Issue |
A&A
Volume 693, January 2025
|
|
---|---|---|
Article Number | A290 | |
Number of page(s) | 5 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361/202453174 | |
Published online | 28 January 2025 |
Self-organized critical characteristics of teraelectronvolt photons from GRB 221009A
1
School of Physics and Physical Engineering, Qufu Normal University, Qufu 273165, China
2
Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
3
School of Physics, Huazhong University of Science and Technology, Wuhan 430074, China
4
School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China
5
Institute of Astrophysics, Central China Normal University, Wuhan 430079, China
⋆ Corresponding authors; yisx2015@qfnu.edu.cn, zouyc@hust.edu.cn
Received:
26
November
2024
Accepted:
19
December
2024
The very high-energy afterglow in GRB 221009A, known as the “brightest of all time” (BOAT), has been thoroughly analyzed in previous studies. In this paper, we conducted a statistical analysis of the waiting time behavior of 172 TeV photons from the BOAT observed by LHAASO-KM2A. The following results were obtained: (I) The waiting time distribution (WTD) of these photons deviates from the exponential distribution. (II) The behavior of these photons exhibits characteristics resembling those of a self-organized critical system, such as a power-law distribution and scale-invariance features in the WTD. The power-law distribution of waiting times is consistent with the prediction of a nonstationary process. (III) The relationship between the power-law slopes of the WTD and the scale-invariant characteristics of the Tsallis q-Gaussian distribution deviates from existing theory. We suggest that this deviation is due to the photons not being completely independent of each other. In summary, the power-law and scale-free characteristics observed in these photons imply a self-organized critical process in the generation of teraelectronvolt photons from GRB 221009A. Based on other relevant research, we propose that the involvement of a partially magnetically dominated component and the continuous energy injection from the central engine can lead to deviations in the generation of teraelectronvolt afterglow from the simple external shock-dominated process, thereby exhibiting the self-organized critical characteristics mentioned above.
Key words: gamma-ray burst: general / gamma-ray burst: individual: GRB 221009A
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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