Self-organized critical characteristics of teraelectronvolt photons from GRB 221009A

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2025-01-28 DOI:10.1051/0004-6361/202453174
Wen-Long Zhang, Shuang-Xi Yi, Yuan-Chuan Zou, Fa-Yin Wang, Cheng-Kui Li, Sheng-Lun Xie
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Abstract

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.
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来自GRB 221009A的太电子伏光子的自组织临界特性
GRB 221009A的高能余辉,被称为“有史以来最亮的”(BOAT),在之前的研究中已经被彻底分析过。本文对lhaso - km2a观测到的172个TeV的BOAT光子的等待时间行为进行了统计分析。得到以下结果:(1)光子的等待时间分布偏离指数分布。(II)这些光子的行为表现出类似于自组织临界系统的特征,如WTD中的幂律分布和尺度不变性特征。等待时间的幂律分布与非平稳过程的预测一致。(III) WTD的幂律斜率与Tsallis q-高斯分布的尺度不变特征之间的关系偏离了现有理论。我们认为这种偏差是由于光子不是完全相互独立的。总之,在这些光子中观察到的幂律和无标度特征意味着GRB 221009A产生太电子伏特光子的自组织临界过程。在其他相关研究的基础上,我们提出部分磁主导元件的参与和中央发动机的持续能量注入可以导致太电子伏余辉的产生偏离简单的外部冲击主导过程,从而表现出上述自组织临界特性。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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