Broadband spectral modelling of bent jets of Active Galactic Nuclei
B. Sunder Sahayanathan

TL;DR
This thesis develops models to analyze the radiation emission from AGN jet knots and blazar jets, incorporating shock acceleration, shear acceleration, and spectral modeling to explain observed multi-wavelength spectra and features.
Contribution
It introduces a comprehensive framework combining continuous injection, shock, and shear acceleration models for AGN jets, advancing understanding of jet emission mechanisms.
Findings
X-ray emission from knots explained by continuous injection plasma model.
Limb-brightening in MKN501 attributed to shear acceleration, not large viewing angles.
Temporal emission behavior in MKN421 linked to particle acceleration mechanisms.
Abstract
In this thesis, models have been developed to study the radiation emission processes from the knots of AGN jets as well as for blazar jets. A continuous injection plasma model is developed to study the X-ray emission from the knots of sources 1136-135, 1150+497, 1354+195 and 3C 371. The knot dynamics is then studied within the framework of internal shock model. In such a scenario, knots are formed due to the collision of two successive matter blobs emitted sporadically from the central engine of AGN. Shocks, generated in such collisions, accelerate electrons to relativistic energies. These electrons subsequently emit radiation via synchrotron and/or inverse Compton processes in the radio-to-X-ray energy range. The study of M87 knots involves a two zone model where the electrons with a power-law distribution are further accelerated. The synchrotron emission from these energetic electrons…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Aerodynamics and Acoustics in Jet Flows
