Classification and Characteristics of Double-trigger Gamma-ray Bursts
Liang Li

TL;DR
This study systematically analyzes double-trigger gamma-ray bursts, revealing they are not a distinct class but are consistent with long GRBs that experience extended dormant periods and reactivation.
Contribution
It provides a detailed classification and comparison of double-trigger GRBs, demonstrating they are likely reactivated long GRBs rather than a separate subclass.
Findings
All sub-bursts fall within the long GRB classification region.
Double-trigger GRBs are not physically distinct but are reactivated long GRBs.
Extended dormancy and reactivation explain the double-trigger phenomenon.
Abstract
Over the past two decades, the \textit{Swift} and \textit{Fermi} missions have identified a rare class of ``double-trigger'' gamma-ray bursts (GRBs) that produce two independent trigger events. These events are characterized by a sufficiently long quiescent period during which the on-board trigger system can reset, resulting in the subsequent emission being recorded as a second independent event. Consistent sky localization confirms that both trigger events originated from the same astrophysical source. Here, we present a systematic classification and characteristics study of three such cases: GRB 091024A, GRB 110709B, and GRB 220627A. We investigate each trigger episode emission independently using standard classification diagnostics, including duration (), hardness ratio, minimum variability timescale (MVT), spectral lag (), peak energy (), and…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astronomy and Astrophysical Research · Astro and Planetary Science
