activity
20222026
most citedGlobal Transonic Solution of Hot Accretion Flow with Thermal Conduction

17 citations · 33 across the 9 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2026

A Standard Ultraviolet Continuum Can Hide Supercritical Accretion in GN-z11

Samik Mitra, Ramananda Santra

The ultraviolet continuum from a high-redshift accreting black hole is routinely used to infer its mass. GN-z11 offers a sharp test of whether that inference is secure. A thin-disk…

astro-ph.HE2026

Can Isotropic Thermal Conduction Heat One of the Hottest Cool Cores?

Samik Mitra, Ramananda Santra, Norbert Werner

Thermal conduction can act as a heating mechanism for cool-core clusters, yet the same transport must erode any temperature discontinuity it crosses. Ophiuchus permits both effects…

astro-ph.HE2026

Validating Inverse Fundamental-Plane IMBH Mass Estimates in the SKA/ngVLA Era

Shahram Abbassi, Samik Mitra, Ramananda Santra

The radio/X-ray/black-hole-mass Fundamental Plane (FP) is widely used to estimate masses of accreting intermediate-mass black hole (IMBH) candidates. Its inverse use is justified o…

astro-ph.HE2026

Low-angular-momentum accretion shocks can power weak-to-moderate X-ray flares from SgrA*

Samik Mitra, Bożena Czerny, Michal Zajaček +1

X-ray flares from Sgr~A* span broad ranges in duration, fluence, and luminosity, but their origin remains unsettled. We test whether standing shocks in low-angular-momentum magneti…

astro-ph.HE2026

Thermal Stability of Radiation-Pressure-Dominated Accretion Disks Threaded by Net Vertical Magnetic Flux

Shahram Abbassi, Armin Memarian, Samik Mitra

The classical radiation-pressure instability predicts strong thermal variability in luminous black-hole accretion disks, whereas most disk-dominated X-ray binary soft states remain…

astro-ph.GA2026

Traversing the Galactic Centre in space and time

Michal Zajaček, Bożena Czerny, Martin Mondek +5

The Galactic Center is often identified with its central supermassive black hole, Sgr A*. Yet the black hole governs gravitationally only the innermost few parsecs of the Milky Way…

astro-ph.HE2025

Properties of low angular momentum general relativistic MHD accretion flows around black holes

Samik Mitra

In this proceeding, we provide a novel approach to study the General Relativistic Magnetohydrodynamic (GRMHD) accretion flows around rotating black holes (BHs). In doing so, we cho…

astro-ph.HE2024

Low angular momentum general relativistic magnetohydrodynamic accretion flow around rotating black holes with shocks

Samik Mitra, Santabrata Das

We investigate the global structure of general relativistic magneto-hydrodynamic (GRMHD) accretion flows around Kerr black holes containing shock waves, where the disk is threaded…

astro-ph.HE2023

Accretion flows around spinning compact objects in the post-Newtonian regime

Elham Nazari, Samik Mitra, Shahram Abbassi +1

We present the structure of a low angular momentum accretion flows around rotating compact objects incorporating relativistic corrections up to the leading post-Newtonian order. To…

astro-ph.HE2023★ 17 cited

Global Transonic Solution of Hot Accretion Flow with Thermal Conduction

Samik Mitra, Sayyedeh Masoumeh Ghoreyshi, Amin Mosallanezhad +2

We examine the effect of thermal conduction on the low-angular momentum hot accretion flow (HAF) around non-rotating black holes accreting mass at very low rate. While doing so, we…

astro-ph.HE2022

On the origin of core radio emissions from black hole sources in the realm of relativistic shocked accretion flow

Santabrata Das, Anuj Nandi, C. S. Stalin +5

We study the relativistic, inviscid, advective accretion flow around the black holes and investigate a key feature of the accretion flow, namely the shock waves. We observe that th…

astro-ph.HE2022★ 16 cited

Study of general relativistic magnetohydrodynamic accretion flow around black holes

Samik Mitra, Debaprasad Maity, Indu Kalpa Dihingia +1

We present a novel approach to study the global structure of steady, axisymmetric, advective, geometrically thin, magnetohydrodynamic (MHD) accretion flow around black holes in ful…