2 citations · 2 across the 6 of their papers we have counts for
6 papers
Poloidal Field Amplification through Compression-Shear Dynamics in Schwarzschild Accretion: Pathways to MAD States
Malihe Mousapour Gharghabi, Jamshid Ghanbari, Mahboobe Moeen Moghaddas
The amplification of magnetic fields in black hole accretion flows governs key high-energy phenomena such as magnetically arrested disks and relativistic jets. We develop a semi-an…
A Study of thin relativistic magnetic accretion disk around a distorted black hole
Seyyed Masoud Hoseyni, Jamshid Ghanbari, Mahboobe Moeen Moghaddas
Accretion disks, swirling structures of matter spiraling into black holes, play a pivotal role in our understanding of binary star systems and their intricate evolutionary processe…
A Study of thin relativistic viscose accretion disk around a distorted kerr black hole (DKB)
Olya Layeghi, Jamshid Ghanbari, Mahboobe Moeen Moghaddas
In this paper, we analyze a thin disk around the distorted Kerr black hole (DKB) within the framework of general relativity using an axisymmetric solution of the Einstein equations…
Energy-momentum tensor of special relativistic fluids and Connection of relativistic and non-relativistic fluids in the new scaling
Mahboobe Moeen Moghaddas
In this paper, the relativistic fluids with the negligible magnetic field in the flat metric are studied. The iso-dimension scale in introduced, in this scale, all similar componen…
Calculation of the relativistic Bulk Viscosity, Shear Viscosity and Shear-Stress Viscosity of Accretion Disks around the Rotating Black Holes
Mahboobe Moeen Moghaddas
In this paper we study the relativistic bulk tensor, shear tensor and the shear stress viscosity of the relativistic accretion disks around the rotating black holes. we calculate a…
Shear tensor and dynamics of relativistic accretion disks around rotating black holes
Mahboobe Moeen Moghaddas, Jamshid Ghanbari, Ahmad Ghodsi
In this paper we solve the hydrodynamical equations of optically thin, steady state accretion disks around Kerr black holes. Here, fully general relativistic equations are used. We…