Probing shock acceleration in BL Lac jets through X-ray polarimetry: the time-dependent view
F. Tavecchio, M. Landoni, L. Sironi, P. Coppi

TL;DR
This paper models the time-dependent X-ray polarization in BL Lac jets to understand particle acceleration mechanisms, predicting a high, stable polarization in X-rays and complex variability in optical polarization during flares.
Contribution
It extends previous stationary shock models to non-stationary, variable conditions in BL Lacs, providing testable predictions for upcoming X-ray polarimetry missions.
Findings
Predicted high (~40%) stable polarization in X-ray band.
Observed complex polarization behavior during optical flares.
Anticipated polarization rotation coincides with zero polarization moments.
Abstract
Polarimetric measurements, especially if extended at high energy, are expected to provide important insights into the mechanisms underlying the acceleration of relativistic particles in jets. In a previous work we have shown that the polarization of the synchrotron X-ray emission produced by highly energetic electrons accelerated by a mildly relativistic shock carries essential imprints of the geometry and the structure of the magnetic fields in the downstream region. Here we present the extension of our analysis to the non-stationary case, especially suitable to model the highly variable emission of high-energy emitting BL Lacs. We anticipate a large (), almost time-independent degree of polarization in the hard/medium X-ray band, a prediction soon testable with the upcoming mission {\it IXPE}. The situation in other bands, in particular in the optical, is more…
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