29 June 2026 to 3 July 2026
EICC, Edinburgh
Europe/London timezone

Counterpart-induced millisecond-scale truncation mechanism of fast radio bursts

Not scheduled
20m
EICC, Edinburgh

EICC, Edinburgh

150 Morrison St, Edinburgh EH3 8EE
Oral Presentation Astrophysical Plasmas (BSAP)

Description

The observed millisecond-scale duration is an essential yet mysterious feature of fast radio bursts (FRBs). In this work, 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.

Author

Dr Matteo Tamburini (Max Planck Institute for Nuclear Physics)

Co-authors

Prof. Christoph H. Keitel (Max Planck Institute for Nuclear Physics) Dr Yutong He (Max Planck Institute for Nuclear Physics)

Presentation materials

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