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20092021
most citedHydrodynamic Simulation of Two Component Advective Flows around Black Holes

75 citations · 258 across the 12 of their papers we have counts for

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11 papers · 1 filter

astro-ph.HE2019

Higher Order Stability Analysis for Astrophysical Accretion Processes

Sayan Kundu, Kinsuk Giri

We have done nth order perturbation analysis of the Navier-Stokes equation with the presence of turbulent viscosity in context of thin accretion flow around a black hole. In order…

astro-ph.HE2017★ 8 cited

Dynamics of Magnetic Flux Tubes in an Advective Flow around a Black Hole

Arnab Deb, Kinsuk Giri, Sandip K. Chakrabarti

Entangled magnetic fields entering into an accretion flow would very soon be stretched into a dominant toroidal component due to strong differentially rotating motion inside the ac…

astro-ph.HE2016★ 6 cited

Numerical Simulation of Vertical Oscillations in an Axisymmetric Thick Accretion Flow around a Black Hole

Arnab Deb, Kinsuk Giri, Sandip K Chakrabarti

We study time evolution of rotating, axisymmetric, two dimensional inviscid accretion flows around black holes using a grid based finite difference method. We do not use reflection…

astro-ph.HE2015★ 25 cited

Segregation of a Keplerian disc and sub-Keplerian halo from a Transonic flow around a Black Hole by Viscosity and Cooling processes

Kinsuk Giri, Sudip K. Garain, Sandip K. Chakrabarti

A black hole accretion is necessarily transonic. In presence of sufficiently high viscosity and cooling effects, a low-angular momentum transonic flow can become a standard Kepleri…

astro-ph.HE2015

Effects of Turbulent Viscosity on A Rotating Gas Ring Around A Black Hole: Results in Numerical Simulation

Kinsuk Giri, Hsiang-Kuang Chang

In this paper, we present the time evolution of a rotationally axisymmetric gas ring around a non rotating black hole using two dimensional grid-based hydrodynamic simulation. We s…

astro-ph.HE2014

Numerical Simulations of a Two Component Advective Flow for The Study of the Spectral and Timing Properties of Black Holes

Kinsuk Giri, Sandip K. Chakrabarti

Two component advective flows are the most physical accretion disks which arise from theoretical consideration. Since viscosity is the determining factor, we investigate the effect…

astro-ph.HE2013

Role of Viscosity and Cooling in Hydrodynamic Simulation of Two Component Accretion Flow (TCAF) around Black Holes

Kinsuk Giri, Sandip K. Chakrabarti

We carry out numerical simulation of accretion flows around a black hole in presence of both viscous and cooling effects. Instead of using a constant parameter throughout the s…

astro-ph.HE2012★ 75 cited

Hydrodynamic Simulation of Two Component Advective Flows around Black Holes

Kinsuk Giri, Sandip K. Chakrabarti

We carry out a series of numerical simulations of viscous accretion flows having a reasonable spatial distribution of the viscosity parameter. We add the power-law cooling througho…

astro-ph.HE2011★ 24 cited

Hydrodynamic simulations of viscous accretion flows around black holes

Kinsuk Giri, Sandip K. Chakrabarti

We study the time evolution of a rotating, axisymmetric, viscous accretion flow around black holes using a grid based finite difference method. We use the Shakura-Sunyaev viscosity…

astro-ph.HE2011★ 25 cited

Effects of Compton Cooling on the Hydrodynamic and the Spectral Properties of a Two Component Accretion Flow around a Black Hole

Himadri Ghosh, Sudip K. Garain, Kinsuk Giri +1

We carry out a time dependent numerical simulation where both the hydrodynamics and the radiative transfer are coupled together. We consider a two-component accretion flow in which…

astro-ph.HE2009★ 35 cited

Hydrodynamic Simulations of Oscillating Shock Waves in a Sub-Keplerian Accretion Flow Around Black Holes

Kinsuk Giri, Sandip K. Chakrabarti, Madan M. Samanta +1

We study the accretion processes on a black hole by numerical simulation. We use a grid based finite difference code for this purpose. We scan the parameter space spanned by the sp…