Thermal Equilibria of Accretion Disks

Abstract

We show that most of hot, optically thin accretion disk models which ignore advective cooling are not self-consistent. We have found new types of optically thin disk solutions where cooling is dominated by radial advection of heat. These new solutions are thermally and viscously stable.

Submitted to ApJL July 1994. PS file, 8 Pages; 3 Figs available upon request

Cited by in corpus (438)

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• X-ray Dip Monitoring of XB 1916-053
• A non-linear mathematical model for the X-ray variability classes of the microquasar GRS 1915+105 -- I: quiescent, spiking states and QPOs
• A quantitative explanation of the radio--X-ray correlation in black-hole X-ray binaries
• Observational Constraints on Direct Electron Heating in the Hot Accretion Flows in Sgr A* and M87*
• Vertical structure of Advection dominated Accretion Flows
• Two-dimensional Inflow-Wind Solution of Hot Accretion Flow. I. Hydrodynamics
• Advection-dominated accretion flow for the varied transition luminosities in black hole X-ray binaries
• Self-similar solutions of viscous and resistive ADAFs with thermal conduction
• Exploring higher order images with Fe K_α-lines from relativistic disks: black hole spin determination and bias
• Effects of wind on radiation spectra from magnetized accretion disks
• Exact analytical solutions for ADAFs
• A toy model for X-ray spectral variability of active galactic nuclei
• Enhanced gamma radiation toward the rotation axis from the immediate vicinity of extremely rotating black holes
• Nucleosynthesis in the accretion disks of Type II collapsars
• FUSE Spectroscopy of the Accreting Hot Components in Symbiotic Variables
• Dynamics of accretion and winds in tidal disruption events
• Radio Dichotomy in Quasars with H$\beta$ FWHM greater than $15,000$ km\,s${}^{-1}$
• Accretion flows with comparable radiation and gas pressures
• A two-fluid model for black-hole accretion flows: particle acceleration and disc structure
• The influence of outflow in supercritical accretion flows
• On the sub-parsec scale core composition of FR 0 radio galaxies
• Spectral Energy Distribution profiles from AGN accretion disc in multi-gap setup
• Angular momentum transport and thermal stabilization of optically thin, advective accretion flows through large-scale magnetic fields
• The advection-dominated accretion flow for the anti-correlation between the X-ray photon index and the X-ray luminosity in neutron star low-mass X-ray binaries
• Line profile of nuclear de-excitation gamma-ray emission from very hot plasma
• Magnetic Coupling of a Rotating Black Hole with Advection-Dominated Accretion Flows
• Global structure and dynamics of slowly rotating accretion flows
• Effect of generic dark matter halo on transonic accretion onto galactic black holes
• A combined model for the X-ray to gamma-ray emission of Cyg X-1
• Variation of the gas and radiation content in the sub-Keplerian accretion disk around black holes and its impact to the solutions
• On the Relative Surface Density Change of Thermally Unstable Accretion Disks
• Viscosity-Driven Winds from Magnetized Accretion Disks
• Hydrodynamical wind on magnetized Accretion Flows with Convection
• Could an X-ray Flare after GRB 170817A Originate from a Post-merger Slim Accretion Disc?
• Modeling the Spectrum of IGR J17177-3656
• Nuclear $\gamma$-ray emission from very hot accretion flows
• X-Ray Lines from Hot Flows around White Dwarfs. Application to SS Cygni
• Accretion Disc-Jet Couplings in X-ray Binaries
• Two Physically Distinct Populations of Low-Ionization Nuclear Emission-Line Regions
• Two Types of Magnetohydrodynamic Sheath Jets
• Pion production in the inner disk around Cygnus X-1
• On the double natured solutions to the two-temperature external soft photon comptonized accretion disks
• XMM-Newton observation of V1504 Cyg as a probe for the existence of an evaporated corona
• Is the energy generation rate of nuclear reactions in hot accretion flows important?
• Global Neutrino Heating in Hyperaccretion Flows
• Effect of magnetic flux advection on the dynamics of shock in accretion flow around a rotating black hole
• Heating or Cooling: Study of Advective Heat Transport in the Inflow and the Outflow of Optically Thin Advection-dominated Accretion Flows
• Advective accretion disc-corona model with fallback for tidal disruption events
• Effect of Magnetic Field on the Formation of Radiatively Inefficient Accretion Flow around Black Holes
• Iron Line Tomography of General Relativistic Hydrodynamic Accretion around Kerr Black Holes
• Extracting common signal components from the X-ray and optical light curves of GX 339-4: new view for anti-correlation
• The peculiar disk evolution of 4U 1630--472 observed by Insight-HXMT during the 2022 and 2023 outbursts
• Appearance of Jet-Driving Poynting Flux in Hot, Tenuous Accretion Disks Threaded by an Ordered Magnetic Field
• Photometric Constraints on Intermediate-mass Black Holes in the Galactic Centre
• Generalized thermal instability criterion of black hole accretion disks
• Interaction between disk and extended corona in a general relativistic framework
• HOLESOM: Constraining the Properties of Slowly-Accreting Massive Black Holes with Self-Organizing Maps
• Self-Similar Solutions for Viscous and Resistive ADAF
• GRRMHD Simulations of State Transitions in Non-Jetted Tidal Disruption Events
• A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations
• Fast giant flares in discs around supermassive black holes
• Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius