The Polarization Behavior of Relativistic Synchrotron Jets
arXiv:1807.10732 · doi:10.3847/1538-4357/aad69d
Abstract
We describe a geometric model for synchrotron radiation from blazar jets, involving multiple emission zones with turbulent magnetic fields and a transient core with a helical B field. Including the effects of jet divergence, particle cooling and the Relativistic PA rotation (RPAR) to the observer frame, we find polarization behavior consistent with recent data from monitoring campaigns. We predict that under some circumstances multi- rotation phases should exhibit relativistically-induced steps in rate and modulation in polarization that can be helpful in pinning down the jet and . Also, RPAR enhances waveband differences that will be particularly interesting for comparing radio, optical and, soon, X-ray PA and variations.
Accepted for publication in the Astrophysical Journal
References in corpus (8)
- Probing the Inner Jet of the Quasar PKS 1510-089 with Multi-waveband Monitoring during Strong Gamma-ray Activity
- RoboPol: The optical polarization of gamma-ray--loud and gamma-ray--quiet blazars
- RoboPol: Connection between optical polarization plane rotations and gamma-ray flares in blazars
- Polarization Swings Reveal Magnetic Energy Dissipation in Blazars
- Systematic Study of Gamma-ray bright Blazars with Optical Polarization and Gamma-ray Variability
- Polarization swings in blazars
- Rapid Variability of Gamma-ray Emission from Sites near the 43 GHz Cores of Blazar Jets
- A Model of Polarisation Rotations in Blazars from Kink Instabilities in Relativistic Jets
Cited by in corpus (15)
- Polarized Blazar X-rays imply particle acceleration in shocks
- Probing Blazar Emission Processes with Optical/Gamma-ray Flare Correlations
- Frequency and Time Dependence of Linear Polarization in Turbulent Jets of Blazars
- X-ray Polarization of BL Lacertae in Outburst
- Two Flares with One Shock: the Interesting Case of 3C 454.3
- The Polarization Behavior of Relativistic Synchrotron Self-Compton Jets
- IXPE observation of PKS 2155-304 reveals the most highly polarized blazar
- Prospects for Detecting X-ray Polarization in Blazar Jets
- The Time-Dependent Distribution of Optical Polarization Angle Changes in Blazars
- The RoboPol Program: Optical Polarimetric Monitoring of Blazars
- Multiwavelength analysis and the difference in the behavior of the spectral features during the 2010 and 2014 flaring periods of the blazar 3C 454.3
- On the Radio Image of Relativistic Jets -- I. Internal Structure, Doppler Boosting, and Polarization Maps
- Testing particle acceleration in blazar jets with continuous high-cadence optical polarization observations
- Testing High-Energy Emission Models for Blazars with X-ray Polarimetry
- Probing Magnetic Fields and Acceleration Mechanisms in Blazar Jets with X-ray Polarimetry