This review covers the main aspects of black hole accretion disk theory. We begin with the
view that one of the main goals of the theory is to better understand the nature of black holes …

Coalescence of binary supermassive black holes (SBHs) would constitute the strongest
sources of gravitational waves to be observed by LISA. While the formation of binary SBHs …

We study super-Eddington accretion flows onto black holes using a global three-
dimensional radiation magneto-hydrodynamical simulation. We solve the time-dependent …

Deep within galaxies like the Milky Way, astronomers have found a fascinating legacy of
Einstein's general theory of relativity: supermassive black holes. Connected to the evolution …

We analyze a sample of optical light curves for 100 quasars, 70 of which have black hole
mass estimates. Our sample is the largest and broadest used yet for modeling quasar …

Super-Eddington Accretion Disks around Supermassive Black Holes - IOPscience This site
uses cookies. By continuing to use this site you agree to our use of cookies. To find out more …

We conduct global three-dimensional radiation magnetohydrodynamic simulations of the
inner regions of accretion flows around a 5× 10 8 M⊙ black hole, with mass accretion rates …

The quasi-steady structure of supercritical accretion flows around a black hole is studied
based on two-dimensional radiation-hydrodynamic (2D-RHD) simulations. The supercritical …

We examine the effects of density stratification on magnetohydrodynamic turbulence driven
by the magnetorotational instability in local simulations that adopt the shearing box …

We examine the electromagnetic and gravitational wave (GW) signatures of stellar-mass
compact objects (COs) spiraling into a supermassive black hole (extreme mass-ratio …