On the statistical characterization of the synchrotron multi-zone polarization of blazars
arXiv:2510.05324 · doi:10.1051/0004-6361/202556802
Abstract
Multiwavelength polarimetric observations of blazars reveal complex, energy-dependent polarization behavior, including a decrease in polarization fraction from X-rays to millimeter bands and significant variability in the electric vector position angle (EVPA). These trends challenge simple single-zone synchrotron models and suggest a more intricate, turbulent jet structure with multiple emission zones. We develop a statistical framework to model the observed energy-dependent polarization patterns in blazars, focusing on the behavior captured by IXPE in the X-ray band and RoboPol in the optical. The goal is to statistically characterize multi-zone models in terms of the distributions of cell size and the physical parameters of the electron energy distribution (EED). A Monte Carlo approach, implemented with the JetSeT code, is used to generate synthetic multi-zone synchrotron emission from a spherical region filled with turbulent cells with randomly distributed physical properties. Simulations explore scenarios ranging from identical cells to power-law distributions of cell sizes and EED parameters with variable cutoff and low-energy slopes. The results show that a purely turbulent, multi-zone model can reproduce the observed energy-dependent polarization without requiring correlations between cell size and EED parameters. The polarization degree is primarily determined by the effective, flux-weighted, number of emitting cells, modulated by the dispersion in cell properties, particularly the EED cutoff energy at high frequencies and the low-energy spectral index at low frequencies. With a fractional dispersion in cutoff energy of about 90% and a low-energy spectral index dispersion of ~0.5-1.5, the model reproduces the chromatic mm-to-X-ray polarization trends seen by IXPE and the optical polarization limiting envelope observed in the RoboPol dataset.
published in A&A (final version after language editing and proofs)
References in corpus (16)
- Unified Schemes for Radio-Loud Active Galactic Nuclei
- The Spectral Energy Distribution of Fermi bright blazars
- Leptonic and Hadronic Modeling of Fermi-Detected Blazars
- Turbulent, Extreme Multi-Zone Model for Simulating Flux and Polarization Variability in Blazars
- Swift observations of the very intense flaring activity of Mrk 421 during 2006: I. Phenomenological picture of electron acceleration and predictions for the MeV/GeV emission
- Stochastic Acceleration and the Evolution of Spectral Distributions in SSC Sources: A Self Consistent Modeling of Blazars' Flares
- Plasmoids in relativistic reconnection, from birth to adulthood: first they grow, then they go
- Polarized Blazar X-rays imply particle acceleration in shocks
- RoboPol: The optical polarization of gamma-ray--loud and gamma-ray--quiet blazars
- The RoboPol optical polarization survey of gamma-ray - loud blazars
- The RoboPol Pipeline and Control System
- Quasar Luminosity Function at z = 7
- X-ray Polarization Observations of BL Lacertae
- The Polarization Behavior of Relativistic Synchrotron Self-Compton Jets
- IXPE observation of PKS 2155-304 reveals the most highly polarized blazar
- A Model for Nonthermal Particle Acceleration in Relativistic Magnetic Reconnection