Supermassive black holes in scalar field galaxy halos
arXiv:astro-ph/0207493 · doi:10.1103/PhysRevD.66.083005
Abstract
Ultra-light scalar fields provide an interesting alternative to WIMPS as halo dark matter. In this paper we consider the effect of embedding a supermassive black hole within such a halo, and estimate the absorption probability and the accretion rate of dark matter onto the black hole. We show that the accretion rate would be small over the lifetime of a typical halo, and hence that supermassive central black holes can coexist with scalar field halos.
5 pages RevTex4, no figures. Updated file to match published version
Cited by in corpus (50)
- Dark Matter and Dark Energy
- Black hole mass decreasing due to phantom energy accretion
- Galactic Halos of Fluid Dark Matter
- The Accretion of Dark Energy onto a Black Hole
- Newtonian Collapse of Scalar Field Dark Matter
- Schwarzschild black holes can wear scalar wigs
- Are black holes a serious threat to scalar field dark matter models?
- Black holes in the presence of dark energy
- Extreme Dark Matter Tests with Extreme Mass Ratio Inspirals
- Modelling galaxy halos using dark matter with pressure
- Constraining scalar fields with stellar kinematics and collisional dark matter
- Are galaxies extending?
- Schwarzschild scalar wigs: spectral analysis and late time behavior
- Short Review of the main achievements of the Scalar Field, Fuzzy, Ultralight, Wave, BEC Dark Matter model
- Modelling the rotational curves of spiral galaxies with a scalar field
- Parasitic black holes: the swallowing of a fuzzy dark matter soliton
- Gravitational lens optical scalars in terms of energy-momentum distributions
- Scalar Field Dark Matter: behavior around black holes
- Bounds on Ultralight Dark Matter from NANOGrav
- Anisotropic k-essence cosmologies
- Self-gravitating black hole scalar wigs
- Effective field theory for black holes with induced scalar charges
- Slowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime
- On the Possibility that Ultra-Light Boson halos host and form Super-massive Black Holes
- Spherical non-linear absorption of cosmological scalar fields onto a black hole
- Evolution of spherical perturbations in the cosmological environment of degenerate scalarly charged fermions with the Higgs scalar interaction
- Single-field model of gravitational-scalar instability. I. Evolution of perturbations
- Bondi-Hoyle-Lyttleton accretion onto a rotating black hole with ultralight scalar hair
- Boson-fermion stars: exploring different configurations
- Constraining Self-interacting Scalar Field Dark Matter From the Black Hole Shadow of the Event Horizon Telescope
- Lorentzian wormhole in the framework of loop quantum cosmology
- Black holes and the absorption rate of cosmological scalar fields
- Gravitational waves from scalar field accretion
- Formation of supermassive nuclei of Black holes in the early Universe by the mechanism of scalar-gravitational instability. I. Local picture
- Gravitational - Scalar Instability of a Two-Component Degenerate System of Scalar Charged Fermions with Asymmetric Higgs Interaction
- Evolution of plane perturbations in the cosmological environment of the Higgs scalar field and an ideal scalar charged fluid
- Cosmological evolution of a statistical system of degenerate scalar charged fermions with an asymmetric scalar doublet. II. One-component system of doubly charged fermions
- The M-sigma Relation of Super Massive Black Holes from the Scalar Field Dark Matter
- Gravitational atoms beyond the test field limit: The case of Sgr A* and ultralight dark matter
- The quantum character of the Scalar Field Dark Matter
- Accretion of a Phantom Scalar Field by a Black Hole: restrictions on the field distribution
- Gravastar in the framework of Loop Quantum Cosmology
- Interplay between Black Holes and Ultralight Dark Matter: Analytic Solutions
- Evolution of spherical perturbations in the cosmological environment of the Higgs scalar field and an ideal scalar charged fluid
- Gravitational-Scalar Instability of a Cosmological Model Based on a Two-Component System of Degenerate Scalarly Charged Fermions with Asymmetric Higgs Interaction. I. Equations for Perturbations
- A novel model of non-singular oscillating cosmology on flat Randall-Sundrum II braneworld
- Self-gravitating Higgs field of scalar charge. II. Asymmetric scalar doublet
- Galaxies with Fuzzy Dark Matter
- A Natural Explanation of the VPOS from Multistate Scalar Field Dark Matter
- Frequency shift of light emitted from growing and shrinking black holes