scholarly journals General Relativistic Magnetohydrodynamic Simulations of Black Hole Accretion Disks: Results and Observational Implications

2004 ◽  
Vol 155 ◽  
pp. 140-147 ◽  
Author(s):  
Julian H. Krolik ◽  
Shigenobu Hirose
Keyword(s):  
Black Hole ◽  
Accretion Disks ◽  
Black Hole Accretion ◽  
General Relativistic ◽  
Magnetohydrodynamic Simulations ◽  
Hole Accretion

scholarly journals The effects of resolution on black hole accretion simulations of jets

2020 ◽  
Vol 498 (2) ◽  
pp. 2428-2439
Author(s):  
Christopher J White ◽  
Fiona Chrystal
Keyword(s):  
Black Hole ◽  
Velocity Structure ◽  
Grid Resolution ◽  
Black Hole Accretion ◽  
General Relativistic ◽  
Axisymmetric Structure ◽  
Magnetohydrodynamic Simulations ◽  
Jet Power ◽  
Hole Accretion

ABSTRACT We perform three general-relativistic magnetohydrodynamic simulations of black hole accretion designed to test how sensitive results are to grid resolution in the jet region. The cases differ only in numerics, modelling the same physical scenario of a radiatively inefficient, geometrically thick, magnetically arrested flow on to a rapidly spinning black hole. Properties inferred with the coarsest grid generally agree with those found with higher resolutions, including total jet power and its decomposition into different forms, velocity structure, non-axisymmetric structure, and the appearance of resolved millimetre images. Some measures of variability and magnetization are sensitive to resolution. We conclude that most results obtained by limiting resolution near the jet for computational expediency should still be reliable, at least in so far as they would not be improved with a finer grid.

scholarly journals High-Frequency QPOs and Overstable Oscillations of Black-Hole Accretion Disks

2012 ◽  
Vol 8 (S290) ◽  
pp. 57-61 ◽  
Author(s):  
Dong Lai ◽  
Wen Fu ◽  
David Tsang ◽  
Jiri Horak ◽  
Cong Yu
Keyword(s):  
Black Hole ◽  
Accretion Disks ◽  
High Frequency ◽  
Oscillation Mode ◽  
Relativistic Effects ◽  
X Ray ◽  
Black Hole Accretion ◽  
General Relativistic ◽  
X Ray Binaries ◽  
Hole Accretion

AbstractThe physical origin of high-frequency QPOs (HFQPOs) in black-hole X-ray binaries remains an enigma despite many years of detailed observational studies. Although there exists a number of models for HFQPOs, many of these are simply “notions” or “concepts” without actual calculation derived from fluid or disk physics. Future progress requires a combination of numerical simulations and semi-analytic studies to extract physical insights. We review recent works on global oscillation modes in black-hole accretion disks, and explain how, with the help of general relativistic effects, the energy stored in the disk differential rotation can be pumped into global spiral density modes in the disk, making these modes grow to large amplitudes under certain conditions (“corotational instability”). These modes are robust in the presence of disk magnetic fields and turbulence. The computed oscillation mode frequencies are largely consistent with the observed values for HFQPOs in BH X-ray binaries. The approximate 2:3 frequency ratio is also expected from this model. The connection of HFQPOs with other disk properties (such as production of episodic jets) is also discussed.

General relativistic MHD simulations of black hole accretion disks and jets

2007 ◽  
Vol 311 (1-3) ◽  
pp. 117-125 ◽  
Author(s):  
John F. Hawley ◽  
Kris Beckwith ◽  
Julian H. Krolik
Keyword(s):  
Black Hole ◽  
Accretion Disks ◽  
Black Hole Accretion ◽  
Mhd Simulations ◽  
General Relativistic ◽  
Hole Accretion

Iron Fluorescence from within the Innermost Stable Orbit of Black Hole Accretion Disks

1997 ◽  
Vol 488 (1) ◽  
pp. 109-118 ◽  
Author(s):  
Christopher S. Reynolds ◽  
Mitchell C. Begelman
Keyword(s):  
Black Hole ◽  
Accretion Disks ◽  
Stable Orbit ◽  
Black Hole Accretion ◽  
Hole Accretion
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