Influence of Energy-Dependent Particle Diffusion on the X-ray spectral curvature of MKN 421
Pranjupriya Goswami, Sunder Sahayanathan, Atreyee Sinha, Ranjeev, Misra, Rupjyoti Gogoi

TL;DR
This study models the X-ray spectral curvature of blazar MKN 421 using an energy-dependent electron diffusion model, revealing correlations between physical parameters and observed spectral features, thus providing physical insights into flux variations.
Contribution
It introduces an analytical model linking electron energy-dependent diffusion to X-ray spectral shape, offering a physical interpretation beyond empirical descriptions.
Findings
Significant correlation between model parameters and observational data.
Strong anti-correlation among spectral shape parameters.
Flux variations may originate from a specific physical process.
Abstract
The X-ray spectral curvature of blazars is traditionally explained by an empirical log-parabola function characterized by three parameters, namely the flux, curvature and spectral index at a given energy. Since their exact relationship with the underlying physical quantities is unclear, interpreting the physical scenario of the source through these parameters is difficult. To attain an insight on the X-ray spectral shape, we perform a detailed study of the X-ray spectra of the blazar MKN 421, using an analytical model where the electron diffusion from the particle acceleration site is energy-dependent. The resultant synchrotron spectrum is again determined by three parameters, namely, the energy index of the escape time scale, the quantity connecting the electron energy to the observed photon energy and the normalization. The X-ray observations of MKN 421, during July 2012 - April 2013…
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