A fast radio burst cyclone in technicolour: evidence of plasma lensing
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arXiv
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| Autores principales: | , , , , , , , , , , , |
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| Formato: | Preprint |
| Publicado: |
2026
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| _version_ | 1866914336833798144 |
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| author | Uttarkar, Pavan A. Shannon, Ryan M. Gourdji, Kelly Deller, Adam T. Kumar, Pravir Sridhar, Navin Lower, Marcus E. Tuntsov, Artem Kulkarni, Atharva D. Ho, Simon C. -C. Wang, Yuanming Jahns-Schindler, Joscha N. |
| author_facet | Uttarkar, Pavan A. Shannon, Ryan M. Gourdji, Kelly Deller, Adam T. Kumar, Pravir Sridhar, Navin Lower, Marcus E. Tuntsov, Artem Kulkarni, Atharva D. Ho, Simon C. -C. Wang, Yuanming Jahns-Schindler, Joscha N. |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2602_16409 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | A fast radio burst cyclone in technicolour: evidence of plasma lensing Uttarkar, Pavan A. Shannon, Ryan M. Gourdji, Kelly Deller, Adam T. Kumar, Pravir Sridhar, Navin Lower, Marcus E. Tuntsov, Artem Kulkarni, Atharva D. Ho, Simon C. -C. Wang, Yuanming Jahns-Schindler, Joscha N. High Energy Astrophysical Phenomena 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. |
| title | A fast radio burst cyclone in technicolour: evidence of plasma lensing |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2602.16409 |