A fast radio burst cyclone in technicolour: evidence of plasma lensing

TL;DR

This paper presents extensive observations of the repeating FRB 20240114A, revealing extreme spectral and temporal variability consistent with plasma lensing effects, which may explain diversity in FRB activity and energetics.

Contribution

It provides the first ultrawideband, high-repetition observations of a repeating FRB, demonstrating plasma lensing as a key factor in burst variability.

Findings

Detected 5526 bursts from FRB 20240114A with extreme variability.

Observed broadband frequency shifts over months and narrowband correlations.

Evidence suggests plasma lensing influences burst properties.

Abstract

Fast radio bursts (FRBs) are bright, energetic, radio pulses of extragalactic origin. A dichotomy has emerged in the population: some produce repeat bursts, while the majority do not. Most repeating sources only show rare repetitions, and none have been studied extensively over the wide bandwidths necessary to disentangle the physical processes that produce emission from distortions to bursts caused by intervening ionised gas. Here we present radio observations of the most active repeating source, FRB 20240114A. Using an ultrawideband receiving system, we have detected 5526 repetitions, revealing an extreme spectral and temporal variability in the burst emission. The bursts exhibit longer-term broadband variations in central emission frequency over multiple months, and narrowband bursts that have correlations in central frequencies on time scales of milliseconds to minutes. The spectral and temporal properties are consistent with the source undergoing magnification by foreground plasma lenses, potentially embedded in a turbulent circumsource medium. This extreme example highlights the role of plasma lenses in the observed properties of burst emission and can explain the diversity in activity and energetics of the entire FRB population.