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Updated: Jul 27, 2025

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20 mJ, 1 ps Yb:YAG Thin-disk Regenerative Amplifier
Published on: July 12, 2017
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在极其明亮的玛射线爆发中,从一个狭窄的喷射中发出特拉电子伏特后照
, Zhen Cao1,2,3, F Aharonian4,5
1Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
概括
大高空淋浴天文台 (LHAASO) 探测到了221009A马射线爆发的早期特拉电子伏特 (TeV) 后照. 这种观测为这些强大的宇宙事件的喷气结构和能量提供了新的见解.
科学领域:
- 高能天体物理学
- 宇宙射线物理
- 马射线天文学
背景情况:
- 马射线爆发是宇宙中最明亮的爆炸.
- 一些GRB呈现特拉电子伏特 (TeV) 后照,但它们的早期阶段在很大程度上未被观察到.
- 对于探测极端天体物理环境至关重要.
研究的目的:
- 报告从GRB早期出现的TeV后光的第一次观察.
- 描述来自GRB 221009A的TeV辐射的时间演变.
- 调查导致GRB的相对论喷流的特性.
主要方法:
- 使用大型高空淋浴天文台 (LHAASO) 进行广泛的淋浴探测.
- 在LHAASO的视野中观察到GRB 221009A.
- 在最初的3000秒内检测到超过0.2 TeV的64,000个光子.
主要成果:
- 在GRB触发后几分钟发现了显著的TeV流.
- 观测到TeV流的快速上升,大约10秒后达到峰值.
- 确定了随后的衰变阶段,在峰值后的650秒左右加速衰变.
- 观察到的辐射与相对论喷气模型的一致,半开放角度为0.8°.
结论:
- GRB 221009A的早期TeV后照提供了即时高能发射的直接证据.
- 观察到的特征表明排放源自结构喷气的核心.
- 这一发现有助于解释 GRB 观察到的异常高同位素能量.
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