The Extreme Faraday Effect in Fast Radio Bursts
arXiv:2503.20154 · doi:10.3847/2041-8213/adc55e
Abstract
Fast radio bursts (FRBs) are a type of highly-polarized, millisecond-duration electromagnetic pulses in the radio band, which are mostly produced at cosmological distances. These properties provide a natural laboratory for testing the extreme Faraday effect, a phenomenon in which two different propagation modes of a pulse separate after passing through a dense, highly ionized, and magnetized medium. We derive the critical condition (e.g., rotation measure) for the extreme Faraday effect to occur in FRBs, which exceeds the currently observed maximum value but remains within the theoretically predicted range. Some new features of FRBs (in particular, radio bursts with much shorter durations) after undergoing the extreme Faraday effect are predicted, such as sudden sign reversals of circular polarization, conspicuous frequency drifting, and emergency of extremely high circular polarization degrees. A potential application of this effect in FRBs is that, by comparing morphological differences of the two separated twin modes, one can identify the variations of plasma properties over extremely short timescales along the propagation path. Therefore, if this effect is found with future observations, it would provide a new tool for probing dense, magnetized environments near FRB sources.
11 pages, 6 figures, accepted by ApJL
References in corpus (28)
- Fast Radio Bursts
- An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102
- Fast Radio Bursts: An Extragalactic Enigma
- The First CHIME/FRB Fast Radio Burst Catalog
- Dense magnetized plasma associated with a fast radio burst
- FRB 121102 Bursts Show Complex Time-Frequency Structure
- A repeating fast radio burst associated with a persistent radio source
- The Physics of Fast Radio Bursts
- A fast radio burst source at a complex magnetised site in a barred galaxy
- The Physics of Fast Radio Bursts
- Frequency-dependent polarization of repeating fast radio bursts-implications for their origin
- CHIME/FRB Detection of the Original Repeating Fast Radio Burst Source FRB 121102
- FRB microstructure revealed by the real-time detection of FRB170827
- Magnetic field reversal in the turbulent environment around a repeating fast radio burst
- Spectropolarimetric analysis of FRB 181112 at microsecond resolution: Implications for Fast Radio Burst emission mechanism
- The Impact of a Supernova Remnant on Fast Radio Bursts
- FAST observations of an extremely active episode of FRB 20201124A: I. Burst morphology
- On the Time-Frequency Downward Drifting of Repeating Fast Radio Bursts
- Polarization Changes of Pulsars due to Wave Propagation Through Magnetospheres
- Extreme case of Faraday effect: magnetic splitting of ultrashort laser pulses in plasmas
- Temporal Scattering, Depolarization, and Persistent Radio Emission from Magnetized Inhomogeneous Environments Near Repeating Fast Radio Burst Sources
- Detection of ultra-fast radio bursts from FRB 20121102A
- Faraday Rotation Measure Variations of Repeating Fast Radio Burst Sources
- Fast radio burst source properties from polarization measurements
- Scattering variability detected from the circumsource medium of FRB 20190520B
- Dispersion and Rotation Measures from the Ejecta of Compact Binary Mergers: Clue to the Progenitors of Fast Radio Bursts
- Ninety percent circular polarization detected in a repeating fast radio burst
- Induced Polarization from Birefringent Pulse Splitting in Magnetoionic Media