Counterpart-Induced Millisecond-Scale Truncation Mechanism of Fast Radio Bursts
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arXiv
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| Format: | Preprint |
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2025
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| _version_ | 1866913848917753856 |
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| author | He, Yutong Keitel, Christoph H. Tamburini, Matteo |
| author_facet | He, Yutong Keitel, Christoph H. Tamburini, Matteo |
| contents | The observed millisecond-scale duration is an essential yet mysterious feature of fast radio bursts (FRBs). In this Letter, we link the observed soft gamma-ray counterpart of FRB 200428 to electron-positron pair cascades driven by Compton scattering and the Breit-Wheeler process. We demonstrate that such pair cascades can truncate FRBs to durations down to millisecond-scale, thereby establishing millisecond-scale upper bounds on their durations. The physical processes involved in the truncation mechanism occur during the propagation of FRBs after their production. Consequently, this mechanism is independent of the specific production mechanism or origin of the FRBs, suggesting that it could potentially operate in all FRBs. Our results lift the constraint on FRB production mechanisms that they must inherently generate bursts lasting only milliseconds. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2505_14413 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Counterpart-Induced Millisecond-Scale Truncation Mechanism of Fast Radio Bursts He, Yutong Keitel, Christoph H. Tamburini, Matteo High Energy Astrophysical Phenomena High Energy Physics - Phenomenology Plasma Physics The observed millisecond-scale duration is an essential yet mysterious feature of fast radio bursts (FRBs). In this Letter, we link the observed soft gamma-ray counterpart of FRB 200428 to electron-positron pair cascades driven by Compton scattering and the Breit-Wheeler process. We demonstrate that such pair cascades can truncate FRBs to durations down to millisecond-scale, thereby establishing millisecond-scale upper bounds on their durations. The physical processes involved in the truncation mechanism occur during the propagation of FRBs after their production. Consequently, this mechanism is independent of the specific production mechanism or origin of the FRBs, suggesting that it could potentially operate in all FRBs. Our results lift the constraint on FRB production mechanisms that they must inherently generate bursts lasting only milliseconds. |
| title | Counterpart-Induced Millisecond-Scale Truncation Mechanism of Fast Radio Bursts |
| topic | High Energy Astrophysical Phenomena High Energy Physics - Phenomenology Plasma Physics |
| url | https://arxiv.org/abs/2505.14413 |