Beyond the Bulge: a Fundamental Relation Between Supermassive Black Holes and Dark Matter Halos

Abstract

The possibility that the masses of supermassive black holes (SBHs) correlate with the total gravitational mass of their host galaxy, or the mass of the dark matter halo in which they presumably formed, is investigated using a sample of 16 spiral and 20 elliptical galaxies. The bulge velocity dispersion, typically defined within an aperture of size less than 0.5 kpc, is found to correlate tightly with the galaxy's circular velocity, the latter measured at distances from the galactic center at which the rotation curve is flat, 20 to 80kpc. By using the well known M-sigma relation for SBHs, and a prescription to relate the circular velocity to the mass of the dark matter halo in a standard CDM cosmology, the correlation between velocity dispersion and circular velocity is equivalent to one between SBH and halo masses. Such a correlation is found to be nonlinear, with the ratio between the two masses decreasing from 2X10^-4 for halos of 10^14 solar masses, to 10^-5 for halos of 10^12 solar masses. Preliminary evidence suggests that halos smaller than ~5X10^11 solar masses are increasingly less efficient -- perhaps unable -- at forming SBHs.

The Astrophysical Journal, accepted (October 10 2002 issue)

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• Quashing a suspected selection bias in galaxy samples having dynamically-measured supermassive black holes
• Black holes and the absorption rate of cosmological scalar fields
• Evolution of Supermassive Black Holes from Cosmological Simulations
• Super-Massive Black Holes and Dark Halos
• Growth of Intermediate Massive Black Holes in the Hierarchical Formation of Small Spiral Galaxies in the High-z Universe
• Constraints On Duty Cycles Of Quasars At Z $\sim$ 6
• Relativistic corrections to the rotation curves of disk galaxies
• Episodic activities of supermassive black holes at redshift $z\le 2$: driven by mergers?
• Linking X-ray AGN with dark matter halos: a model compatible with AGN luminosity function and large-scale clustering properties
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Shining Light on Merging Galaxies I: The Ongoing Merger of a Quasar with a `Green Valley' Galaxy
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• Spectroscopic classification of a complete sample of astrometrically-selected quasar candidates using Gaia DR2
• On the Evolution of High-Redshift Active Galactic Nuclei
• Probing the growth of supermassive black holes at z>6 with LOFAR
• Do all QSOs have the same black hole mass?
• Black hole in a generalized Chaplygin-Jacobi dark fluid: shadow and light deflection angle
• The relation between globular cluster systems and supermassive black holes in spiral galaxies III. The link to the $M_{\bullet }-M_{\ast }$ correlation
• Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations
• On merger bias and the clustering of quasars
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• The v_c-sigma_c relation in low mass and low surface brightness galaxies
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Can fermionic dark matter mimic supermassive black holes?
• Strong lensing by subhalos in the dwarf-galaxy mass range I: Image separations
• Transonic galactic outflows in a dark matter halo with a central black hole and its application to the Sombrero galaxy
• SMBH Seeds: Model Discrimination with High Energy Emission Based on Scaling Relation Evolution
• Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
• Constraining the host galaxy halos of massive black holes from LISA event rates
• Cosmological Growth History of Supermassive Black Holes and Demographics in the High-z Universe : Do Lyman-Break Galaxies Have Supermassive Black Holes?
• Mission Design for the TAIJI misson and Structure Formation in Early Universe
• On the detectability of massive black hole merger eventsby LISA
• Dark halo microphysics and massive black hole scaling relations in galaxies
• Prospects for Observing High-redshift Radio-loud Quasars in the SKA Era: Paving the Way for 21-cm Forest Observations
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• Searching for AGN-driven Shocks in Galaxy Clusters
• Evolution of supermassive black holes
• Supermassive black holes from OASIS and SAURON integral-field kinematics
• Gravitational Waves from Massive Black Hole Mergers in ASTRID: Predictions for LISA
• Imaging fermionic dark matter cores at the center of galaxies
• Direct Gravitational Imaging of Intermediate Mass Black Holes in Extragalactic Halos
• Supernova-Neutrino-Boosted Dark Matter from All Galaxies
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Imprints of the super-Eddington accretion on the quasar clustering
• Cosmic reionization of hydrogen and helium: contribution from both mini-quasars and stars
• The role of scatter and satellites in shaping the large-scale clustering of X-ray AGN as a function of host galaxy stellar mass
• Detecting quasars at very high redshift with next generation X-ray telescopes
• Reionization Models Classifier using 21cm Map Deep Learning
• A new delivery route to Galactic Nuclei: Warm halo cloud impacts
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• The galactic spin of AGN galaxies
• Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
• Accretion discs onto supermassive compact objects: a portal to dark matter physics in active galaxies
• The cosmological constant and scale hierarchies with emergent gauge symmetries
• Low-redshift quasars in the SDSS Stripe 82 II: associated companion galaxies and signature of star formation
• Insights into the evolution of five isolated galaxies
• The impact of large-scale galaxy clustering on the variance of the Hellings-Downs correlation: numerical results
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics
• Gravitational waves of quasi-circular, inspiraling black hole binaries in an ultralight vector dark-matter environment
• Negative feedback effects on star formation history and cosmic reionization
• Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• QSO MUSEUM III: the circumgalactic medium in Ly$\alpha$ emission around 120 $z\sim 3$ quasars covering the SDSS parameter space. Witnessing the instantaneous AGN feedback on halo scales
• Supermassive black holes may be limited by the Holographic Bound
• Spatial Correlation of Massive Black Hole Mergers: Probing the Formation Mechanism and Reionization
• A study of the scaling relation $M_{\bullet }\propto R_e{\sigma }^3$ for supermassive black holes and an update of the corresponding theoretical model
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Black Hole Scaling Relations Are Not Biased by Selection Effects
• Cosmic spin and mass evolution of black holes and its impact
• Probing the mass relation between supermassive black holes and dark matter halos at high redshifts by gravitational wave experiments
• Signatures of AGN induced metal loss in the stellar population
• A STIS Atlas of CaII Triplet Absorption Line Kinematics in Galactic Nuclei
• Method for Determining AGN Accretion Phase in Field Galaxies
• Study of central intensity ratio of early-type galaxies from low density environment
• Merging history of massive galaxies at 3<z<6
• Star Formation Rates in [Ne V] 3426 Å Selected Active Galactic Nuclei: Evidence for a Decrease along the Main Sequence?
• The relation between circular velocity and central velocity dispersion in low surface brightness galaxies
• Holes within galaxies: the egg or the hen?
• Recoiling supermassive black holes in analytical and numerical galaxy potential
• The $M_{\bullet }-\sigma$ relation in spherical systems
• Radio continuum observations of the candidate supermassive black hole in the dwarf elliptical VCC128
• Prospects for CDM sub-halo detection using high angular resolution observations
• AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03
• Thermodynamics of self-gravitating fermions as a robust theory for dark matter halos: Stability analysis applied to the Milky Way
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release
• The contribution of non-central radio galaxies to AGN feedback in rich galaxy clusters
• Investigation of homogeneity and matter distribution on large scales using large quasar groups