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

17 citations · 17 across the 8 of their papers we have counts for

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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.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…