Gamma-ray polarization of synchrotron-self-Compton process from a highly relativistic jet
arXiv:1407.1651 · doi:10.1088/0004-637X/795/1/36
Abstract
The high polarization observed in the prompt phase of some gamma-ray bursts (GRBs) arouses extensive studies on the emission mechanism. In this paper, we investigate the polarization properties of the synchrotron-self-Compton (SSC) process from a highly relativistic jet. A magnetic-dominated, baryon-loaded jet ejected from the central engine travels with a large Lorentz factor. Shells with slightly different velocities collide with each other and produce shocks. The shocks accelerate electrons to power-law distribution, and at the same time, magnify the magnetic field. Electrons move in the magnetic field and produce synchrotron photons. The synchrotron photons suffer from the Compton scattering (CS) process and then are detected by an observer locating slightly off-axis. We derive analytically the formulae of photon polarization in the SSC process in two magnetic configurations: magnetic field in the shock plane and perpendicular to the shock plane. We show that photons induced by the SSC process can be highly polarized, with the maximum polarization in the energy band MeV. The polarization depends on the viewing angles, peaking in the plane perpendicular to the magnetic field. In the energy band MeV, in which most -ray polarimeters are active, the polarization is about twice of that in the Thomson limit, reaching to . This implies that the Klein-Nishina effect, which is often neglected in literatures, should be carefully considered.
14 pages, 4 figures
References in corpus (5)
- The Internal-Collision-Induced Magnetic Reconnection and Turbulence (ICMART) Model of Gamma-Ray Bursts
- Ten per cent polarized optical emission from GRB 090102
- Polarisation studies of the prompt gamma-ray emission from GRB 041219a using the Spectrometer aboard INTEGRAL
- Circular polarization in the optical afterglow of GRB 121024A
- X-ray Polarization in Relativistic Jets
Cited by in corpus (3)
- Gamma-ray burst polarization reduction induced by the Lorentz invariance violation
- Monte-Carlo Applications for Partially Polarised Inverse External-Compton Scattering (MAPPIES) -- I. Description of the code and First Results
- Polarization of gamma-ray burst afterglows in the synchrotron self-Compton process from a highly relativistic jet