Magnetically Arrested Disk: An Energetically Efficient Accretion Flow
arXiv:astro-ph/0305029 · doi:10.1093/pasj/55.6.L69
Abstract
We consider an accretion flow model originally proposed by Bisnovatyi-Kogan & Ruzmaikin (1974), which has been confirmed in recent 3D MHD simulations. In the model, the accreting gas drags in a strong poloidal magnetic field to the center such that the accumulated field disrupts the axisymmetric accretion flow at a relatively large radius. Inside the disruption radius, the gas accretes as discrete blobs or streams with a velocity much less than the free-fall velocity. Almost the entire rest mass energy of the gas is released as heat, radiation and mechanical/magnetic energy. Even for a non-rotating black hole, the efficiency of converting mass to energy is of order 50% or higher. The model is thus a practical analog of an idealized engine proposed by Geroch and Bekenstein.
4 pages, 2 figure, new refs added, in print in PASJ
References in corpus (2)
Cited by in corpus (464)
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- Launching and Quenching of Black Hole Relativistic Jets at Low Accretion Rate
- The plunging region of a thin accretion disc around a Schwarzschild black hole
- On the efficiency of the Blandford-Znajek mechanism for low angular momentum relativistic accretion
- Deciphering the properties of the central engine in GRB collapsars
- Semi-analytic studies of accretion disk and magnetic field geometry in M87*
- A comprehensive X-ray view of the active nucleus in NGC 4258
- Time delays between radio and X-ray and between narrow radio bands of Sgr A* flares in the shock oscillation model
- A full relativistic thin disc -- the physics of the plunging region and the value of the stress at the ISCO
- Inertial range of magnetorotational turbulence
- Accretion disc winds in X-ray binaries
- Viscous torque in turbulent magnetized AGN accretion disks and its effects on EMRI's gravitational waves
- The Effects of Resolution on Black Hole Accretion Simulations of Jets
- Spectral Energy Distribution profiles from AGN accretion disc in multi-gap setup
- Interpreting MAD within multiple accretion regimes
- Black holes shielded by magnetic fields
- Modeling Hadronic Gamma-ray Emissions from Solar Flares and Prospects for Detecting Non-thermal Signatures from Protostars
- A simple analytical model of magnetic jets
- Inner Engine Shutdown from Transitions in the Angular Momentum Distribution in Collapsars
- Hot, cold, and multi-component accretion flows around supermassive black hole binaries
- Distinguishing compact objects in extreme-mass-ratio inspirals by gravitational waves
- The Origin of Radio Emission in Black Hole X-ray Binaries
- Effects of Spin on High-Energy Radiation from Accreting Black Holes
- Bubble in the Whale: Identifying the Optical Counterparts and Extended Nebula for the Ultraluminous X-ray Sources in NGC 4631
- A possible influence on standard model of quasars and active galactic nuclei in strong magnetic field
- Magnetic Field Strength Effects on Nucleosynthesis from Neutron Star Merger Outflows
- Probing magnetic fields with Square Kilometre array and its precursors
- The Study of Jet Formation Mechanism in Fermi Blazars
- Magnetic reconnection and Blandford-Znajek process around rotating black holes
- Constraining X-ray emission of magnetically arrested disk (MAD) by radio-loud AGNs with extreme ultraviolet (EUV) deficit
- Jet Tilt Instability from Stream-Disk Interactions in MAD Disks
- Global simulations of magnetorotational turbulence III: influence of field configuration and mass injection
- Helical and nonhelical large-scale dynamos in thin accretion discs
- Black hole outflows initiated by a large-scale magnetic field
- Tilted Accretion Disks
- The correlation between the total magnetic flux and the total jet power
- Jet Archaeology and Forecasting: Image Variability and Magnetic Field Configuration
- GRMHD simulations of black hole accretion variabilities: Implications to hard state X-ray binary transients
- Global resistive MHD accretion flows around spinning AGNs: impact of resistivity on MAD state
- Non-thermal Synchrotron Emission and Polarization Signatures during Black Hole Flux Eruptions
- On the Zeeman Effect in Magnetically-Arrested Disks
