Dark matter effect on black hole accretion disks

Abstract

Comparing different dark matter (DM) models, we explore the DM influence on black hole (BH) accretion disk physics, considering corotating and counterrotating thick accretion tori orbiting a central spinning BH. Our results identify accretion onto a central BH as a good indicator of DM presence, signaling possible DM tracers in accretion physics. We analyze accretion around a spinning BH immersed in perfect-fluid dark matter, cold dark matter and scalar field dark matter. Our investigation addresses observational evidence of distinctive DM effects on toroidal accretion disks and protojet configurations, proving that BH accretion tori immersed in DM can present characteristics, such as interdisk cusp or double tori, which have usually been considered as tracers for superspinars and naked singularity attractors. Therefore, in this context DM influence on the BH geometry could manifest as superspinar mimickers. DM also affects the central spinning attractor energetics associated with accretion physics, and its influence on accretion disks can be searched for in a variation of the central BH energetics as an increase of the mass accretion rates.

References in corpus (50)

• Foundations of Black Hole Accretion Disk Theory
• Global General Relativistic MHD Simulation of a Tilted Black-Hole Accretion Disk
• The Black Hole Accretion Code
• Dark matter distributions around massive black holes: A general relativistic analysis
• Two-dimensional models of hydrodynamical accretion flows into black holes
• Black Hole Surrounded by a Dark Matter Halo in the M87 Galactic Center and its Identification with Shadow Images
• Three-Dimensional Simulations of Magnetized Thin Accretion Disks around Black Holes: Stress in the Plunging Region
• Reconstructing the Last Major Merger of the Milky Way with the H3 Survey
• Quasinormal Modes of Black Holes Surrounded by Dark Matter and Their Connection with the Shadow Radius
• Off the baryonic Tully-Fisher relation: a population of baryon-dominated ultra-diffuse galaxies
• Black Hole Space-time In Dark Matter Halo
• Black Hole Shadow of Sgr A${}^{\ast }$ in Dark Matter Halo
• Rotating Black Hole Shadow in Perfect Fluid Dark Matter
• Galactic Dark Matter in the Phantom Field
• Equatorial circular motion in Kerr spacetime
• Influence of the relict cosmological constant on accretion discs
• Search for topological defect dark matter with a global network of optical magnetometers
• Shadows of Sgr A${}^{\ast }$ Black Hole Surrounded by Superfluid Dark Matter Halo
• $S^5$: The Orbital and Chemical Properties of One Dozen Stellar Streams
• All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data
• General relativistic polytropes with a repulsive cosmological constant
• Perfect Fluid Dark Matter
• Equatorial photon motion in the Kerr-Newman spacetimes with a non-zero cosmological constant
• Kerr-Anti-De-Sitter/De-Sitter Black Hole In Perfect Fluid Dark Matter Background
• On the stability of thick accretion disks around black holes
• On the growth of massive scalar hair around a Schwarzschild black hole
• Direct limits on the interaction of antiprotons with axion-like dark matter
• Exploring the high-redshift PBH-$\Lambda$CDM Universe: early black hole seeding, the first stars and cosmic radiation backgrounds
• Constraints on compact dark matter from gravitational wave microlensing
• Investigation of circular geodesics in a rotating charged black hole in the presence of perfect fluid dark matter
• Efficiency of the Keplerian accretion in the Braneworld Kerr--Newman Spacetimes and mining instability of some naked singularity spacetimes
• Ringed accretion disks: equilibrium configurations
• Three-Dimensional Hydrodynamic Simulations of Accretion Tori in Kerr Spacetimes
• Core-Halo Mass Relation in Scalar Field Dark Matter Models and its Consequences for the Formation of Supermassive Black Holes
• Growth of accretion driven scalar hair around Kerr black holes
• Unique probe of dark matter in the core of M87 with the Event Horizon Telescope
• Ringed accretion disks: instabilities
• Rotating black holes with an anisotropic matter field
• On the Polish doughnut accretion disk via the effective potential approach
• Relativistic thick accretion disks: morphology and evolutionary parameters
• Superradiance and Stability of Kerr Black Hole Enclosed by Anisotropic Fluid Matter
• Connecting the Extremes: A Story of Supermassive Black Holes and Ultralight Dark Matter
• Proto-jets configurations in RADs orbiting a Kerr SMBH: symmetries and limiting surfaces
• RADs energetics and constraints on emerging tori collisions around super-massive Kerr Black Holes
• Relating Kerr SMBHs in Active Galactic Nuclei to RAD configurations
• Squeezing of toroidal accretion disks
• Stellar Shocks From Dark Matter Asteroid Impacts
• When Leaving the Solar System: Dark Matter Makes a Difference
• Dragged surfaces. On the accretion tori in the ergoregion
• Jet collision with accreting tori around SMBHs. GRHD and light surfaces constraints in aggregates of misaligned tori

Cited by in corpus (7)

• Observational constraints on a logarithmic scalar field dark energy model and black hole mass evolution in the Universe
• Black hole surrounded by the pseudo-isothermal dark matter halo
• Energy extraction from Janis-Newman-Winicour naked singularity
• Seeing dark matter via acceleration radiation
• Accreting Black Holes in Dark Matter Halos
• Topological dyonic black holes of massive gravity with generalized quasitopological electromagnetism
• Observational constraints on the Kerr and its several single-parameter modified spacetimes using quasi-periodic oscillation data