Possible Accretion Disk Origin of the Emission Variability of a Blazar Jet
Ritaban Chatterjee, Agniva Roychowdhury (Presidency University,, Kolkata), Sunil Chandra (North-West University, Potchefstroom), Atreyee Sinha, (AstroParticule et Cosmologie, Paris)

TL;DR
This study analyzes X-ray variability in the blazar Mrk 421, revealing a break in its power spectral density that suggests a connection between accretion disk processes and jet emission, similar to other black hole systems.
Contribution
It provides evidence for a potential disk-jet connection in blazars by identifying a characteristic timescale in X-ray variability linked to accretion disk properties.
Findings
X-ray PSD of Mrk 421 shows a break with a steeper slope below the timescale.
The break timescale is comparable to those in other black hole systems, indicating a universal property.
Results support the hypothesis that accretion disk variations influence jet emission in blazars.
Abstract
We analyze X-ray light curves of the blazar Mrk 421 obtained from the Soft X-ray Imaging Telescope and the Large Area X-Ray Proportional Counter instrument onboard the Indian space telescope and archival observations from . We show that the X-ray power spectral density (PSD) is a piece-wise power-law with a break, i.e., the index becomes more negative below a characteristic "break-timescale". Galactic black hole X-ray binaries and Seyfert galaxies exhibit a similar characteristic timescale in their X-ray variability that is proportional to their respective black hole mass. X-rays in these objects are produced in the accretion disk or corona. Hence, such a timescale is believed to be linked to the properties of the accretion flow. Any relation observed between events in the accretion disk and those in the jet can be used to characterize the disk-jet connection. However,…
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