Filamentation of Fast Radio Bursts in magnetar winds
arXiv:2112.07017 · doi:10.1093/mnras/stac251
Abstract
Magnetars are the most promising progenitors of Fast Radio Bursts (FRBs). Strong radio waves propagating through the magnetar wind are subject to non-linear effects, including modulation/filamentation instabilities. We derive the dispersion relation for modulations of strong waves propagating in magnetically-dominated pair plasmas focusing on dimensionless strength parameters , and discuss implications for FRBs. As an effect of the instability, the FRB radiation intensity develops sheets perpendicular to the direction of the wind magnetic field. When the FRB front expands outside the radius where the instability ends, the radiation sheets are scattered due to diffraction. The FRB scattering timescale depends on the properties of the magnetar wind. In a cold wind, the typical scattering timescale is at the frequency . The scattering timescale increases at low frequencies, with the scaling . The frequency-dependent broadening of the brightest pulse of FRB 181112 is consistent with this scaling. From the scattering timescale of the pulse, one can estimate that the wind Lorentz factor is larger than a few tens. In a warm wind, the scattering timescale can approach . Then scattering produces a frequency modulation of the observed intensity with a large bandwidth, . Broadband frequency modulations observed in FRBs could be due to scattering in a warm magnetar wind.
Section 3 is modified. Accepted for publication in MNRAS
References in corpus (10)
- A bright millisecond radio burst of extragalactic origin
- A fast radio burst associated with a Galactic magnetar
- A bright millisecond-duration radio burst from a Galactic magnetar
- Fast Radio Burst Discovered in the Arecibo Pulsar ALFA Survey
- A Second Source of Repeating Fast Radio Bursts
- Observations of Fast Radio Bursts at Frequencies down to 400 Megahertz
- Spectropolarimetric analysis of FRB 181112 at microsecond resolution: Implications for Fast Radio Burst emission mechanism
- Coherent Electromagnetic Emission from Relativistic Magnetized Shocks
- The synchrotron maser emission from relativistic magnetized shocks: Dependence on the pre-shock temperature
- Self-modulation of Fast Radio Bursts
Cited by in corpus (9)
- The Physics of Fast Radio Bursts
- Linearly-polarized Coherent Emission from Relativistic Magnetized Ion-electron Shocks
- Saturation of the filamentation instability and dispersion measure of Fast Radio Bursts
- Escape of fast radio bursts from magnetars
- Relativistic Collisionless Shocks in Inhomogeneous Magnetized Plasmas
- The Northern Cross Fast Radio Burst project IV. Multi-wavelength study of the actively repeating FRB 20220912A
- Kinetic Simulations of the Filamentation Instability in Pair Plasmas
- Fast Radio Bursts from non-resonant Alfvén waves and synchrotron maser emission in the magnetar wind
- Filamentation of the electromagnetic precursor in relativistic quasi-perpendicular electron-positron shocks