Computing waveforms for spinning compact binaries in quasi-eccentric orbits
- LISA detection of massive black hole binaries: imprint of seed populations and of exterme recoils
- SDSS 0956+5128: A Broad-line Quasar with Extreme Velocity Offsets
- Imprints of recoiling massive black-holes on the hot gas of early type galaxies
- Super massive black holes in star forming gaseous circumnuclear discs
- Angular Momentum and the Formation of Stars and Black Holes
- Emission Lines as a Tool in Search for Supermassive Black Hole Binaries and Recoiling Black Holes
- Nonlinear Dynamical Friction of a Circular-Orbit Perturber in a Gaseous Medium
- Dynamical friction-driven orbital circularisation in rotating discs: a semi-analytical description
- Pairing of Massive Black Holes in Merger Galaxies Driven by Dynamical Friction
- Star cluster disruption by a massive black hole binary
- Massive black hole and gas dynamics in mergers of galaxy nuclei - II. Black hole sinking in star-forming nuclear discs
- Gravitationally Induced Density Wake of a Circularly Orbiting Object As an Interpretative Framework of Ubiquitous Spirals and Arcs
- Binary-disk interaction: Gap-Opening criteria
- Massive Black Holes: formation and evolution
- Gravitational drag on a point mass in hypersonic motion through a gaseous medium
- RABBITS -- I. The crucial role of nuclear star formation in driving the coalescence of supermassive black hole binaries
- Constraints on the Galactic Centre environment from \textit{Gaia} hypervelocity stars III: Insights on a possible companion to Sgr A*
- Binary Disk interaction II: Gap-Opening criteria for unequal mass binaries
- Massive black hole binary evolution in gas-rich mergers
- Probing the Merger Rates of Supermassive Black Holes and Galaxies with Gravitational Waves
- Dynamical evolution of massive perturbers in realistic multi-component galaxy models I: implementation and validation
- Multiple regimes and coalescence timescales for massive black hole pairs ; the critical role of galaxy formation physics
- On the fragility of nuclear stellar discs against galaxy mergers: surviving photometric and kinematic signatures of nuclear discs
- Radio Bimodality: Spin, Accretion Mode, or Both?
- Dynamical friction in a gaseous medium with a large-scale magnetic field
- Probing the Delay Time of Supermassive Black Hole Binary Mergers With Gravitational Waves
- Dynamical evolution of massive black hole pairs in the presence of spin-dependent radiative feedback
- RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
- Stellar hardening of massive black hole binaries: the impact of the host rotation
- Binary AGN simulations with radiation pressure reveal a new duty cycle, and a reduction of gravitational torque, through 'minitori' structures
- A conservation-based method for simulating the inspiral of binary black holes
- Accretion of clumpy cold gas onto massive black holes binaries: the challenging formation of extended circumbinary structures
- Astrophysics with the Laser Interferometer Space Antenna
- Linear frictional forces cause orbits to neither circularize nor precess
- Black hole-galaxy co-evolution and the role of feedback
- Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
- Multi-scale simulations of merging galaxies with supermassive black holes
- Living with Neighbors. V. Better-aligned Spiral+Spiral Galaxy Pairs Show Stronger Star Formation
- A Shining Death of Unequal Supermassive Black Hole Binaries
- Formation of counter-rotating and highly eccentric massive black hole binaries in galaxy mergers
- Effects of Minor Mergers on Coalescence of a Supermassive Black Hole Binary
- Probing the Growth of Massive Black Holes with Black Hole-Host Galaxy Spin Correlations
- Evolution of massive black holes
- Contaminating Electromagnetic Transients in LISA Gravitational Wave Localization Volumes. I: The Intrinsic Rates
- Spacetime in motion: an evolving relativistic binary black hole metric for GIZMO
- Black Hole merger rates in the first billion years in light of JWST data
- Mass flow in the circumbinary disk with gap around supermassive binary black holes