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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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非常に明るいガンマ線爆発の狭いジェットからのテラ電子ボルトの余光
, 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.
まとめ
大型高空シャワー観測所 (LHAASO) は,ガンマ線爆発 (GRB) 221009Aからの初期のテラ電子ボルト (TeV) の余光を検出しました. この観測はこれらの強力な宇宙現象の ジェット構造とエネルギーについて 新たな洞察を与えてくれます
科学分野:
- 高エネルギー天体物理学
- 宇宙線物理学
- ガンマ線天文学
背景:
- ガンマ線爆発 (GRB) は 宇宙で最も明るい爆発です
- いくつかのGRBはテラ電子ボルト (TeV) の後光を放つが,その初期段階はほとんど観測されないままである.
- 極度の天体物理環境を 探査するには GRBの余分な光を理解することが重要です
研究 の 目的:
- GRBから TeVの後に発光した最初の観測を報告する.
- GRB 221009Aからの TeV 放射の時間的な進化を特徴づける.
- GRBの原因となる 相対論ジェットの性質を調査する
主な方法:
- 大規模な高空シャワー観測所 (LHAASO) を利用し,大規模な空気シャワー検出を行いました.
- LHAASOの視野内で偶然 GRB 221009Aを観測した.
- 最初の3000秒で検出された エネルギーが0.2テレボルトを超える 6万4000個の光子を分析した.
主要な成果:
- GRBのトリガーから数分後に 重要なTeVの流れが検出されました
- 10秒後にピークに達した.
- ピークから650秒後に加速した衰退を特定した.
- 観測された放射は,半開角約0.8°の相対論的ジェットモデルと一致する.
結論:
- GRB 221009Aの初期の TeV 後光は,即時の高エネルギー放射の直接的な証拠を提供します.
- 観測された特徴は 放射は構造ジェットの中心から発生することを示唆しています
- この発見は,このGRBで観測された例外的に高い同位体エネルギーを説明するのに役立ちます.
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