Three Dimensional Simulations of Advective, Sub-Keplerian Accretion Flow onto Non-rotating Black Holes
arXiv:2212.08310 · doi:10.1093/mnras/stac3736
Abstract
We study the time evolution of sub-Keplerian transonic accretion flow onto a non-rotating black hole using a three-dimensional, inviscid hydrodynamics simulation code. Prior two-dimensional simulations show that centrifugal barrier in the accreting matter may temporarily halt the nearly free-falling matter and produce a stable, geometrically thick disk which may contain turbulent eddies. Our goal in this work is to investigate whether the disk develops any instability because of this turbulence when we dynamically activate all three dimensions. We find that the disk remains stable and axisymmetric even close to the central black hole. However, if we explicitly apply non-axisymmetric azimuthal perturbation, the axisymmetric structure of the disk is destroyed and instability is developed.
arXiv comment15 pages, 15 figures, accepted in MNRAS
References in corpus (44)
- Spectral Properties of Accretion Disks Around Galactic and Extragalactic Black Holes
- The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project
- The Black Hole Accretion Code
- Resonance Oscillation Of Radiative Shock Waves In Accretion Disks Around Compact Objects
- The Spherical Accretion Shock Instability in the Linear Regime
- Temporal Properties of Cygnus X-1 During the Spectral Transitions
- Correlation among QPO frequencies and Quiescence-state Duration in Black Hole Candidate GRS 1915+105
- High-order conservative reconstruction schemes for finite volume methods in cylindrical and spherical coordinates
- Zero Energy Rotating Accretion Flows near a Black Hole
- Accretion Processes On a Black Hole
- Simulation of Thick Accretion Disks with Standing Shocks by Smoothed Particle Hydrodynamics
- Smoothed Particle Hydrodynamics Confronts Theory: Formation of Standing Shocks in Accretion Disks and Winds Around Black Holes
- Numerical Simulations of Standing Shocks in Accretion Flows around Black Holes: A Comparative Study
- The effect of cooling on time dependent behaviour of accretion flows around black holes
- Effect of Rotation on the Stability of a Stalled Cylindrical Shock and its Consequences for Core-Collapse Supernovae
- Hydrodynamic Simulation of Two Component Advective Flows around Black Holes
- Smoothed Particle Hydrodynamic Simulations of Viscous Accretion Discs Around Black Holes
- Evolution of X-Ray Properties of MAXI J1535-571: Analysis with the TCAF Solution
- Three-Dimensional Simulations of Dynamics of Accretion Flows Irradiated by a Quasar
- Stable and Unstable Accretion Flows with Angular Momentum near a Point Mass
- Shocks in the relativistic transonic accretion with low angular momentum
- General Relativistic Hydrodynamic Simulations and Linear Analysis of the Standing Accretion Shock Instability around a Black Hole
- On the Azimuthal Stability of Shock Waves around Black Holes
- Oscillating shocks in the low angular momentum flows as a source of variability of accreting black holes
- Quasi Periodic Oscillations in a Radiative Transonic Flow: Results of a Coupled Monte Carlo-TVD Simulation
- Simulations of Viscous Accretion Flow around Black Holes in Two-Dimensional Cylindrical Geometry
- Effects of Compton Cooling on Outflow in a Two Component Accretion Flow around a Black Hole: Results of a Coupled Monte Carlo-TVD Simulation
- Shock oscillation model for QPOs in stellar-mass and supermassive black holes
- SWIFT view of the 2015 outburst of GS 2023+338 (V404 Cyg): complex evolution of spectral and temporal characteristics
- The Standing Accretion Shock Instability in the Disk around the Kerr Black Hole
- Model Dependence of Transonic Properties of Accretion Flows Around Black Holes
- General Relativistic Numerical Simulation of sub-Keplerian Transonic Accretion Flows onto Rotating Black Holes: Kerr Spacetime
- A Possible Model for the Long-Term Flares of Sgr A*
- Segregation of a Keplerian disc and sub-Keplerian halo from a Transonic flow around a Black Hole by Viscosity and Cooling processes
- General Relativistic Numerical Simulation of sub-Keplerian Transonic Accretion Flows onto Black Holes: Schwarzschild Spacetime
- Time Evolution of the 3-D Accretion Flows: Effects of the Adiabatic Index and Outer Boundary Condition
- Nonaxisymmetric Effects in the Black Hole Accretion Inviscid Hydrodynamics: Formation and Evolution of a Tilted Torus
- Monte-Carlo Simulations of Thermal Comptonization Process in a Two Component Accretion Flow Around a Black Hole in presence of an Outflow
- Evidence of Outflow Induced Soft Lags of Galactic Black Holes
- Effects of Magnetic Field Loops on the Dynamics of Advective Accretion Flows and Jets around a Schwarzschild Blackhole
- Effects of resistivity on standing shocks in low angular momentum flows around black holes
- Dynamics of Magnetic Flux Tubes in an Advective Flow around a Black Hole
- Numerical Simulation of Vertical Oscillations in an Axisymmetric Thick Accretion Flow around a Black Hole
- Spectral signature of mass outflow in Two Component Advective Flow Paradigm
Cited by in corpus (6)
- General relativistic hydrodynamic simulations of perturbed transonic accretion
- The implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism
- Spectral and Temporal Studies of Swift\,J1658.2--4242 using {\it AstroSat} Observations with {\tt JeTCAF} Model
- Implications of post-kick jets in core collapse supernovae
- On the nature of jets from a main sequence companion at the onset of common envelope evolution
- The azimuthal structure of magnetically arrested disks during flux eruption events