activity
20092026
most citedSynchrotron radiation of self-collimating relativistic MHD jets

115 citations · 997 across the 40 of their papers we have counts for

collaborators

40 papers

astro-ph.HE2026

Simulating radio emission from flickering AGN jets: travelling shocks and hotspot brightening

Emma L. Elley, James H. Matthews, Dipanjan Mukherjee +1

We investigate the impact of flickering variability in jet power on the luminosity and morphology of radio galaxies. We use a Lagrangian particle method together with relativistic…

astro-ph.HE2024

Particles in Relativistic MHD Jets II: Bridging Jet Dynamics with Multi-waveband Non-Thermal Emission Signatures

Ravi Pratap Dubey, Christian Fendt, Bhargav Vaidya

Relativistic magnetized jets, originating near black holes, are observed to exhibit sub-structured flows. In this study, we present synthetic synchrotron emission signatures for di…

astro-ph.HE2024

Bridging Simulations of Kink Instability in Relativistic Magnetized Jets with Radio Emission and Polarisation

Nikita Upreti, Bhargav Vaidya, Amit Shukla

Relativistic outflows emanating from active galactic nuclei can extend up to kiloparsec scales in length, displaying a variety of complex morphologies. This study explores the intr…

astro-ph.HE2024★ 8 cited

Imprint of "Local Opacity" Effect in Gamma-Ray Spectrum of Blazar Jet

Sushmita Agarwal, Amit Shukla, Karl Mannheim +2

Relativistic jets from accreting supermassive black holes at cosmological distances can be powerful emitters of -rays. However, the precise mechanisms and locations responsible…

physics.space-ph2023

Global-MHD Simulations using MagPIE : Impact of Flux Transfer Events on the Ionosphere

Arghyadeep Paul, Antoine Strugarek, Bhargav Vaidya

This study presents a recently developed two-way coupled magnetosphere-ionosphere model named MagPIE that enables the investigation of the impact of flux transfer events (FTEs) on…

astro-ph.GA2023

Deciphering the morphological origins of X-shaped radio galaxies: Numerical modeling of Back-flow vs. Jet-reorientation

Gourab Giri, Bhargav Vaidya, Christian Fendt

X-shaped Radio Galaxies (XRGs) develop when certain extra-galactic jets deviate from their propagation path. An asymmetric ambient medium (Back-flow model) or complex Active Galact…