Accretion Onto Supermassive Black Hole Binaries
In this chapter, we give an overview of our current understanding of the physics of accreting massive black hole binaries (MBHBs), with a special focus on the latest developments in numerical simulations and General-Relativistic Magnetohydrodynamics (GRMHD) simulations in particular.
Gutiérrez, Eduardo M. +2 more
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Stellar Black Holes Can “Stretch” Supermassive Black Hole Accretion Disks
Abstract Stellar black holes (sBHs) are widely believed to exist in the accretion disks of active galactic nuclei (AGNs). Previous studies often focus on the transient emission produced by embedded sBHs. Here, we explore the possible observational consequences of an AGN accretion disk that contains a population of accreting sBHs ...
Shuying Zhou +5 more
openaire +3 more sources
Probing black holes in a dark matter spike of M87 using quasinormal modes
Dark matter density can be significantly enhanced by the supermassive black hole at the galactic center, leading to a structure called dark matter spike. Dark matter spike may change the spacetime properties of black holes that constitute deviations from
Dong Liu, Yi Yang, Zheng-Wen Long
doaj +1 more source
Simulating ULXs and Blazars as GRMHD Accretion Flows Around a Black Hole
General relativistic magnetohydrodynamic (GRMHD) simulations have been instrumental in our understanding of high-energy astrophysical phenomena over the past two decades.
Mayank Pathak, Banibrata Mukhopadhyay
doaj +1 more source
Time delay of light in the gravitational lensing of supermassive black holes in dark matter halos
The dark matter halo has non-negligible effects on the gravitational lensing of supermassive black hole in the galaxy center. Our work presents a study on the time-delay of light in gravitational lensing of black holes enclosed by dark matter halos.
Chen-Kai Qiao, Ping Su
doaj +1 more source
Cosmological evolution of supermassive black holes in galactic centers unveiled by hard X-ray observations. [PDF]
Ueda Y.
europepmc +1 more source
Using of the Correction Schwarzschild radius Equation and Its Application of the Black Holes
This study is a try to compare between the traditional Schwarzschild’s radius and the equation of Schwarzschild’s radius including the photon’s wavelength that is suggested by Kanarev for black holes to correct the error in the calculation of ...
Majida H. Al-kubaisy
doaj
"Fermi" bubbles are bursting from our galaxy. Their origins remain a mystery. [PDF]
Mann A.
europepmc +1 more source
Little red dots as young supermassive black holes in dense ionized cocoons. [PDF]
Rusakov V +16 more
europepmc +1 more source
Reading signatures of supermassive binary black holes in pulsar timing array observations. [PDF]
Goncharov B +12 more
europepmc +1 more source

