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arXiv · 2012.09495

Origin of Strong Linear Polarization from Fast Radio Bursts

Runna Wang·Siming Liu·Anda Xiong·Qi-Hui Chen·Fengrong Zhu
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Abstract

The detection of almost 100% linearly polarized emission from the fast radio burst source FRB 121102 implies coherent emission of relativistic electrons moving in perpendicular to the ambient magnetic field. The origin of such a particle distribution is very intriguing. Given that FRB 121102 is likely driven by a neutron star, we explored orbits of charged particles trapped in a dipole magnetic field (the Störmer problem). Most previous studies focused on particles with relatively low energies so that the guiding center approximation may be applied. High energy particles usually have chaotic orbits except those on a periodic orbit or near stable periodic orbits. Via evaluation of the maximum Lyapunov exponent of orbits of particles launched from the equatorial plane with an axial velocity (the angular velocity sets the length and energy scales of the system), we found prominent regions of quasi-periodic orbits around stable periodic orbits in the equatorial plane at high-energies. Particles in these orbits oscillate around the equatorial plane and their radial distance from the dipole can vary by a factor of/,2. Relativistic electrons in such orbits may be responsible for the almost 100% polarized emission from FRB 121102.

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Runna Wang, Siming Liu, Anda Xiong, Qi-Hui Chen, Fengrong Zhu. 2020-12-17. Origin of Strong Linear Polarization from Fast Radio Bursts. https://doi.org/10.3847/1538-4357%2Fabd704

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