- Diverse Polarimetric Features of AGN Jets from Various Viewing Angles: Towards a Unified View
- Radio signals from early direct collapse black holes
- Viscous Evolution of Magnetized Clumps: a Source for X-ray Flares in Gamma-ray Bursts
- Development and Application of Numerical Techniques for General-Relativistic Magnetohydrodynamics Simulations of Black Hole Accretion
- Self-Gravity in Magnetized Neutrino-Dominated Accretion Discs
- Fast Transients from Magnetic Disks Around Non-Spinning Collapsar Black Holes
- Current Status of Simulations
- Magnetically Driven Relativistic Jet in the High-Redshift Blazar OH~471
- Binary black holes in magnetized AGN disks
- Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
- Time-domain Radio-loudness of Active Galactic Nuclei: Intermittency, Memory, and Jet Escape
- Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks
- A general relativistic magnetohydrodynamics extension to mesh-less schemes in the code GIZMO
- Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
- MAD-Accretion Scenario in High-Mass X-Ray Binaries with Neutron Stars
- Magnetically arrested transmutation of a compact star
- A magnetic model for low/hard state of black hole binaries
- On the universality of the split monopole black hole magnetosphere
- Explaining the 'outliers' track in Black Hole X-ray Binaries with the BZ-jet and inner-disk coupling
- Atacama Cosmology Telescope: Observations of supermassive black hole binary candidates. Strong sinusoidal variations at 95, 147 and 225 GHz in PKS 2131021 and PKS J08050111
- Algorithms and radiation dynamics for the vicinity of black holes I. Methods and codes
- State transitions triggered by inverse magnetic field: probably applied in high-mass X-ray binaries?
- Jet MHD analytical model - framework for radiative transfer
- Extreme magnetic fields around black holes
- Transverse Oscillations and Wave Propagation in the Magnetically Dominated M87 Jet
- Binary black holes gone MAD: Magnetically arrested minidisks around nonspinning black holes
- The Core-shift of Sagittarius A* as a Discriminant between Disk and Jet Emission Models with millimeter-VLBI
- Three-dimensional GRMHD simulations of jet formation and propagation in self-gravitating collapsing stars
- Impacts of radiative cooling on the images of a black hole shadow and extended jets in two-temperature GRMHD simulations
- Exploring the Role of Vector Potential and Plasma- in Jet Formation from Magnetized Accretion Flows
- Millimeter VLBI constraints on the central magnetic field and symmetric jet production in the twin-jet galaxy NGC 1052
- Dynamics of magnetoviscous warped discs around compact objects
- Universality in quasinormal modes of a magnetized black hole
- The dependence of the fraction of radio luminous quasars on redshift and its theoretical implications
- Dynamical Unification of Tidal Disruption Events
- Parameter Inference of Black Hole Images using Deep Learning in Visibility Space
- Investigating the Disk-Jet Structure in M87 through Flux Separation in the Linear and Circular Polarization Images
- Photon Ring Symmetries in Simulated Linear Polarization Images of Messier 87*
- A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations
- PATOKA: Simulating Electromagnetic Observables of Black Hole Accretion
- Prompt and Afterglow Constraints on the Central Engine of GRB 240825A
- Dirty waveforms: multiband harmonic content of gas-embedded gravitational wave sources
- Accretion in Active Galactic Nuclei
- Accretion into black hole, and formation of magnetically arrested accretion disks
- A revised view of the linear polarization in the subparsec core of M87 at 7 mm
- The High-energy emission of jetted AGN
- Interpreting Swift and NuSTAR Observations of the Low-Luminosity Active Galactic Nucleus NGC 4278 with Radiatively Inefficient Accretion Flows and Implications for Neutrino Emission
- GRRMHD Simulations of State Transitions in Non-Jetted Tidal Disruption Events
- Observational distinguishability of the Kerr and Kerr-Hayward metrics to EHT
- The azimuthal structure of magnetically arrested disks during flux eruption events
- GRMHD Simulations of Magnetized Accretion Disk/Jet: Variabilities of Black Holes and Spectral Energy Distributions in Magnetic States